{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:YSNMWTL36IQP5NBPFCGLI343SS","short_pith_number":"pith:YSNMWTL3","schema_version":"1.0","canonical_sha256":"c49acb4d7bf220feb42f288cb46f9b94a98581f3054df9c2f6fff92ee43835a6","source":{"kind":"arxiv","id":"1510.03352","version":1},"attestation_state":"computed","paper":{"title":"Quantum Scalar Corrections to the Gravitational Potentials on de Sitter Background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"R. P. Woodard (University of Florida), Sohyun Park (KASI), Tomislav Prokopec (Utrecht University)","submitted_at":"2015-10-12T16:17:58Z","abstract_excerpt":"We employ the graviton self-energy induced by a massless, minimally coupled (MMC) scalar on de Sitter background to compute the quantum corrections to the gravitational potentials of a static point particle with a mass $M$. The Schwinger-Keldysh formalism is used to derive real and causal effective field equations. When evaluated at the one-loop order, the gravitational potentials exhibit a secular decrease in the observed gravitational coupling $G$. This can also be interpreted as a (time dependent) anti-screening of the mass $M$."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1510.03352","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-10-12T16:17:58Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"7dd3cab23266f640fcb9005a11815281420b739cb4eb5ac01cd7f5822f789d5a","abstract_canon_sha256":"3e91d47c087d6382823011aeceacb36e4ea815d4fc988d25906700c640e10a7d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:20:42.432212Z","signature_b64":"G1/S++QJ9LDZP9QadOR9Vmtyn+FUsmm4qi/xqPGYm+XgiZhzAzLRlhbIrMFh2PV+9vTmrFU2UJx5I/ypofL5Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c49acb4d7bf220feb42f288cb46f9b94a98581f3054df9c2f6fff92ee43835a6","last_reissued_at":"2026-05-18T01:20:42.431773Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:20:42.431773Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quantum Scalar Corrections to the Gravitational Potentials on de Sitter Background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"R. P. Woodard (University of Florida), Sohyun Park (KASI), Tomislav Prokopec (Utrecht University)","submitted_at":"2015-10-12T16:17:58Z","abstract_excerpt":"We employ the graviton self-energy induced by a massless, minimally coupled (MMC) scalar on de Sitter background to compute the quantum corrections to the gravitational potentials of a static point particle with a mass $M$. The Schwinger-Keldysh formalism is used to derive real and causal effective field equations. When evaluated at the one-loop order, the gravitational potentials exhibit a secular decrease in the observed gravitational coupling $G$. This can also be interpreted as a (time dependent) anti-screening of the mass $M$."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.03352","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1510.03352","created_at":"2026-05-18T01:20:42.431836+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.03352v1","created_at":"2026-05-18T01:20:42.431836+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.03352","created_at":"2026-05-18T01:20:42.431836+00:00"},{"alias_kind":"pith_short_12","alias_value":"YSNMWTL36IQP","created_at":"2026-05-18T12:29:52.810259+00:00"},{"alias_kind":"pith_short_16","alias_value":"YSNMWTL36IQP5NBP","created_at":"2026-05-18T12:29:52.810259+00:00"},{"alias_kind":"pith_short_8","alias_value":"YSNMWTL3","created_at":"2026-05-18T12:29:52.810259+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.10513","citing_title":"A Nonlocal Realization of MOND that Interpolates from Cosmology to Gravitationally Bound Systems","ref_index":3,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YSNMWTL36IQP5NBPFCGLI343SS","json":"https://pith.science/pith/YSNMWTL36IQP5NBPFCGLI343SS.json","graph_json":"https://pith.science/api/pith-number/YSNMWTL36IQP5NBPFCGLI343SS/graph.json","events_json":"https://pith.science/api/pith-number/YSNMWTL36IQP5NBPFCGLI343SS/events.json","paper":"https://pith.science/paper/YSNMWTL3"},"agent_actions":{"view_html":"https://pith.science/pith/YSNMWTL36IQP5NBPFCGLI343SS","download_json":"https://pith.science/pith/YSNMWTL36IQP5NBPFCGLI343SS.json","view_paper":"https://pith.science/paper/YSNMWTL3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.03352&json=true","fetch_graph":"https://pith.science/api/pith-number/YSNMWTL36IQP5NBPFCGLI343SS/graph.json","fetch_events":"https://pith.science/api/pith-number/YSNMWTL36IQP5NBPFCGLI343SS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YSNMWTL36IQP5NBPFCGLI343SS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YSNMWTL36IQP5NBPFCGLI343SS/action/storage_attestation","attest_author":"https://pith.science/pith/YSNMWTL36IQP5NBPFCGLI343SS/action/author_attestation","sign_citation":"https://pith.science/pith/YSNMWTL36IQP5NBPFCGLI343SS/action/citation_signature","submit_replication":"https://pith.science/pith/YSNMWTL36IQP5NBPFCGLI343SS/action/replication_record"}},"created_at":"2026-05-18T01:20:42.431836+00:00","updated_at":"2026-05-18T01:20:42.431836+00:00"}