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Paper Citation Record · LEDGER

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

As of 15 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

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measured 100 of 131 reference resolution

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

measured 100 of 100 standing notices

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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.

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Reference resolution

100 of 131 outbound references displayed

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  • verified fuzzy0
  • unresolved91
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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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source=pdf_text observed=2026-08-14T04:20:55.705896Z digest=sha256:60bc492d0a6bdaa2c1a1c22edc5b2bc3c41d34e0c0108b810dd510a199aa2891

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

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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

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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

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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

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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

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source=pdf_text observed=2026-08-14T04:20:55.735334Z digest=sha256:c200946c64177a7c461a1215dfe8cd1b45a4e1cdfdc2d9afa5c66c61b00dd8de

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

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source=pdf_text observed=2026-08-14T04:20:55.740454Z digest=sha256:bf1ddd9a2816ea7405fd088a492fd70e78465b5a07c7477cff8692ac037104ed

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

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source=pdf_text observed=2026-08-14T04:20:55.747349Z digest=sha256:7ee546cbc23b652f4efeb82235cf483700d995e06dc8c3f7bcc93b651c07bf2f

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

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source=pdf_text observed=2026-08-14T04:20:55.754414Z digest=sha256:98ce9529b0a808d9fc6ba82dd771f8ec750dac143fc3ba85e224bb9256d786aa

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

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source=pdf_text observed=2026-08-14T04:20:55.761480Z digest=sha256:6d3facc2d90174e82af95e6ae36ad00681487c63164e4b17f3460bbf67a8e55c

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

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source=pdf_text observed=2026-08-14T04:20:55.767127Z digest=sha256:b184cd804c618a024446c8a66a63e06466ab24b82626a9e6f2c03cd0d1c53d79

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

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source=pdf_text observed=2026-08-14T04:20:55.772190Z digest=sha256:955813310aa5dba047748aa31825032e62ff89a52ee1197f0c559b37b1b3a487

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

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source=pdf_text observed=2026-08-14T04:20:55.777558Z digest=sha256:dc28ab17e10050b07b6f59550ff95f1077a1b244170c67aab65827ba556322a0

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

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source=pdf_text observed=2026-08-14T04:20:55.782289Z digest=sha256:bfac30be0e48ccbba49d2fe195b59232d21f1ecd7d8e41cfb26616170fff694a

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

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source=pdf_text observed=2026-08-14T04:20:55.787498Z digest=sha256:e3f06978a439276c24642b542d065027a457c0f6c6fc1d8b772ab9fe25ed90d9

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

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source=pdf_text observed=2026-08-14T04:20:55.792215Z digest=sha256:b86f9edae0af8839400f68983ba9cda73a526c9023b87833f9edd226261987b9

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

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source=pdf_text observed=2026-08-14T04:20:55.798518Z digest=sha256:cec7255319017db63810a6e472ba388826ec2de0df39b282fec63db812af524e

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

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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=sha256:6887c4a24dfde43d2319d5368f425096127e0c99b0096fce14832e7be52cb3de

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=sha256:8dc6b9b8626746a796a6c2c495bc2447b14fd9145c2b8099829513bf38208beb

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=sha256:55ac7853176921108bd3ae4a085b1b9a5e1d793606300ba0c412e6840445a496

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=sha256:880ba9999fae7d2741cd0724e9b554d6f388b34e456e13c7e67167afa9025ddd

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:ff6911ec5fa73066997ac7b1c0f524d3edd410164c799049160414e71c257123

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:ffaced6978199699f7e51f3ffdeced97eee8a0d0987552a2d8581620ed225431

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=sha256:69209463d7cb7cfe201074605723e648b681780880a1a200b80b4abd02c3d015

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=sha256:6d52a9de70604a047ba2af4b713130e3193dc3946af5076ae90f4acf321a45d8

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=sha256:2472dd9c32735c7789d1859d9fe170412b8ab051fa7978536ead2fa9cf08fe38

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=sha256:321a1234f95c213ff0c2da74e89eaccaf22313262a1f8a9ef912bc1306588bd4

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:ab600efd0f334e77916edc4e82e14a57aae3d8ffb9f44fbcd618a4e87dd5efcf

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:d0bc8e964b7554d7b29043ffeaa8b3e47a55d2be727e0960477c484ce98da973

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=sha256:85e3722a20fe615dca22fc49420dbebc0123fd10bf0a2ecc1bbc56fd4b364f3d

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=sha256:2c995d65eb8d4c6a2db07523a50c4cd4a152577e6cb53050bba5f30b0302b6b5

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=sha256:98bde1f750783448108d69fecfc097efe6f42c5d9577901adf01e24bbe454232

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:ca1c8646f6a5fe2834dc23e9d6f9b882b10a604fd32f32c5cb4bfc61f91fa089

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=sha256:9cb3df625612e185e683f0fb3cdd56c0d6f2919db90d21c8fca9492ddfa24e5d

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=sha256:3f4193bc6d7e6d5e1276973b9c82ae700b6e0060bc2662252906d836a0dda355

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=sha256:78547c42383fa3245cd8533d8418195ce464312a54426f3821a6c8e04848d468

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:ca5390b8f7e3d3d3dfb119c85a9c71c250aac3cc49fc6e2eeb90c8e24848ca10

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:a985f589eb4897be8a0c0b518cb2855fb2df5458506e7e592c73347febc3f7a3

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:f56b44005f00aaf2dcfd4001d513748c96a8d466e1575368c81cdc4ad411e77d

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:f5616866dc5c05fe781a5263afd8434f108362160dab6c021a08ed03a062ec07

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=sha256:6f864b29f2665daa825bfec1d00ac9d51ec48682e0fc30828fabed51773dfcc4

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=sha256:3997b76629bb78d33782b53cdb7e8ad92c68312afdb5b13e31f0ce2d0730b71b

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:bfc3e7c6de5b4f4588032fb15e1323c52aad50b9adac3fb628a2f5eacf9b4dc1

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=sha256:44fb9f9b127b02180733cfbae849ad9f63aa6fda38a2bfbc1d686d0197d55305

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:d162e4eda7a29473e25333229263e57fe455c737e98b13dfb15459d8dbf500b7

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

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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:ef485d1ce9dc621edd2f40638316675cd41d4c9f72dfd9e917ac23d189451f0c

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:d3cedb82f7dbf120239fd0bb514d10b69a4457e7b2625400fbf4bbb37e493078

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

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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=sha256:4df0fea97ffe3682b1034c10c75bc5227b4f0d71f08ffa425c1ef782f71263f1

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=sha256:513e8dc41ac4e5af2cee4477a56d5d2bf406c067626b035b71561409e3593240

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=sha256:656c3114802956a6ad7ba92fafc0119297b657e7c119bea19d5a3f0f79ebaffd

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:d86a847ad98428fe616d5f95254ffdb1e4cc1173b26198c84a87782282fe784c

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:be7895d4112f6ad23cdba8ab917418db744a9cbef830cdeea3f36d6644681e75

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

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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:f5b7414ec5e677985d9d37cfad905b92c2532dd0769e063f5ef63755fbe69ec4

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=sha256:9bdb734c82bc8c3a8aa63c808ac2312c210d44a3d4a35c90e17d14f3c192666a

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:b880e372f4d29293e6a6e5ecd48b9fad0531a92cdc4599aa30eb51af93e21f03

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

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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=sha256:809e956a38f44fc151d14486d7d3c48c91862702336a49a77469d97b265e17e7

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:df1b5bec5c0af1b5f675c157f329e0c79cb5ce8e92d1fc71f8d022042597959c

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

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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=sha256:6677e4ce728b1938dc5e8312c6189b52d5e4d3587acaf3fe27402b8ef51612d4

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:d6dfc58fc59ee411593084ae49213f38e9327cd736f8cd275efa003fe1141bbc

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=sha256:379453a18ab4ce85ad3749facbd718e77505c7a6032c16fecd3431488cbca6bc

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=sha256:07a8138736b9fcfc7ce9abb39a1ab709e6e1d783dc5ba45431b2209fde4febb1

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=sha256:44280b1d5e16945eb8a232c70681f703e61332b3250e4543995526f87ebf04cd

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

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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:e569934b5914f2754e0e7905d16299ac2a6369510541577256af09c0f11d7094

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=sha256:5df83fc8d9e9c83ed5bfbd50707d5188a6c34de070518df4dd8a422e2035a25b

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=sha256:17b694306276ef2994bd0a20ba4f4c69d854bf73f4a45d9ce6a727154ff5fea8

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

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source=pdf_text observed=2026-08-14T04:20:56.094626Z digest=sha256:0d856f961c244cb6c279ce83a953222b3efdf690e90daee284a38ac22052ab1a

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=sha256:33ff18c302f5d05e84c6b6fe050b32543ce5547b40bac19543112b4e32791e84

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

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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=sha256:016fc8881a15d656f6115188793f23934737020cc8a34eec43528e583d71bd13

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

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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=sha256:45e858bdd24c0da95689db88a82bf5b6d3c73fce8d61178a20e4c726888fe887

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

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

Source-reported events for the cited work

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source=pdf_text observed=2026-08-14T04:20:56.119611Z digest=sha256:fb4b384ae70a644ab9e010fb64ac134ac31a4ba5e205208df8ea4a17df14006d

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

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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:a9d8a74a9d6206b918b7b9f93fce69dc04c704cbb04932fc3bb36bb5da0800dd

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:a8eccba1028428704234278efa90ac0e8ddc6b00972775430221b7cb73d52cc2

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=sha256:9203f9f488e892a510c3b1d7f8bb8ef20d053169dc3ae970e5e38542fc0a0a87

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=sha256:3ff09720eebebdf661fc52bbd578f7ad3226f6cd4671c45bfc3cfa4b86609afe

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:e6bc70911d9d46997498d93955a4eca9cb329be183cccc620884231268f97a79

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=sha256:6a47a87cbff104e7c3588700a965bd988ec6453e61fab1149e81eeeaa20ed78a

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=sha256:804152d18a710a4b81a322e85403f206f3beadf53903a74903da9951f062798a

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:fd1eb2f652ef8516957fe7a2e2f74d11dbac67e4fe8c2bd3aaac0234026d8e2f

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=sha256:32d4c50125959c87247352d461e0574994c03c15d5ed5be05b93a5ac844a6dbc

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:eef98a98f4b657b52ec53aa526e7fe3721624a284b8b9513171dda3d3e580c17

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

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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:c0b768b8eae45c66f16016c8c3c9a4ed9d901f313e7a2dbfe05aef6eb5b39809

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:ef5c5269fa438976b8b9dfbfb61c248643a9765b378a8b2a3f6b58d4fd19f492

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

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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=sha256:70bc6b78240b6bd7d38b80ed7a3b1f2134a597dabece8c1da2db084b5a261626

Pith citing papers

No inbound Pith citation observations are available.