Pith. sign in

Paper Citation Record · LEDGER

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves

As of 14 August 2026, this Paper Citation Record lists 100 of 131 outbound references and 0 inbound Pith citation observations for arXiv:2608.10100.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2608.10100 v1

Coverage vector

measured 100 of 131 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:20:56.189425Z

measured 100 of 100 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

Reference resolution

100 of 131 outbound references displayed

  • verified exact8
  • verified fuzzy0
  • unresolved91
  • parse uncertain0
  • malformed identifier1
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation b2755e63-ee02-43d3-b66e-ccdf270f0025 · outbound

This paper cites The Dynamics of Binary Neutron Star Mergers and of GW170817.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The Dynamics of Binary Neutron Star Mergers and of GW170817

Reference 1

Resolution
malformed identifier
no resolver link, observed 2026-08-14T04:20:55.606593Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.606593Z digest=sha256:c25ab316bf695031b6db0f785c1c6ba38365f3e1d9196d6867074386c0727e19

Observation 488e107d-bb8d-49ea-8dd8-875dd02033fe · outbound

This paper cites Transient Events from Neutron Star Mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Transient Events from Neutron Star Mergers

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.612448Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.612448Z digest=sha256:68d078be17b14c3255181d46292412d392fbd70487467591a2c66fa4738bf339

Observation 5404f074-fefa-4780-bddd-3e6cbd3650a9 · outbound

This paper cites an unresolved cited work.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Unresolved cited work

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.617980Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.617980Z digest=sha256:062bd467c7b2c3822b948f86019d5a0aa9df8f3255d63a0b063f6a2279341301

Observation 001a9dd2-7a88-41f3-ae21-6850826fc1b7 · outbound

This paper cites Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.623559Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.623559Z digest=sha256:b4e18d8933dfaff192b7cb02c4a28f95b7fdbf49d3259a880d4f6b9130b31812

Observation 11fb483d-5731-4cc6-b890-030f295c20ae · outbound

This paper cites Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.630787Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.630787Z digest=sha256:a83572e3075cbb989e68aa0606ad457267110d9076608e793d9fd7a1d16042b4

Observation 55d380bf-a064-4804-a69b-5640c13ff1e5 · outbound

This paper cites Properties of the binary neutron star merger GW170817.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Properties of the binary neutron star merger GW170817

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.638010Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.638010Z digest=sha256:0698a151c1b2cd096025a611bdce5554eb71bcb3f86be31fefea7a1c768b8802

Observation 671014f2-4b17-4cc4-adc1-4ffe2ead893a · outbound

This paper cites Multi-messenger Observations of a Binary Neutron Star Merger.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Multi-messenger Observations of a Binary Neutron Star Merger

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.643896Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.643896Z digest=sha256:b47e82afe692b57d9fab7aacd71d2b07031156a6753055453508547a16369b33

Observation 8b175ad6-1115-40af-87b5-5e31737c98f7 · outbound

This paper cites Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.650272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.650272Z digest=sha256:404ea044fe36207e966048e24b6115920a92e5aabfd899e9f3d1edb469601a75

Observation b1856e41-495c-4471-84d7-efd5c262587e · outbound

This paper cites Arcavi, C.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Arcavi, C

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.655820Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.655820Z digest=sha256:6903eb410e155a04237ee170fb2c054ee4eaf2b9c0ececba728a446235d9c3b4

Observation 4a792f6e-c629-4aa7-9086-4024fd397959 · outbound

This paper cites The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.661865Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.661865Z digest=sha256:473071fe6a204d0e387437bfdf74b6578bfa02aaa6467da1b8109d4a1af93658

Observation 145caba3-7db5-4ba4-8367-432914013eef · outbound

This paper cites Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.667404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.667404Z digest=sha256:00c204c2d97d687ff3d022bf5f2951fc02a3be3fda0291a6b932bdbd547bb7a2

Observation 6c3a9002-586b-4293-a232-e75997eca7d0 · outbound

This paper cites Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.672978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.672978Z digest=sha256:2387dfba6b92d010d1575026dadd530028282dd1753ab21e330eb7f385c115d8

Observation d350fb89-6917-4b9b-9506-a1b9ad90a613 · outbound

This paper cites Swift and NuSTAR observations of GW170817: detection of a blue kilonova.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Swift and NuSTAR observations of GW170817: detection of a blue kilonova

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.678876Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.678876Z digest=sha256:5f6bcb275e31dfd846491b9b2920fb68d58744683521875e1ad671296371a572

Observation 4b0b3835-553d-4f1a-834c-041359bb6673 · outbound

This paper cites Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.686656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.686656Z digest=sha256:38ad742171ca9e31f875ca481f77631cae9dc109c8a6c465201ff1313224ebda

Observation 76767a84-282f-43d0-9f70-894abebbae8c · outbound

This paper cites Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.691649Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.691649Z digest=sha256:6b388a7d49b77e0a06846f34bf7be204ec035d84ed6754db11dc5b0a5cffdaae

Observation 9c4b0c1f-ae6e-41bb-9476-71cd5b8a44d4 · outbound

This paper cites A kilonova as the electromagnetic counterpart to a gravitational-wave source.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.696468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.696468Z digest=sha256:cdfb35fdfdd3a0c5f12a007bb0e97600b7a664f5ebe3b8794c20ef76e184fc84

Observation abde3858-1388-40c9-9497-66b1f30a49b0 · outbound

This paper cites The X-ray counterpart to the gravitational wave event GW 170817.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The X-ray counterpart to the gravitational wave event GW 170817

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.701348Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.701348Z digest=sha256:5ca82352f350dfc497f1e1c1f517819087434c97a82d0302379e495caeb71863

Observation 63476646-d7cc-4b4a-a36a-9aa2f1480366 · outbound

This paper cites J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.705896Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.705896Z digest=sha256:092af070e7900e46cc3533f731c827a75ebd190f5c2c9a21083098023d92d9b1

Observation 9c861578-b2f9-41a3-98c0-d5cb8f2a9abe · outbound

This paper cites The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.713059Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.713059Z digest=sha256:a207a803bd0b6034d0c1b44d4f078995e75fc2ebdd0b7b5d82d648a921926198

Observation fae4210f-2249-4bde-b970-7c92230c5689 · outbound

This paper cites The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.719612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.719612Z digest=sha256:95689a7bc39912a7081f3ef51f3571744e11d3b60beebc1d59086ce8d6852e15

Observation 1c4ec2d0-8e76-4cf7-9098-d9afc2838287 · outbound

This paper cites Neutron Star Merger Remnants.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Neutron Star Merger Remnants

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.725230Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.725230Z digest=sha256:b0fc79c6beec0bbde4e28cdc32b8b523a8d1b4fd070283e3bb5db07863be4072

Observation b67e452d-43f8-4b34-9713-6b12eb6ed607 · outbound

This paper cites Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts and Nucleosynthesis.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts and Nucleosynthesis

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.730244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.730244Z digest=sha256:ff98a35dfbc394d40b6dfccb19d2d55671872727979199f280e9361ca389871c

Observation 83bbcb5c-bd13-4b10-90d2-45651add061d · outbound

This paper cites Mass ejection in neutron star mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Mass ejection in neutron star mergers

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.735334Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.735334Z digest=sha256:d7ee1815704c533d085fbf5399809acea115a19248b5463eef89319c43233afe

Observation c73ff12c-767e-48e1-be75-a6475d707a92 · outbound

This paper cites Rosswog, Philosophical Transactions A373, 2036 (2013).

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Rosswog, Philosophical Transactions A373, 2036 (2013)

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.740454Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.740454Z digest=sha256:f104f3bfa4bb009ba1667cc0726da1f26e9c89029322fc9b6d5160ee8326d82d

Observation f34d5484-bb1c-406a-bf9f-27b7d58a2c7f · outbound

This paper cites Thermodynamics conditions of matter in neutron star mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Thermodynamics conditions of matter in neutron star mergers

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.747349Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.747349Z digest=sha256:8ac3dd73d78978b62169ae000fc2f2c5ff7685cf1fa89f62577dccbb5e8cf43c

Observation 619b12ff-6e5a-4d5c-ae07-b201812e0bed · outbound

This paper cites Spiral-wave wind for the blue kilonova.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Spiral-wave wind for the blue kilonova

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.754414Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.754414Z digest=sha256:9cb6781f4c6a900445fc496f7791a45eb2551532ca384563dbe409719c99b545

Observation 2e320e8a-7af1-470e-8126-b70dff709bb1 · outbound

This paper cites Secular Outflows from Long-Lived Neutron Star Merger Remnants.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Secular Outflows from Long-Lived Neutron Star Merger Remnants

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.761480Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.761480Z digest=sha256:2d8113b5c19064565fdb594c27afc23305868f5e94b8f8fcab536e5a8c167889

Observation c63c808a-508c-4e98-9446-7a5a64601dac · outbound

This paper cites GRMHD simulations of neutron-star mergers with weak interactions: r-process nucleosynthesis and electromagnetic signatures of dynamical ejecta.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves GRMHD simulations of neutron-star mergers with weak interactions: r-process nucleosynthesis and electromagnetic signatures of dynamical ejecta

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.767127Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.767127Z digest=sha256:46f0ea6aef2f40063dbc2a5bf945fc999902a0be7eb84c4c42ebfb5782f4482d

Observation 2fda9fec-a3f6-4589-9948-9b3ec1ea2452 · outbound

This paper cites Neutrino signatures and the neutrino-driven wind in Binary Neutron Star Mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Neutrino signatures and the neutrino-driven wind in Binary Neutron Star Mergers

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.772190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.772190Z digest=sha256:06b92e72a5ddec17cb8d7b75e6542f9f7df4fa43afbe6a0f9703c6db532f1ee8

Observation 2ff669d1-dd26-4f8a-815c-a03ba764a31c · outbound

This paper cites Neutrino-driven winds from neutron star merger remnants.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Neutrino-driven winds from neutron star merger remnants

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.777558Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.777558Z digest=sha256:24ddc2079ee917d5770b66d293c69509d081f91363a3b4e18c6f8411d4e27577

Observation efa59e6d-dc0f-49c2-85db-87399feeccd2 · outbound

This paper cites Neutrino-driven winds in the aftermath of a neutron star merger: nucleosynthesis and electromagnetic transients.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Neutrino-driven winds in the aftermath of a neutron star merger: nucleosynthesis and electromagnetic transients

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.782289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.782289Z digest=sha256:582594324726c8008e73cdd42e59eb0cda97c2c9ac617f955deec18e14c99141

Observation e5f8dbea-8e97-45f6-8ac1-594ce66f641e · outbound

This paper cites Self-consistent picture of the mass ejection from a one second-long binary neutron star merger leaving a short-lived remnant in general-relativistic neutrino-radiation magnetohydrodynamic simulation.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Self-consistent picture of the mass ejection from a one second-long binary neutron star merger leaving a short-lived remnant in general-relativistic neutrino-radiation magnetohydrodynamic simulation

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.787498Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.787498Z digest=sha256:a27878f50a4e7084915fb2453e16b8bf68684c509e67f5cc8d443bef72baac6a

Observation 73273d55-82f4-4a9f-a604-f713c98da1c8 · outbound

This paper cites R-Process Nucleosynthesis in Dynamically Ejected Matter of Neutron Star Mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves R-Process Nucleosynthesis in Dynamically Ejected Matter of Neutron Star Mergers

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.792215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.792215Z digest=sha256:c3f8c481761f49c1860eaf334498c49f20da1faf784426886a6a04c1306a3a72

Observation caf2eaec-847a-4df9-9c6a-08da3169a2f9 · outbound

This paper cites On the astrophysical robustness of neutron star merger r-process.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves On the astrophysical robustness of neutron star merger r-process

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.798518Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.798518Z digest=sha256:7886a14deae379afe19e956b207056c634bb6dec5dda9f0a0c6ba4488fa2b46e

Observation e86cb978-9de9-4094-918a-233000e0c32b · outbound

This paper cites $^{56}$Ni production in long-lived binary neutron star merger remnants.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves $^{56}$Ni production in long-lived binary neutron star merger remnants

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.804895Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.804895Z digest=sha256:81165c992177e1cf8ac05000cefdec674d1aaabd84f61a95423614c4863828fb

Observation fd3e7f74-c41a-4277-95b0-2da3b271818c · outbound

This paper cites Nuclear Composition of Gamma-Ray Burst Fireballs.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Nuclear Composition of Gamma-Ray Burst Fireballs

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.813139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.813139Z digest=sha256:876e0ba7cf7c7fd1e106367ca383a31eb50d16773e89bd8ac68180a258ae3c98

Observation 171b7cd2-bf3a-4f6b-9e03-59915d1e1abc · outbound

This paper cites Three-dimensional GRMHD simulations of the remnant accretion disks from neutron star mergers: outflows and r-process nucleosynthesis.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Three-dimensional GRMHD simulations of the remnant accretion disks from neutron star mergers: outflows and r-process nucleosynthesis

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.819363Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.819363Z digest=sha256:e77f1e6f744d4f54feb85d581dad051df650e297c2888f3b85d30e386bfe4252

Observation 69f68d53-11a4-4326-a971-c48df3724014 · outbound

This paper cites Emergent nucleosynthesis from a 1.2 second long simulation of a black-hole accretion disk.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Emergent nucleosynthesis from a 1.2 second long simulation of a black-hole accretion disk

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.824978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.824978Z digest=sha256:d4611bdd43a7bf039d3e8036e37176b20dfb239c06d3cad5ade3205fe5202a0c

Observation a49ec711-11f6-447a-98b5-0b0b7df3b292 · outbound

This paper cites Kilonova Light Curves from the Disk Wind Outflows of Compact Object Mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Kilonova Light Curves from the Disk Wind Outflows of Compact Object Mergers

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.830100Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.830100Z digest=sha256:d3bccab52dcac74f276cf8e966f7246ed4d5c4e37b2b2c8c4f0e8cc4f653a508

Observation f8902103-bd89-4abc-a3c8-fd2470d1c68b · outbound

This paper cites Kilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Kilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.836260Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.836260Z digest=sha256:a82c83be9bb18f68acca41247a8496eb5d6684a5bdad242c658c5d2f59be0b5d

Observation a0323cd4-b0ce-431b-8d3a-ac3348329d43 · outbound

This paper cites AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.844332Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.844332Z digest=sha256:b8aae1df6ce265f44530939a22820de5ce0477e0592451f9eb6f58e879397c24

Observation b4e5bd7f-067c-4baa-a012-5f37b574e0fc · outbound

This paper cites Numerical Relativity Simulations of the Neutron Star Merger GW170817: Long-Term Remnant Evolutions, Winds, Remnant Disks, and Nucleosynthesis.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Numerical Relativity Simulations of the Neutron Star Merger GW170817: Long-Term Remnant Evolutions, Winds, Remnant Disks, and Nucleosynthesis

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.849417Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.849417Z digest=sha256:bd70aacf75477058ccfdac083bb246a5ba8a0ea6fc6b1e0465f738dd9a9b1a67

Observation b00fa826-6bc4-4b7f-ab0e-b1a0b20e75e6 · outbound

This paper cites SkyNet: A modular nuclear reaction network library.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves SkyNet: A modular nuclear reaction network library

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.855091Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.855091Z digest=sha256:9f9197255b82d2e0479a08a923cd4e6c0c4d58226cfb1cf416e16688b318c28a

Observation ae84ebbf-f080-4da2-addc-df7d24e9fb2c · outbound

This paper cites The nuclear reaction network WinNet.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The nuclear reaction network WinNet

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.860849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.860849Z digest=sha256:5189cb34565c2f5ef75d0348fd0c2c04c03ce2dd38b0289015af6a72be33b8dd

Observation 98c9ab87-67c8-423c-a6b5-c2f6bbf1951c · outbound

This paper cites Element formation in radiation-hydrodynamics simulations of kilonovae.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Element formation in radiation-hydrodynamics simulations of kilonovae

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.866408Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.866408Z digest=sha256:d6e1f6bc84006fac93a9b2745a38b129dda2fdd0756ad2109f03a36aca957d3b

Observation e05cefe3-efcb-49c7-92d7-5d3b796b70f3 · outbound

This paper cites Impact of in situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Impact of in situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.873342Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.873342Z digest=sha256:2d469c5d906b3db7ad1b8301aeb480e26caa730fa171e22a421002cd7f7270ce

Observation 91a630a6-bc0e-4208-8d4a-c9d5c56b5096 · outbound

This paper cites Dynamical Mass Ejection from Binary Neutron Star Mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Dynamical Mass Ejection from Binary Neutron Star Mergers

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.878498Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.878498Z digest=sha256:7a5f60d843b6bca19368d77b9c44c57b2fe6526096062c2a8a02436b8063d040

Observation 6c17f28b-ed89-42ef-8783-17c6100f5339 · outbound

This paper cites Multimessenger Parameter Estimation of GW170817.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Multimessenger Parameter Estimation of GW170817

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.884554Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.884554Z digest=sha256:a99495c726e9b9b592ed69a2b4cb174eb88082a1bd821b0a053d3090fefdd2d4

Observation c71f22f8-23cd-40a6-9044-d63617c5f69c · outbound

This paper cites Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.890720Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.890720Z digest=sha256:7b33187ed690ba9fcd17a8a60a13e301854e4d4a7cfbf3786a58d1a96a77eabe

Observation 671bc9e7-f3b1-440a-b973-6f9a2d53a8df · outbound

This paper cites Long-Term Simulations of Dynamical Ejecta: Homologous Expansion and Kilonova Properties.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Long-Term Simulations of Dynamical Ejecta: Homologous Expansion and Kilonova Properties

Reference 50

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:20:58.010558Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T04:20:55.896534Z digest=sha256:3e9fa6f4cc9e55d35879e40d9549787c40da61932163fceb97c05762e3d3e99c

Observation 575fd796-48c4-42cc-a677-d2cd17ee2237 · outbound

This paper cites Neuweileret al., Phys.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Neuweileret al., Phys

Reference 51

Resolution
verified exact
raw_fallback, observed 2026-08-14T04:20:57.984166Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T04:20:55.901458Z digest=sha256:815c116fba3f00e2138a8e81b9fc1aadb78553949d75fa37c91ed1380a3c0622

Observation ffed1057-7fea-4e71-bbf0-441a208433a8 · outbound

This paper cites The long-term evolution of neutron star merger remnants - I. The impact of r-process nucleosynthesis.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The long-term evolution of neutron star merger remnants - I. The impact of r-process nucleosynthesis

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.908612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.908612Z digest=sha256:0253215ce8683ad2cf9b620585786f9b7c4f1b3e04acd88b73f672bdaae31705

Observation c8b55ee8-3d7c-46ea-8503-a8b36d9ac35c · outbound

This paper cites Three dimensional end-to-end simulation for kilonova emission from a black-hole neutron-star merger.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Three dimensional end-to-end simulation for kilonova emission from a black-hole neutron-star merger

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.913270Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.913270Z digest=sha256:3962d548e3dc1c7c19677596bfd88b0ea370a7f7d06f25f0a4c353239e12900f

Observation 6cefa4a8-c6eb-4b4c-b395-6a3b8aa1b8d8 · outbound

This paper cites Light Curves of Core-Collapse Supernovae with Substantial Mass Loss using the New Open-Source SuperNova Explosion Code (SNEC).

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Light Curves of Core-Collapse Supernovae with Substantial Mass Loss using the New Open-Source SuperNova Explosion Code (SNEC)

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.918098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.918098Z digest=sha256:28af2a50e761eecb63eb0d02bd9441f7a7274692080c434f1647d83122115b40

Observation e4f821be-ddb0-4abe-b85e-8ba6d3e7048a · outbound

This paper cites POSSIS: predicting spectra, light curves and polarization for multi-dimensional models of supernovae and kilonovae.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves POSSIS: predicting spectra, light curves and polarization for multi-dimensional models of supernovae and kilonovae

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.922652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.922652Z digest=sha256:9a37230baf9bd2ed0e8e387d57b59c8c9fa477f430a11d19e442d7a98c42d40e

Observation 833c3326-3ce9-430a-a633-0db8f6353f61 · outbound

This paper cites 3D radiative transfer kilonova modelling for binary neutron star merger simulations.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves 3D radiative transfer kilonova modelling for binary neutron star merger simulations

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.927562Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.927562Z digest=sha256:5910425ef7af42b59716bd1e4713c96111816a57c9716144e74414ecf93fd0a7

Observation 51837883-a44c-4ad6-92d2-2a3a3972e9ad · outbound

This paper cites an unresolved cited work.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Unresolved cited work

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.937918Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.937918Z digest=sha256:eb26a6007e016304b2b23643476da5fc904b08620dcb4fbc9e7a8b4d6512efab

Observation 6a3b9d74-a456-41af-b0e4-5ce85fcde6fb · outbound

This paper cites AT2017gfo: Bayesian inference and model selection of multi-component kilonovae and constraints on the neutron star equation of state.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves AT2017gfo: Bayesian inference and model selection of multi-component kilonovae and constraints on the neutron star equation of state

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.942369Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.942369Z digest=sha256:fdac1eb4a529696caf789251d55cc8e862314337a0b4da34fcb582489abfbcbb

Observation 82a7caf4-5dde-4e28-9d52-b95f04623eed · outbound

This paper cites Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.947411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.947411Z digest=sha256:0de7a7ddfd5ad1ebd37b9f1f9de6c16acb1b9b5318f1eead8a90549be8b59e40

Observation c321b679-0857-45a6-882a-9931340d16ca · outbound

This paper cites Kilonovae.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Kilonovae

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.952418Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.952418Z digest=sha256:4973979a5b7b3566b3584035a9b5f8a732672e3f3e1a4eb0e5817563ac48ce65

Observation 03f12d27-912f-4b10-96cf-ed51246aed86 · outbound

This paper cites Tight multi-messenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light curve synthesis.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Tight multi-messenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light curve synthesis

Reference 61

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:20:57.690625Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T04:20:55.957840Z digest=sha256:a936b6f99d744009f3d7f533d8179f0342ee2b201d185fbcb9da2e973703b5ee

Observation cbebccc2-014e-4578-8362-78de64394c2a · outbound

This paper cites End-to-end kilonova models of neutron-star mergers with delayed black-hole formation.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves End-to-end kilonova models of neutron-star mergers with delayed black-hole formation

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.964114Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.964114Z digest=sha256:408bdaad476f0a8b78ce9bb0856919f2c135320f5000f18afc008fe7eeeae8e2

Observation 43128db9-4c6e-4d4a-b91f-740ab5bdb216 · outbound

This paper cites A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.970052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.970052Z digest=sha256:0602a987b01a18745789ac539ea1755c3dea0323e858f01432b7312b830abb2b

Observation 8491415f-c539-4ed4-a745-e579fa21d848 · outbound

This paper cites thesis, Max-Planck-Institute for Astrophysics, Garching (2008).

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves thesis, Max-Planck-Institute for Astrophysics, Garching (2008)

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.975593Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.975593Z digest=sha256:74070263f70881be75c7b16e24d40516ff553461cfffec1cbc10ae4ac36fbae6

Observation 66d22412-0233-4448-b43a-f3d546bfba08 · outbound

This paper cites The Athena++ Adaptive Mesh Refinement Framework: Design and Magnetohydrodynamic Solvers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The Athena++ Adaptive Mesh Refinement Framework: Design and Magnetohydrodynamic Solvers

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.981031Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.981031Z digest=sha256:fe9a36354712742dc6939bd3cb9fc4361445e2e2573d666b78d38ae8c54f64bc

Observation 19095b42-50b9-4a1d-9aab-af216561512a · outbound

This paper cites an unresolved cited work.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Unresolved cited work

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.985957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.985957Z digest=sha256:cd00b3b964aaac35837686d66c2d6fdc6bd368b9c1dd10e0fd625c4b232a0295

Observation a41e048c-64d1-4d16-b09a-53aa9bc20fc2 · outbound

This paper cites Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.990974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.990974Z digest=sha256:a5bf3f0a10240a424e8cbaf6211b3749bb2ba3547dffc613c4eb4e2190c76bd5

Observation c89b637c-77b3-401a-ab46-59df539c1e35 · outbound

This paper cites Cocoon shock breakout emission from binary neutron star mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Cocoon shock breakout emission from binary neutron star mergers

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:55.995594Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.995594Z digest=sha256:5ee92435ff4a50167041862ac11a058f42e9fa1497cfb3475dc423acd3299c63

Observation ae07c095-7b8b-4953-a9d8-2408d54b0aca · outbound

This paper cites an unresolved cited work.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Unresolved cited work

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.007083Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.007083Z digest=sha256:fa4855eecfdcdab658a9d86725f8a31d8564840978ea5a3324006b5b765fcded

Observation 020ccf33-54ea-4209-aea7-92d1a2032f59 · outbound

This paper cites Radiation hydrodynamics modeling of kilonovae with SNEC.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Radiation hydrodynamics modeling of kilonovae with SNEC

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.012920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.012920Z digest=sha256:edd31d487a7ae8115c59680427c1f9c3149eeb77ee591f82228c12191efecea1

Observation a47093de-0173-419b-ab60-1b447d51678e · outbound

This paper cites Banyuls, J.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Banyuls, J

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.019581Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.019581Z digest=sha256:412d40b4dc5dede33750f4b9e567e33ce93260c8df733a15320061583a8dd091

Observation 7c36fb00-5569-40c7-847f-25149fca6412 · outbound

This paper cites Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.024998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.024998Z digest=sha256:3a214caaeebec9959ed3c53c041da07803435e836202ec9a551646e7d069f5c7

Observation 8fc5ca6f-7489-4025-b726-8b517ef89af2 · outbound

This paper cites Microscopic equation of state of hot nuclear matter for numerical relativity simulations.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Microscopic equation of state of hot nuclear matter for numerical relativity simulations

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.031848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.031848Z digest=sha256:ea3039abdce59f2db1037334e6809672adc0f26a309669a0d776a4fcd8cf8a32

Observation ac0328dc-041d-458f-802a-205b07e89d9a · outbound

This paper cites The Equation of State from Observed Masses and Radii of Neutron Stars.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The Equation of State from Observed Masses and Radii of Neutron Stars

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.038160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.038160Z digest=sha256:23f5ff12bfed6e2e8e7587f402ad2acb7bc8a5d00654f0f031f39fc41469c6bb

Observation 89fdc1d4-d2c2-4996-a505-8bd8f21696cf · outbound

This paper cites Composition and thermodynamics of nuclear matter with light clusters.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Composition and thermodynamics of nuclear matter with light clusters

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.044508Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.044508Z digest=sha256:96bf0396da2fd62c76b7e0892b3ed386d88c10fb30fee71c5d8d025620454fa7

Observation b4ef3a0d-defb-4250-86f6-82c80af13d12 · outbound

This paper cites Statistical Model for a Complete Supernova Equation of State.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Statistical Model for a Complete Supernova Equation of State

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.051029Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.051029Z digest=sha256:3971a4564197904e92ec4d9a408bfbdded2dbd313e614b54676878459804297a

Observation 7663495a-fbae-4d9e-9e83-43950814a080 · outbound

This paper cites THC: a new high-order finite-difference high-resolution shock-capturing code for special-relativistic hydrodynamics.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves THC: a new high-order finite-difference high-resolution shock-capturing code for special-relativistic hydrodynamics

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.056266Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.056266Z digest=sha256:cd5c2e86ec1106fb3e41169e89de3a22f8cd1079573a737ac9ed24d2004058cf

Observation f59fedac-83b2-4b5f-9fd3-b1e77479c48d · outbound

This paper cites Beyond second-order convergence in simulations of binary neutron stars in full general-relativity.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Beyond second-order convergence in simulations of binary neutron stars in full general-relativity

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.061911Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.061911Z digest=sha256:5e306d8c436d2d3eacea0972e931176b9292241a741e1a30742d80b8196be4d6

Observation 1b6c5590-5eac-4686-9cfd-1bb9d694b9a5 · outbound

This paper cites High-Order Fully General-Relativistic Hydrodynamics: new Approaches and Tests.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves High-Order Fully General-Relativistic Hydrodynamics: new Approaches and Tests

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.067187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.067187Z digest=sha256:50500da874fd55a8611bec53040ea02d5c5f0f9a5903f7c0762c4b65f4acec35

Observation aa8bac4b-7f6a-4b84-a81f-ced6417e46c3 · outbound

This paper cites High-Order Numerical-Relativity Simulations of Binary Neutron Stars.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves High-Order Numerical-Relativity Simulations of Binary Neutron Stars

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.073609Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.073609Z digest=sha256:6293c945d699a89560266ebb6e11a8f1ba79b1558dee8335d059a871cdd5864f

Observation fd5d8289-9a32-4a4d-bb4d-ad30338c6e48 · outbound

This paper cites General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves General-Relativistic Large-Eddy Simulations of Binary Neutron Star Mergers

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.079157Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.079157Z digest=sha256:c0887f61de438938ab4144c585aeba566f4d98da8362b86dc3b60d2ed7e73ff0

Observation dae6b4d5-ee8c-4c99-aa15-c89c238d377b · outbound

This paper cites Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.087549Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.087549Z digest=sha256:e63b59eb11585ac735f36431eb98da15df42ed3f990da8bb647c9ec192137938

Observation 5b3dc02e-cbe1-4bda-ae62-6a459039ee38 · outbound

This paper cites A New Moment-Based General-Relativistic Neutrino-Radiation Transport Code: Methods and First Applications to Neutron Star Mergers.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves A New Moment-Based General-Relativistic Neutrino-Radiation Transport Code: Methods and First Applications to Neutron Star Mergers

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.094626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.094626Z digest=sha256:3621fe0de6711771f255f6d82c0ef1b9ec6d72affdda2d85d97e03e26ac0b2ef

Observation 36a449d2-8c27-48ad-919a-3763d0869afe · outbound

This paper cites Implementation of chemistry in the Athena++ code.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Implementation of chemistry in the Athena++ code

Reference 84

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:20:57.262247Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T04:20:56.101186Z digest=sha256:288a1600d81ed736b4b9eee82ff59a0c694972242f8be93c84d2ea018a9b0885

Observation 85e7fffe-a330-478c-b5f9-0d58a0c81834 · outbound

This paper cites R-process heating implementation in hydrodynamic simulations with neural networks.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves R-process heating implementation in hydrodynamic simulations with neural networks

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.106943Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.106943Z digest=sha256:8d15b5a19b355dbfb91c863cb53af907dd6302693002ab282e77d34e6e3fe29d

Observation 91f190fa-4f3e-4830-9963-1d53ee63aa37 · outbound

This paper cites GR-Athena++: General-relativistic magnetohydrodynamics simulations of neutron star spacetimes.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves GR-Athena++: General-relativistic magnetohydrodynamics simulations of neutron star spacetimes

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.113963Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.113963Z digest=sha256:8acd596705cc7fa5e8d335924faa945e892886adddab9fef64e37350e28485c3

Observation 3f0de12b-6e5a-4f5a-80ed-7d7f92443cfd · outbound

This paper cites Robust Recovery of Primitive Variables in Relativistic Ideal Magnetohydrodynamics.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Robust Recovery of Primitive Variables in Relativistic Ideal Magnetohydrodynamics

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.119611Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.119611Z digest=sha256:97c256054c70af04206fc9a3de61b40086ba82f9788d96b783e319eb71fb2cac

Observation cba870e5-ab7d-4a5e-b7f5-9d096e35fd3f · outbound

This paper cites an unresolved cited work.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Unresolved cited work

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.124731Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.124731Z digest=sha256:2c6e75920a1c51bdccd8e58931503be22e54ffff3b72e5d232b193757486d6c9

Observation 06850e81-e566-45fe-8fd3-cc12e8973489 · outbound

This paper cites an unresolved cited work.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Unresolved cited work

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.129309Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.129309Z digest=sha256:caeb256f9693e1af9b485abbab6091ddb111ec795ae3f2be5a3a961b3f213be3

Observation db926b9b-a08c-403f-bc93-160643038141 · outbound

This paper cites an unresolved cited work.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Unresolved cited work

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.133914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.133914Z digest=sha256:b2bbd6514585bd3c5e81d8b3bf4385b74f1922c74e6bd37229a430a9594df970

Observation 569cf1f3-d172-468f-ada4-2b4957f58e08 · outbound

This paper cites Langanke and G.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Langanke and G

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.138791Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.138791Z digest=sha256:e96339926c76e859ad129e5d0546bafafb7af773a0ef7681e6f3bb3acb76d18d

Observation 21dd6d81-923e-45be-9ae9-3fd2c7be07de · outbound

This paper cites On the rapidly cooling interior of supergalactic winds.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves On the rapidly cooling interior of supergalactic winds

Reference 92

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:20:57.182348Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T04:20:56.145009Z digest=sha256:552008ab82dc23327e69e9ece4974469eb51af17af4dd5683dbbd0b30ece6d76

Observation 731719ab-0e05-4dfa-af77-fa7020928367 · outbound

This paper cites Vibration-induced field fluctuations in a superconducting magnet.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Vibration-induced field fluctuations in a superconducting magnet

Reference 93

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:20:57.158423Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T04:20:56.150727Z digest=sha256:a714e2ff148bac240849e682171c45be67403eb7a7822ccfe998c2cd7f8e83db

Observation 50b9b1c3-f32e-46af-a398-82bdde4f7b47 · outbound

This paper cites Beta-delayed fission in the coupled Quasi-particle Random Phase Approximation plus Hauser-Feshbach approach.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Beta-delayed fission in the coupled Quasi-particle Random Phase Approximation plus Hauser-Feshbach approach

Reference 94

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:20:57.132947Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T04:20:56.158128Z digest=sha256:c974a85806fd8494ccf2d320855f9dba06e5b5c35cdabe38940f14499fb81b96

Observation ae885938-1775-45dd-b1a3-87523cb85f9b · outbound

This paper cites Neutron-induced astrophysical reaction rates for translead nuclei.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Neutron-induced astrophysical reaction rates for translead nuclei

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.164123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.164123Z digest=sha256:cd673d6fdb3be3f8288e3aea43121d00133308fd8a8c08dc5c4a906ea4c69e1d

Observation ee9dcb08-7cc4-42b5-b35e-c1d43bcd2fca · outbound

This paper cites Khuyagbaatar, Nucl.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Khuyagbaatar, Nucl

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.169760Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.169760Z digest=sha256:02f706f83078c7a45eb36d8d4c78da12cb2b280fe25d3a7b638cdc8990a395d7

Observation b77b2d08-307f-4c08-a90a-88906f304288 · outbound

This paper cites Discovery of the correlation between peak episodic jet power and X-ray peak luminosity of the soft state in black hole transients.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Discovery of the correlation between peak episodic jet power and X-ray peak luminosity of the soft state in black hole transients

Reference 97

Resolution
verified exact
local_arxiv, observed 2026-08-14T04:20:57.085460Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-14T04:20:56.174887Z digest=sha256:9aedb5ca26e293361dbe95b1188980f8e55f8d45fc299a4f30451dd23901da95

Observation 8009b6ba-e372-435a-9789-ae9ca8d06eaa · outbound

This paper cites an unresolved cited work.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Unresolved cited work

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.179456Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.179456Z digest=sha256:2e17347d90c69e09079dce7dea61aab06cabcd7b911caa614deeb54a24ec40b5

Observation c755c880-1d33-473f-89ba-98f721d2e95c · outbound

This paper cites Dong and Z.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves Dong and Z

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.184371Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.184371Z digest=sha256:24e5dd2d5793b68942539cf9b0bac99f85773da78539dfa1d92be0ac947ef06b

Observation 0d3af2cb-695d-4305-a818-52a0477eb5ac · outbound

This paper cites The fate of star clusters near the Galactic center I: Analytic considerations.

3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves The fate of star clusters near the Galactic center I: Analytic considerations

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:56.189425Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.189425Z digest=sha256:18f706b6f1d727f6e1525fdb094143ab7809f451b5eba858fc3a5f640262dc6b

Pith citing papers

No inbound Pith citation observations are available.