{"as_of":"2026-08-12T21:07:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:edb8a6a13d1038ac8cec60f88308bc32dba9921e2c88ac77777cfe3a61a40aa6","coverage":[{"denominator":65,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":65,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T23:27:52.149081Z","state":"measured"},{"denominator":68,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":68,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T23:27:51.866473Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-19T05:07:04.711820Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.02519","snapshot_observed_at":"2026-08-11T23:27:51.866473Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.866473Z"},"links":{"cited_paper":"/paper/2412.02519","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:7c0946aa91bbf2b9660fae39aca8f4388e0b56254c07beac6a823936d8c98e22","observation_id":"0ba31398-3d6f-4c28-a875-c822018ab886","resolution":{"observed_at":"2026-08-11T23:27:51.866473Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.02519","snapshot_observed_at":"2026-08-10T22:24:13.300650Z","title":"Galazo Garc ´ ıa, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.02297","last_updated":"2025-05-24T13:15:22Z","snapshot_observed_at":"2026-08-11T00:20:42.464025Z","submitted_at":"2025-01-04T14:29:35Z","title":"Vortices and rotating solitons in ultralight dark matter","version":2},"reference_index":106,"source":"pdf_text","source_observed_at":"2026-08-10T22:24:13.300650Z"},"links":{"cited_paper":"/paper/2412.02519","citing_paper":"/paper/2501.02297"},"observation_digest":"sha256:1c23d09d5304a33ae8090b1119d3e5e7a743ea4afdfc3626cd981c5044c0abe3","observation_id":"2bee2e94-1218-4789-9188-ebcd2c666231","resolution":{"observed_at":"2026-08-10T22:24:13.300650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"cited_work":{"arxiv_id":"2412.02519","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.02519","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Formation of solitons and their transitions in scalar- field dark matter models with a nonpolynomial self-interaction potential","venue":null,"work_id":"91f24463-ef12-415e-bce4-6ea1b0041ce7","year":2025},"citing_paper":{"arxiv_id":"2507.08786","last_updated":"2026-04-12T09:44:59Z","snapshot_observed_at":"2026-08-12T13:54:36.467385Z","submitted_at":"2025-07-11T17:47:36Z","title":"Non-relativistic effective theories for fields with general potentials and their implications for cosmology","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-19T05:03:19.542657Z"},"links":{"cited_paper":"/paper/2412.02519","citing_paper":"/paper/2507.08786"},"observation_digest":"sha256:e3668b529c9730514cd008abfe4cdafac52f06ffec1eed67f5591767c8f9e159","observation_id":"15483dc1-5d99-492e-b912-812ee15c24c2","resolution":{"observed_at":"2026-05-19T05:07:04.713628Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2412.02519/citation-record","integrity":"/paper/2412.02519/integrity","json":"/paper/2412.02519/citation-record.json","paper":"/paper/2412.02519"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:53.058287Z","title":null,"venue":null,"work_id":"efda1462-1b19-4842-b053-9eff6784bc8f","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.871875Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:ef16aa9c307240f93c288aaa164ea61da4038ec92d4c19eda5da848e862303dc","observation_id":"cab4cc5a-9cb8-4a2e-aa24-15fbdffa51de","resolution":{"observed_at":"2026-08-11T23:27:53.062224Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:53.045683Z","title":"The Thomas- Fermi regime no longer exists and the soliton is deter- mined by the balance between gravity and the quantum pressure","venue":null,"work_id":"644474af-1cc5-4fe4-a8ba-1c4405ded9e4","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.876407Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:fe24bbb0424f1218329623d1092e882f678c564e69cb7aca1238d6d05242d771","observation_id":"b92570a0-85e6-4695-9911-10f92e556a85","resolution":{"observed_at":"2026-08-11T23:27:53.050684Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:53.004614Z","title":"(44) We recover the scaling (32)","venue":null,"work_id":"960cb07e-c0f3-4eb7-aa28-fe3e9813c652","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.889231Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:5785dbfd37a5f2723f62e1675967162ffb202db60ff2d15eda8b5521b34dc721","observation_id":"856980b6-835e-40ac-a49f-7c7087d5a686","resolution":{"observed_at":"2026-08-11T23:27:53.009111Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:53.032212Z","title":"(33) This bypasses the numerical computation of the soliton profiles and should provide the correct scalings and be- haviors","venue":null,"work_id":"bc47e57f-b999-4c07-a891-590af9982a8a","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.880673Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:8a06df0b79cb843d99ed9b9745c96571b8d492e95b50b188ed7c70d5b3489c0d","observation_id":"612f70a9-d81c-4926-a93e-f2eea6d72526","resolution":{"observed_at":"2026-08-11T23:27:53.037691Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:53.018373Z","title":"(42) Up to factors of order unity, we recover the exact result (30)","venue":null,"work_id":"25545442-9efe-4a27-a935-51d593ffeeee","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.885149Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:36f2c684f26606c1245df51bdbc1817baf19951a1a868ebc34739f4eec5a5bad","observation_id":"605bc88b-7469-44bf-8c65-7e9131d0bc84","resolution":{"observed_at":"2026-08-11T23:27:53.022935Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.07364","last_updated":"2017-03-21T18:00:12Z","snapshot_observed_at":"2026-07-06T05:34:39.701740Z","submitted_at":"2017-03-21T18:00:12Z","title":"The Waning of the WIMP? A Review of Models, Searches, and Constraints","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.07364","snapshot_observed_at":"2026-08-11T23:27:51.971654Z","title":"Arcadi, M","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.971654Z"},"links":{"cited_paper":"/paper/1703.07364","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:9ba1e4c12522b2f97d62642f38105c0da258f2cf6fb24d62ce0838f57b813bd1","observation_id":"7d0b41ab-9079-411f-8259-3ab268c4cd65","resolution":{"observed_at":"2026-08-11T23:27:51.971654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.991287Z","title":null,"venue":null,"work_id":"5dd91a08-2e1e-4194-b63b-8d9e39ad2715","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.893612Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:8c7df77fb2e031ef7a18a6cfc3cbcaff3121f95dc4c3778532ae089290c3b830","observation_id":"19b07735-f105-4adf-a1f6-fa8b02f4149f","resolution":{"observed_at":"2026-08-11T23:27:52.995564Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.978694Z","title":null,"venue":null,"work_id":"9d12facc-63a6-400b-abdb-f76fedc33ad6","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.898343Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:e5bc5b00dbcee592c400b8e92d510154179207457b8b2cc524777ebe5b48b1b5","observation_id":"97b27da1-e167-4b65-863f-480347d1c2ef","resolution":{"observed_at":"2026-08-11T23:27:52.982443Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.966981Z","title":null,"venue":null,"work_id":"f90f1323-7cf4-45c7-b80a-f52493c544ff","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.902414Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:e45e6c48889fea7eed28c910538f6f5b4948f34df6e183b6044e35c392b67efd","observation_id":"c9c7d1be-fe97-43d2-83f5-8ff43986bf46","resolution":{"observed_at":"2026-08-11T23:27:52.970907Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.953978Z","title":null,"venue":null,"work_id":"842e7d03-3201-4451-b326-c2055a43a4ed","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.906972Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:0929b24dc621eb1737dcd786ba23c42f73b36c64f90bc38df9133e0b87ff7fa3","observation_id":"09507f3f-eefa-48cd-bfa2-c3fbdfe184b9","resolution":{"observed_at":"2026-08-11T23:27:52.958069Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.941406Z","title":null,"venue":null,"work_id":"ad8b8af3-11b3-4f59-a728-4709d7458b84","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.911755Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:6db9cd747e68b596129bf22f92f6e11d08b9beca3a30bc1fbd621143c2d3a082","observation_id":"5bd616a2-15cb-4310-9241-dbd70a3edee5","resolution":{"observed_at":"2026-08-11T23:27:52.945913Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.927671Z","title":null,"venue":null,"work_id":"82eb787f-c2d6-40d9-8f95-308c1a872f4e","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.915909Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:33515a435014ab1604207499cbbcb8cfb2ed8d2c011491b7f08450f5d40470d3","observation_id":"2b6bbf56-27d7-4aec-aa85-d1cd1260b744","resolution":{"observed_at":"2026-08-11T23:27:52.932693Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.914143Z","title":"V A 1, we first set the threshold ρc = 500 to a very high value so that the self-interaction potential always takes the form Φ I = λρ","venue":null,"work_id":"e1f410dc-e26b-45c4-8e03-b6a5640997fc","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.920071Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:348f95f657e6d6a8aa29910c6b43b7d29ae54598edb15e41ca58d8b9958fa858","observation_id":"e8a3b43c-ce33-4e73-91c5-bef6a52fd815","resolution":{"observed_at":"2026-08-11T23:27:52.918824Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.901136Z","title":"9 the case of a small thresh- old, ρc = 0.5","venue":null,"work_id":"dddf0141-7ff7-4f09-ab45-36f0248694c9","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.924286Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:9e9175750a27221cc3e5fca1d0a8de8973b21fce74549526aa706666d8eac3c6","observation_id":"88901f0e-4030-42d6-a0f1-a89bd0c22f75","resolution":{"observed_at":"2026-08-11T23:27:52.905339Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.887096Z","title":null,"venue":null,"work_id":"b3242fdd-d328-4dd1-a889-daea52d1c9a0","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.928382Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:2139403500abaa7b2ad6b8ac41b7e601cdfb1f81d87fd28c7445e8ead90a852f","observation_id":"dd3a0e55-ab80-415d-98b7-e66dfd398bdf","resolution":{"observed_at":"2026-08-11T23:27:52.891888Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.874469Z","title":null,"venue":null,"work_id":"26ccb838-34f7-49f7-ad66-f72bc9be999b","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.932863Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:c6af734550821bec7eaf83a91cb6159bcb72d67a203c4ff6e98d06ca94fe30c1","observation_id":"65c6a16c-60ff-46e0-8963-5708861eaa73","resolution":{"observed_at":"2026-08-11T23:27:52.878489Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.861844Z","title":null,"venue":null,"work_id":"b22208a2-0bdc-40e2-82ef-ccc51d5dc0e5","year":null},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.936829Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:df2ddb7b037ffc0ae3b81db05cec0e96d49ae0ed9470816a7f7f82d91694a83f","observation_id":"d50389ea-f917-4647-a740-822c4e072667","resolution":{"observed_at":"2026-08-11T23:27:52.865981Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.849176Z","title":"13 the intermediate case ρc = 80","venue":null,"work_id":"f5f261f2-7cc3-4345-8498-512193b998e2","year":2000},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.941254Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:3bff64bfa40a8f2f1934ce89a01444d80f7e80f3b8fee93e1b9ad09d61beb412","observation_id":"906d3df6-4260-44c6-8c80-18afa1cacb93","resolution":{"observed_at":"2026-08-11T23:27:52.853414Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9506380","last_updated":"1995-06-22T03:59:24Z","snapshot_observed_at":"2026-08-10T06:37:51.336238Z","submitted_at":"1995-06-22T03:59:24Z","title":"Supersymmetric Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9506380","snapshot_observed_at":"2026-08-11T23:27:51.945862Z","title":"Jungman, M","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.945862Z"},"links":{"cited_paper":"/paper/hep-ph/9506380","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:990b08ecd0f369bc1e7cf2d601439ab0a7ecdec81cdf6d703cbd3edb2aa51e96","observation_id":"010fd641-a0a0-4e16-9a70-63fe9fc697cf","resolution":{"observed_at":"2026-08-11T23:27:51.945862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:51.950498Z","title":"Drees, R","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.950498Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:878e9bd3190f653de64307e1c498b1ddb067fbe978bdf5b0e523039fc628a4c8","observation_id":"d85e7ed0-d148-4df0-80ce-425486ef6f9c","resolution":{"observed_at":"2026-08-11T23:27:51.950498Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.836139Z","title":"Steigman and M","venue":null,"work_id":"25f72c5e-ae38-4faf-a594-acd5c441c33d","year":1985},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.955007Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:a9f7fa49fd5ad7d5f82b378397579915e3721916d22aa775067d6c46c1c4571a","observation_id":"6fb34651-2d32-4584-8089-040638407894","resolution":{"observed_at":"2026-08-11T23:27:52.840732Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.03026","last_updated":"2019-07-04T12:29:15Z","snapshot_observed_at":"2026-08-11T04:16:46.584587Z","submitted_at":"2019-03-07T16:24:13Z","title":"Direct Detection of WIMP Dark Matter: Concepts and Status","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.03026","snapshot_observed_at":"2026-08-11T23:27:51.961406Z","title":"Schumann, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.961406Z"},"links":{"cited_paper":"/paper/1903.03026","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:750fe5ed91759ff3cfacaec22cf349519c8a27521cbb847d7f1cee3056d302a9","observation_id":"906b0453-1d6d-43f1-890c-b2c7ac126db4","resolution":{"observed_at":"2026-08-11T23:27:51.961406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.1925","last_updated":"2014-11-07T14:17:40Z","snapshot_observed_at":"2026-07-06T03:59:52.359872Z","submitted_at":"2014-11-07T14:17:40Z","title":"Indirect Detection of WIMP Dark Matter: a compact review","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.1925","snapshot_observed_at":"2026-08-11T23:27:51.966801Z","title":"Conrad, in Interplay between Particle and Astroparti- cle physics (2014), 1411.1925","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.966801Z"},"links":{"cited_paper":"/paper/1411.1925","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:0936b0278231aa273e125f57f96eac4f277edc96ab924424a1b69d0259cacbce","observation_id":"8d89f073-5f25-40bf-8af1-8da8b2834d20","resolution":{"observed_at":"2026-08-11T23:27:51.966801Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.06268","last_updated":"2017-10-10T17:28:15Z","snapshot_observed_at":"2026-08-08T13:01:50.086509Z","submitted_at":"2017-10-10T17:28:15Z","title":"Phase transitions between dilute and dense axion stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.06268","snapshot_observed_at":"2026-08-11T23:27:52.055335Z","title":"Chavanis, Phys","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.055335Z"},"links":{"cited_paper":"/paper/1710.06268","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:4bf2d7fe7a5fd35cc9df96ba86a3fe14577ec9f07e720d0698bd494f04d0df02","observation_id":"5f871e29-284a-4f13-8b99-b2094c25d3c3","resolution":{"observed_at":"2026-08-11T23:27:52.055335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.0913","last_updated":"2013-06-04T20:03:01Z","snapshot_observed_at":"2026-08-07T08:04:31.832805Z","submitted_at":"2013-06-04T20:03:01Z","title":"Cold dark matter: controversies on small scales","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.0913","snapshot_observed_at":"2026-08-11T23:27:51.975908Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.975908Z"},"links":{"cited_paper":"/paper/1306.0913","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:26945949a68a3305f53574755ddc6f4a408d1c22740f225c8b996b4292698954","observation_id":"1a3dd5dc-ca5a-43bf-9572-b517c29c04cb","resolution":{"observed_at":"2026-08-11T23:27:51.975908Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.07790","last_updated":"2017-03-23T20:57:00Z","snapshot_observed_at":"2026-07-06T05:01:13.662899Z","submitted_at":"2016-06-24T19:01:40Z","title":"Small scale problems of the $\\Lambda$CDM model: a short review","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.07790","snapshot_observed_at":"2026-08-11T23:27:51.981331Z","title":"Del Popolo and M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.981331Z"},"links":{"cited_paper":"/paper/1606.07790","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:b9933f0e682d0a996f64108877ddd2c8a45b3da5abc4081eda57e12a204d48ff","observation_id":"dd0bacc2-81ce-4cb6-af8c-63ac8d587d4b","resolution":{"observed_at":"2026-08-11T23:27:51.981331Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.10559","last_updated":"2017-06-28T19:18:37Z","snapshot_observed_at":"2026-08-07T15:24:57.800360Z","submitted_at":"2017-03-30T16:36:08Z","title":"Shedding light on the small-scale crisis with CMB spectral distortions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.10559","snapshot_observed_at":"2026-08-11T23:27:51.986063Z","title":"Nakama, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.986063Z"},"links":{"cited_paper":"/paper/1703.10559","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:f25800b9b8322d66eaed53ce1eaee913b3eb640733e85763b4a1c94fa7c9cd0b","observation_id":"a5df6c1a-c37b-41e8-a13f-7fc868772c2f","resolution":{"observed_at":"2026-08-11T23:27:51.986063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.01100","last_updated":"2022-06-07T13:23:26Z","snapshot_observed_at":"2026-07-06T09:01:38.630614Z","submitted_at":"2020-03-02T18:51:00Z","title":"The landscape of QCD axion models","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.01100","snapshot_observed_at":"2026-08-11T23:27:51.990586Z","title":"Di Luzio, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.990586Z"},"links":{"cited_paper":"/paper/2003.01100","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:9fbe973841a3c4a3a845381361b33f904020fb59dc609267afbbddf4519185b9","observation_id":"f7dc5f56-3b4d-4151-9286-1ee5ab2c7586","resolution":{"observed_at":"2026-08-11T23:27:51.990586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0003365","last_updated":"2000-03-26T22:50:24Z","snapshot_observed_at":"2026-07-07T00:10:35.167895Z","submitted_at":"2000-03-24T00:29:30Z","title":"Cold and Fuzzy Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0003365","snapshot_observed_at":"2026-08-11T23:27:51.995206Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.995206Z"},"links":{"cited_paper":"/paper/astro-ph/0003365","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:ebffdf7950c3b4b9fd545a215efe1d0eb104ee57d08f0860b7d46c024d6bfcb1","observation_id":"e50d9907-ac1e-40fc-867d-a94cd685eeb6","resolution":{"observed_at":"2026-08-11T23:27:51.995206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.02519","snapshot_observed_at":"2026-08-11T23:27:51.866473Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.866473Z"},"links":{"cited_paper":"/paper/2412.02519","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:7c0946aa91bbf2b9660fae39aca8f4388e0b56254c07beac6a823936d8c98e22","observation_id":"0ba31398-3d6f-4c28-a875-c822018ab886","resolution":{"observed_at":"2026-08-11T23:27:51.866473Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.08297","last_updated":"2017-02-24T21:01:45Z","snapshot_observed_at":"2026-07-06T05:16:05.217762Z","submitted_at":"2016-10-26T12:25:05Z","title":"Ultralight scalars as cosmological dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.08297","snapshot_observed_at":"2026-08-11T23:27:51.999394Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:51.999394Z"},"links":{"cited_paper":"/paper/1610.08297","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:8aa72f07f792b463dd6fe7ab94b553eb267188c3509903516f46f3de62ff181e","observation_id":"de7d757e-1183-455d-a7fa-5cdc533cac75","resolution":{"observed_at":"2026-08-11T23:27:51.999394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.003906Z","title":"Goodman, New Astron","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.003906Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:5b627229784169c03f3a415a580a63910862dd8eedc67b83cf2e63f746f47500","observation_id":"679d078c-4fd7-4630-8c16-a20574ba5400","resolution":{"observed_at":"2026-08-11T23:27:52.003906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9908152","last_updated":"2000-03-23T19:38:51Z","snapshot_observed_at":"2026-08-04T12:07:10.209252Z","submitted_at":"1999-08-13T22:58:28Z","title":"Scalar Field as Dark Matter in the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9908152","snapshot_observed_at":"2026-08-11T23:27:52.008382Z","title":"Matos, F","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.008382Z"},"links":{"cited_paper":"/paper/astro-ph/9908152","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:494bae3417be6dffc20924addb4fa12788731b26da6d8fe766ccbf2ae57e2a16","observation_id":"59212afc-2cae-4f96-812d-a8a61c861364","resolution":{"observed_at":"2026-08-11T23:27:52.008382Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.6586","last_updated":"2014-06-25T14:37:53Z","snapshot_observed_at":"2026-08-06T04:45:50.540058Z","submitted_at":"2014-06-25T14:37:53Z","title":"Cosmic Structure as the Quantum Interference of a Coherent Dark Wave","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.6586","snapshot_observed_at":"2026-08-11T23:27:52.013448Z","title":"Schive, T","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.013448Z"},"links":{"cited_paper":"/paper/1406.6586","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:c0b3128620cd2ad77e61b2f16e01973315078fcfe75bbc756b4921578bae65c0","observation_id":"3e3da519-b6bc-4626-a859-fece8ea7a293","resolution":{"observed_at":"2026-08-11T23:27:52.013448Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.03254","last_updated":"2021-02-03T00:50:34Z","snapshot_observed_at":"2026-08-07T11:04:26.350563Z","submitted_at":"2020-05-07T05:22:55Z","title":"Ultra-Light Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.03254","snapshot_observed_at":"2026-08-11T23:27:52.019196Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.019196Z"},"links":{"cited_paper":"/paper/2005.03254","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:548ebcf0f714e370d823460d6abc104ec579e8d9fa09ba139e82588b87226225","observation_id":"ed95aab5-fc59-49fb-ad93-18a4c565b923","resolution":{"observed_at":"2026-08-11T23:27:52.019196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.6061","last_updated":"2014-10-29T21:51:12Z","snapshot_observed_at":"2026-08-07T06:41:47.646527Z","submitted_at":"2013-10-22T21:25:21Z","title":"Cosmological Constraints on Bose-Einstein-Condensed Scalar Field Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.6061","snapshot_observed_at":"2026-08-11T23:27:52.024385Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.024385Z"},"links":{"cited_paper":"/paper/1310.6061","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:827b3ffeeceedf58cc26234acbcd7f429b93efa87294d342d1d688bc937b5640","observation_id":"a05be3e3-14e8-4958-99b7-c21ac037d423","resolution":{"observed_at":"2026-08-11T23:27:52.024385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.029694Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.029694Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:4d418bcc498505ce50d7245d76d0229f2024a4d4b2b7cb063c103cb6896ad542","observation_id":"374dfa97-e720-4191-8a14-703017135f83","resolution":{"observed_at":"2026-08-11T23:27:52.029694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.5930","last_updated":"2015-11-11T21:00:01Z","snapshot_observed_at":"2026-07-06T04:04:03.682106Z","submitted_at":"2014-12-18T16:32:07Z","title":"Do Dark Matter Axions Form a Condensate with Long-Range Correlation?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.5930","snapshot_observed_at":"2026-08-11T23:27:52.033656Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.033656Z"},"links":{"cited_paper":"/paper/1412.5930","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:a32250a49a9990ebfd24903a81b72cea0c11c3e11c0a0cc2c2e2150257909495","observation_id":"127bb6eb-9630-4367-a41f-20e20d0f4f14","resolution":{"observed_at":"2026-08-11T23:27:52.033656Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.1106","last_updated":"2009-09-02T20:15:05Z","snapshot_observed_at":"2026-07-06T01:47:45.207581Z","submitted_at":"2009-01-08T18:44:45Z","title":"Bose-Einstein Condensation of Dark Matter Axions","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.1106","snapshot_observed_at":"2026-08-11T23:27:52.037790Z","title":"Sikivie and Q","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.037790Z"},"links":{"cited_paper":"/paper/0901.1106","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:440c56dc8deeb6968d5d744f8e574a27c53a6c750dc51775145926798f2d9989","observation_id":"43b92bc3-5475-4c7f-9e97-d70f1cb6e97b","resolution":{"observed_at":"2026-08-11T23:27:52.037790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.07633","last_updated":"2016-06-15T09:26:10Z","snapshot_observed_at":"2026-07-06T04:34:18.606343Z","submitted_at":"2015-10-26T20:14:39Z","title":"Axion Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.07633","snapshot_observed_at":"2026-08-11T23:27:52.042070Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.042070Z"},"links":{"cited_paper":"/paper/1510.07633","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:bdcc198bee8639deb82ff1dfbcd714c3e324a8b6e603633237849c9201e98542","observation_id":"df226476-7698-4a7d-bcab-16c1f6a3b9f5","resolution":{"observed_at":"2026-08-11T23:27:52.042070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.09647","last_updated":"2018-08-08T12:58:02Z","snapshot_observed_at":"2026-08-10T07:37:58.413740Z","submitted_at":"2018-04-25T16:03:05Z","title":"Formation and structure of ultralight bosonic dark matter halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.09647","snapshot_observed_at":"2026-08-11T23:27:52.046275Z","title":"Veltmaat, J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.046275Z"},"links":{"cited_paper":"/paper/1804.09647","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:c76c8d08ef058c4f7eb95f0abd9cd8dfa98d4cf0ffa45b44fd79e159b09922f7","observation_id":"1b7bec3a-45fe-436c-8f4b-ebf6891bf152","resolution":{"observed_at":"2026-08-11T23:27:52.046275Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1103.2050","last_updated":"2011-08-22T18:35:22Z","snapshot_observed_at":"2026-07-06T02:24:40.203449Z","submitted_at":"2011-03-10T14:43:39Z","title":"Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: I. Analytical results","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1103.2050","snapshot_observed_at":"2026-08-11T23:27:52.050569Z","title":"Chavanis, Phys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.050569Z"},"links":{"cited_paper":"/paper/1103.2050","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:dfd1dfe8f9ec64dc8956b9bd2013627bb29bd80fed4ec08266c1b35d7093c4aa","observation_id":"63905086-9171-4e90-9619-c4dfefc7669f","resolution":{"observed_at":"2026-08-11T23:27:52.050569Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.07043","last_updated":"2021-08-01T03:59:40Z","snapshot_observed_at":"2026-07-06T10:59:39.139457Z","submitted_at":"2021-04-14T18:00:06Z","title":"Core-Envelope Haloes in Scalar Field Dark Matter with Repulsive Self-Interaction: Fluid Dynamics Beyond the de Broglie Wavelength","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.07043","snapshot_observed_at":"2026-08-11T23:27:52.059333Z","title":"Dawoodbhoy, P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.059333Z"},"links":{"cited_paper":"/paper/2104.07043","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:25303a4fbf2eb14a20416c9a6a61e352804728d7a95877c3e753cb864df223bc","observation_id":"bac06fde-0243-49ca-87cb-304182144e02","resolution":{"observed_at":"2026-08-11T23:27:52.059333Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.13244","last_updated":"2021-11-03T04:47:57Z","snapshot_observed_at":"2026-08-10T16:52:09.147017Z","submitted_at":"2021-06-24T18:00:00Z","title":"Cosmological structure formation in scalar field dark matter with repulsive self-interaction: The Incredible Shrinking Jeans Mass","version":2},"cited_work":{"arxiv_id":"2106.13244","doi":null,"metadata_source":"pith","pith_arxiv_id":"2106.13244","snapshot_observed_at":"2026-08-11T23:27:52.377816Z","title":"Cosmological structure formation in scalar field dark matter with repulsive self-interaction: The Incredible Shrinking Jeans Mass","venue":"astro-ph.CO","work_id":"161721df-9ad8-4f8b-90bb-7b16b33865f0","year":2021},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.063616Z"},"links":{"cited_paper":"/paper/2106.13244","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:3b6229000669647feb983e243c9602bbbaf50f3059a57e3b47de454c7481a3df","observation_id":"93ead4e1-6a40-4193-b3f5-16e2d506c66d","resolution":{"observed_at":"2026-08-11T23:27:52.382547Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.067635Z","title":null,"venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.067635Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:0585c326206eddc690f9cab0de604c2f32714e9c0aedd8bccbfe4c47da176731","observation_id":"b79a0b6d-9b49-4077-b9e5-940f1d98be61","resolution":{"observed_at":"2026-08-11T23:27:52.067635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.071227Z","title":"Weinberg, Phys","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.071227Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:9dfe384307dd1d5fc03175eb808b7697133d7e5312fb512767d79644ff24379a","observation_id":"fbf73b52-3630-457d-879e-c1e80d0e76c8","resolution":{"observed_at":"2026-08-11T23:27:52.071227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.075291Z","title":"Wilczek, Phys","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.075291Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:16ff61e760eb41862fd38d303502d1f54e78c7269874f89f01d825b588d3ab9c","observation_id":"c2f3701b-3fbe-4060-9c58-911eb697738f","resolution":{"observed_at":"2026-08-11T23:27:52.075291Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.787149Z","title":null,"venue":null,"work_id":"c430b5a8-3017-47c4-98cf-4514d9343f49","year":1987},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.079199Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:0febe4dbbb3454302a7ecba1b5ddc59b75cd1d3ced285010ac6434ccc36fffe9","observation_id":"40fea0bc-fa75-455f-a672-b51591c2705d","resolution":{"observed_at":"2026-08-11T23:27:52.792687Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0803.3085","last_updated":"2008-03-23T20:25:21Z","snapshot_observed_at":"2026-07-06T01:37:52.114941Z","submitted_at":"2008-03-21T16:26:35Z","title":"Monodromy in the CMB: Gravity Waves and String Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.3085","snapshot_observed_at":"2026-08-11T23:27:52.082964Z","title":"Silverstein and A","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.082964Z"},"links":{"cited_paper":"/paper/0803.3085","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:4f419df94dec5c95e44ea0bb3e9a190d84340490ecdf89c71c49ae4f02e686a8","observation_id":"783a2816-5975-4d55-bea9-a7a3fcd5d681","resolution":{"observed_at":"2026-08-11T23:27:52.082964Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.0706","last_updated":"2008-08-05T20:00:25Z","snapshot_observed_at":"2026-07-06T01:40:51.680937Z","submitted_at":"2008-08-05T19:44:50Z","title":"Gravity Waves and Linear Inflation from Axion Monodromy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.0706","snapshot_observed_at":"2026-08-11T23:27:52.087137Z","title":"McAllister, E","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.087137Z"},"links":{"cited_paper":"/paper/0808.0706","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:c341d1cfbfbecc98d76bc1903fb18de6486134ea34a533cd8e6477b1acdcd68f","observation_id":"14eac8c3-808a-4e95-84bc-42bd773a4f5c","resolution":{"observed_at":"2026-08-11T23:27:52.087137Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.00730","last_updated":"2019-08-22T08:57:54Z","snapshot_observed_at":"2026-07-06T07:57:29.321260Z","submitted_at":"2019-06-03T12:10:54Z","title":"Impact of kinetic and potential self-interactions on scalar dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.00730","snapshot_observed_at":"2026-08-11T23:27:52.091367Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.091367Z"},"links":{"cited_paper":"/paper/1906.00730","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:9ac3d610858233558a027bf858c973963ee31442b90ccbfc2b79e7cd1bc087ad","observation_id":"2121625d-14f2-4e19-9064-5fe26d5d4c09","resolution":{"observed_at":"2026-08-11T23:27:52.091367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.095817Z","title":"Madelung, Z","venue":null,"work_id":null,"year":1927},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.095817Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:a28d679afa654444e82660e6e28d3b4d23f34d4fc6443f461ea12f4c17a1e065","observation_id":"c77fca79-45ac-44bf-a740-2874f2f0f848","resolution":{"observed_at":"2026-08-11T23:27:52.095817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1103.2054","last_updated":"2011-08-22T19:13:20Z","snapshot_observed_at":"2026-08-08T08:08:59.979586Z","submitted_at":"2011-03-10T15:08:49Z","title":"Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: II. Numerical results","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1103.2054","snapshot_observed_at":"2026-08-11T23:27:52.099434Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.099434Z"},"links":{"cited_paper":"/paper/1103.2054","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:cf870bfe7819437a637ac9e1df95dd85a547171c21f0fde3e94edf9615cdc378","observation_id":"1ab4ac0d-0e0f-4292-8731-f08f98af3b85","resolution":{"observed_at":"2026-08-11T23:27:52.099434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1101.3655","last_updated":"2011-02-10T04:20:49Z","snapshot_observed_at":"2026-07-06T02:22:15.104916Z","submitted_at":"2011-01-19T10:36:11Z","title":"Evolution of cosmological perturbations in Bose-Einstein condensate dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.3655","snapshot_observed_at":"2026-08-11T23:27:52.103481Z","title":"Harko, Mon","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.103481Z"},"links":{"cited_paper":"/paper/1101.3655","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:09f307077a61bbe6936a32c42cc22f990bd73bceadef2020ca6c26856d96d572","observation_id":"6869b293-3ca7-4219-8270-6ebe59c8b561","resolution":{"observed_at":"2026-08-11T23:27:52.103481Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.04638","last_updated":"2020-11-12T10:37:50Z","snapshot_observed_at":"2026-07-06T09:36:49.009695Z","submitted_at":"2020-07-09T08:40:48Z","title":"Non-Relativistic Formation of Scalar Clumps as a Candidate for Dark Matter","version":3},"cited_work":{"arxiv_id":"2007.04638","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.04638","snapshot_observed_at":"2026-08-11T23:27:52.293878Z","title":"Non-Relativistic Formation of Scalar Clumps as a Candidate for Dark Matter","venue":"astro-ph.CO","work_id":"ab012152-dc36-40f3-b4d3-a406f32759e5","year":2020},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.107441Z"},"links":{"cited_paper":"/paper/2007.04638","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:e463419112251ead5e38cceeb9d3b584bd1549f4f307e65ae6567051e3f15d7c","observation_id":"a45437f9-cbfc-4ea9-af71-5b7eaaf4d5a3","resolution":{"observed_at":"2026-08-11T23:27:52.301192Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.02320","last_updated":"2018-04-06T07:57:36Z","snapshot_observed_at":"2026-07-06T06:17:34.819413Z","submitted_at":"2018-01-08T06:44:09Z","title":"Self-consistent construction of virialized wave dark matter halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.02320","snapshot_observed_at":"2026-08-11T23:27:52.111559Z","title":"Lin, H.-Y","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.111559Z"},"links":{"cited_paper":"/paper/1801.02320","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:88cb8539e45a020e05f414d445de4c777a71b751d6aff0edf799c7fc75d62b00","observation_id":"26e23500-0fa0-4566-a097-3f4992d75ef6","resolution":{"observed_at":"2026-08-11T23:27:52.111559Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.06125","last_updated":"2023-01-05T19:54:24Z","snapshot_observed_at":"2026-07-06T11:47:13.744987Z","submitted_at":"2021-09-13T17:03:17Z","title":"Construction of Wave Dark Matter Halos: Numerical Algorithm and Analytical Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.06125","snapshot_observed_at":"2026-08-11T23:27:52.115763Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.115763Z"},"links":{"cited_paper":"/paper/2109.06125","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:c8eb1e08758f0e388b4fe66abdb827fbc1a101261afb97aa84205d0fead0e39d","observation_id":"596338da-09aa-4ed5-ad93-87dfbcbfd2c3","resolution":{"observed_at":"2026-08-11T23:27:52.115763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.764933Z","title":"Binney and S","venue":null,"work_id":"69a48f6c-6ec3-42f6-a781-e98d3a9d13be","year":2008},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.119954Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:2deb3f63471d2c0d868e9e7755c46ffc35182117a086d3d05a806fbd300f96fd","observation_id":"46393341-d571-4274-b846-b5fe08d19310","resolution":{"observed_at":"2026-08-11T23:27:52.769258Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.123683Z","title":"Pathria and J","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.123683Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:acfdb835139fa63ceb151c47e463d9236880cb419225af029d97c380fdeb1478","observation_id":"331cc734-8676-4a7d-89eb-1899acc97b03","resolution":{"observed_at":"2026-08-11T23:27:52.123683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T23:27:52.127422Z","title":"Zhang and M","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.127422Z"},"links":{"citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:ab8939117ef4d99d188966d1deff919d7a58bda5f8e19a16ae8df12b23d0ea6f","observation_id":"d9f242f7-6bb7-410c-a2b9-5976742db216","resolution":{"observed_at":"2026-08-11T23:27:52.127422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.04037","last_updated":"2018-10-16T22:46:27Z","snapshot_observed_at":"2026-08-10T06:42:51.015654Z","submitted_at":"2018-07-11T09:38:23Z","title":"PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.04037","snapshot_observed_at":"2026-08-11T23:27:52.131766Z","title":"Edwards, E","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.131766Z"},"links":{"cited_paper":"/paper/1807.04037","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:29f20e77c91d2b8376a8bcfdf2ddf22ffc5344d8d453e6dc68e2afc271be76e9","observation_id":"2d1038f8-2baf-4e3f-8120-e7de342a5fd2","resolution":{"observed_at":"2026-08-11T23:27:52.131766Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.10221","last_updated":"2024-02-06T09:58:56Z","snapshot_observed_at":"2026-08-03T13:22:20.098910Z","submitted_at":"2023-04-20T11:35:41Z","title":"Solitons and halos for self-interacting scalar dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.10221","snapshot_observed_at":"2026-08-11T23:27:52.135805Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.135805Z"},"links":{"cited_paper":"/paper/2304.10221","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:da5cc6cc175642e50ac08d2be3f101e29508fb3a5670572e8415f01b52a861de","observation_id":"e7d6af8f-d1d6-4832-a425-f826bf3c4f4b","resolution":{"observed_at":"2026-08-11T23:27:52.135805Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.05857","last_updated":"2018-09-20T18:00:06Z","snapshot_observed_at":"2026-08-10T12:30:43.768717Z","submitted_at":"2018-04-16T18:00:09Z","title":"Gravitational Bose-Einstein condensation in the kinetic regime","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.05857","snapshot_observed_at":"2026-08-11T23:27:52.139906Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.139906Z"},"links":{"cited_paper":"/paper/1804.05857","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:a0bfa9d09528510bedb85ec402517c2608861f742a06852bcbd1fa1b279fc7eb","observation_id":"a2bc70e1-f3d7-491f-a644-2576054c4aee","resolution":{"observed_at":"2026-08-11T23:27:52.139906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.04057","last_updated":"2023-04-25T00:58:46Z","snapshot_observed_at":"2026-08-02T02:34:36.249439Z","submitted_at":"2022-07-08T18:00:00Z","title":"Condensation and Evaporation of Boson Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.04057","snapshot_observed_at":"2026-08-11T23:27:52.144082Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.144082Z"},"links":{"cited_paper":"/paper/2207.04057","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:693b17015f4d4a737d7f370147845b5b981f12005184c904e77d0a35fa89027b","observation_id":"e258c3ba-63d9-460f-9f67-1cefe3a5270d","resolution":{"observed_at":"2026-08-11T23:27:52.144082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.01985","last_updated":"2023-05-19T16:35:14Z","snapshot_observed_at":"2026-08-04T16:18:28.754747Z","submitted_at":"2023-04-04T17:41:29Z","title":"Kinetic relaxation and Bose-star formation in multicomponent dark matter- I","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.01985","snapshot_observed_at":"2026-08-11T23:27:52.149081Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-11T23:27:52.149081Z"},"links":{"cited_paper":"/paper/2304.01985","citing_paper":"/paper/2412.02519"},"observation_digest":"sha256:90a64d451e4ea6e4f67e65e12bc403e1aa06ffa4d31c71664ebfd1dadf7e8f62","observation_id":"e6689980-479b-4dcc-87ee-70b49ce1e120","resolution":{"observed_at":"2026-08-11T23:27:52.149081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.02519","last_updated":"2024-12-03T16:11:57Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-11T23:58:03.038269Z","submitted_at":"2024-12-03T16:11:57Z","title":"Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential"},"reference_resolution":{"displayed":65,"state_counts":{"malformed_identifier":6,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":50,"verified_exact":2,"verified_fuzzy":7},"total_outbound_references":65},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 65 of 65 outbound references and 3 inbound Pith citation observations for arXiv:2412.02519."}