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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 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

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measured 100 of 131 reference resolution

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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

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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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source=pdf_text observed=2026-08-14T04:20:55.623559Z digest=sha256:1878e51831baa21d315c378a70a8d10e309507f9666fe3e7df345bcc79adb502

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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source=pdf_text observed=2026-08-14T04:20:55.630787Z digest=sha256:524417064c8ab6266a7bc141bc946dd29c74e2e639a847371e9afc2034a7921c

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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source=pdf_text observed=2026-08-14T04:20:55.650272Z digest=sha256:23e1bb8726e8641a311ca983046b5e228ca9dcbda9f3b2507fcb4b959f0c1494

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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source=pdf_text observed=2026-08-14T04:20:55.655820Z digest=sha256:6dd8250c7be5a1c62ebf3b40e2d46d1e8d95bca1473fd6081437f4ff885e1038

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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source=pdf_text observed=2026-08-14T04:20:55.661865Z digest=sha256:e3405b73b068ae1551b82e01f0cf3ee4eb2975799d13acdcc2878fa19b686747

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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source=pdf_text observed=2026-08-14T04:20:55.678876Z digest=sha256:9eb4a780840c1ad787dd4532edb7d64d8d3324f45bf24a9c2b0788cfff367644

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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source=pdf_text observed=2026-08-14T04:20:55.686656Z digest=sha256:caa144ae61df01c5e16089117486655fc3c34f545127e0cc889af8be3016d76a

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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source=pdf_text observed=2026-08-14T04:20:55.696468Z digest=sha256:90169e4befce62391f4d99ed3b9532b2d804e9112218b6f909a9f591a7afd8b3

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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source=pdf_text observed=2026-08-14T04:20:55.701348Z digest=sha256:707d4c430160b464e246df582d903f2bb62b10192eaa726b5707927d2e1f0d01

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=sha256:4e01aafd9e8a6e00fb45becbbc29ad4e03a07f5220ceeeafc2a920ced7491f23

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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source=pdf_text observed=2026-08-14T04:20:55.725230Z digest=sha256:94b10bf961d6a9d21eabe6eac74fedd05dbeb6267208cddbc6f7657acd4b0be5

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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source=pdf_text observed=2026-08-14T04:20:55.730244Z digest=sha256:6f26b981994f5b519c74c1b1a999d335af355592de57917b8dfc293af6b19093

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=sha256:5f9f312dd3e83cf55b5a689f6ba48ff0707f33524ecd541d6496eed6f46ebddf

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:a99ff04ed7fdd0c01ab906e0ad51582a74fe7115f8d9e05b570b10b6adcba264

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:e9d13637452a2ccdabb702ef36c75d51337b99f62dea8c3667ba5b5d0d8f4fa8

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=sha256:3f797c4a2a8ec87d380e04f24c138b48230b4d3ad9728b7b8cdca329dc4d5cc5

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:f52eb05666114d7e23805b53766c37e58d0371434238d54a9a2c7ef90f40c332

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=sha256:6d7b7c191c36abb4230255da7cbca4843d7b0867b081d95b08cbe4d272e5c08b

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=sha256:72a15df01e300caf67feac6b7958bace2795ca430457c838295ae783dba0c15b

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:eaa1b8425d2368d437cec8e3aa30a0067bdfb687a28a54bc4dcc26c6c7e1a8c5

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=sha256:55305e4b68dc68cd26f23dbf9ac53c4482c62a7b5db8d8cfbe97cf49508d1077

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:d275216ce0fc46d2d5579d22d83348708587978ad909d166286a532487623f55

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=sha256:20d6907ac6900f3014fd0d87042efde202dbd657cfb73507c4b290717e121b0a

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:d8387336b76ff997ed134cae7d2dbb8ba795b392831ec4142c2617f77050d98d

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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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=sha256:039e53598ee12141b613c96c8492e95b2443740bd67d57ae5370a3a321a56718

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

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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=sha256:2f97513416b0ad2088bddf91c778ef970f62cbf47ef5d4cb977f9a2d762219c8

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

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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=sha256:641e2b823bc582cee2a965361c1e7908eed7455036b867d361fdd868f3ebfb34

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

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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=sha256:0f0da3009da415486c8d454e663901d41dfef3023524371452ff45a0c51df7c3

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=sha256:673aad1f1f4c9c17ae18f6d4bb0cef31882ca34e84bc40c9d1e3bf9e9ef59937

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:cd7f8d85bc6e69700e53446fcb9a6d7f190de1207ac08e7905810b4ce1077878

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=sha256:75e6b7f8e2743fb2002ce1ea42455342b1f4014c505f8aaca4630424ddb4aa56

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

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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=sha256:6a7a0b7e17b2503ffd1a6dce82b6c48d04a256dea5948d88f5acd9fc619b2aec

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=sha256:15c494b15f74d54374c99388250e587a08c7b7c21315d507af1c04f9b12652fb

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=sha256:38ea70659c1a70b040c36d32228c44c191e2251119c4bcf3a38c8580a88224e4

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=sha256:0261c04afb87969b80affe10e32d6196955bea40530dab0473ba0f1f1cf1374a

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=sha256:9f889e86f5fbd17566d5b3efa1d442a46edbeaca393912c62da8276f96a0f28e

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=sha256:35392a048dc3c4f7fbfd076b63b5557cb8b4aec315636144157419f3144a214f

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:cd9e5679fd5cff063cdac75a3086a083d690792a74065ef2c9f34fd586af37de

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:d26c948ed78d789385e35f6d89a07d35b0cc4dd6b805653ad8b0a80f97d726d3

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=sha256:59a5f2caea393fd84de70c00cf834dedabe12b1da5b9712ce93068dd97e2a3ae

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=sha256:296a9362cb6f5f0b23b90cfe1613a3529619ce392b6fe28cddd485d51ac02872

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=sha256:25dd702cf11d56e468e21b8af7ce30fe0867c19f778419e0d1519b5eef5c92b4

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=sha256:688d5b38a6a728c4ba10bb46466e5526d900e98bbc555b87eca3758c2d8bb475

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=sha256:9b8b031331bbd23d3de4cf0095763c36d419e13027db62085810c3434c7d0cae

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:f7ee5c6f1a558ab1d326311fdadd8b8bbc130982d351301707a1db2dd4da76d3

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

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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=sha256:48488ea662d4700be0b48dd6885da20d27f216b99c37d302982c96e2bbca2c54

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=sha256:2d2158d339fba82372595156ae8b154b0117a7ec950c59b230fb1af613b41069

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=sha256:1080141e120ee85635ebdfdb4598ae769782ff834c5c3d1131d91eaf20310a43

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=sha256:00bcc4172e23fd4a59dc6e7a9df268fad1ec525021002d8ccc0956aa142fc1e3

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=sha256:712c8967d4516eef77c8ce6a4fdd63b04342e7f25c935f4c014514b966be3f98

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=sha256:0bc8d884e29c510572cb4b7af5363aa1a3b086b34af38aeaad2e38f01c43b369

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=sha256:2112e6c6ff3003aae35911fcc2ca8bb51e92830a7bca3f99fbc99beddde94d5c

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:bc1851efd2a9fe19e67ee345771f52d37e15b9d767e16e604004fb4664731acb

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

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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=sha256:1b9f5492937c4719ee6d9896371dab1bf092b5f75c405004fffc21d8486037ed

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=sha256:897d3f51ae1e7ba46892c9153c67c0720cda7f3c0f0a00dd982652b42cb37479

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=sha256:533b9179256c319d84fe7ccc2d26331c2563f535c976895bf2d48cd02a74431b

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:e2f51a94e84cd1be245003db8953e48ed1c1d56912b2cd5d17bbad0e5c1e5399

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:d4bad00f2c68826a74c839c100996a0cb48afd743733cc236314514775e08b25

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:b273f8ca71fc7d06491e9f777d5a4cbfae4a98cd69bbb6b29c8fdd1a0fb5a65d

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

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source=pdf_text observed=2026-08-14T04:20:56.012920Z digest=sha256:f5f693ddae5febe33ddfe1f5ac7eb7a4769ad8891e5c09ced9eed7ce8db31d8f

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

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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=sha256:2ec426ddde56ca8bad3d5091de0a09b531091b98a128779bf9d132b3b200de2e

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=sha256:45627adebd6b8acef128caa2fbfca4b848832621bb7baff6c5186cc51d4b1f34

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=sha256:0ea80cda037a6631ded0f3fb9e434861bc6f18808250334df21e02deb0072f91

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=sha256:98c484097515d1d68b24b772f53bd9ff61c4c417124a7648dfc80ee49252a356

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
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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=sha256:91c571b71679577144cb45cb41476b994e8c435f836f5d42711aab9525e47ac8

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

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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:e2fa97e40caa4dba388f8625451488908b7eca4a3a9dd1faef3d78184b6f99bc

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

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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:cc2721bb96505dc5eb247714721ef1421c49aa134c11db4e99d1506429d9f2d1

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

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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=sha256:69b4690f24c5134558823cf294dff2a5cec90db80748416a7c16927e1e71e356

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

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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:eacd00e85205c5d86b86191807e95233517914923935778a88d362e925451b81

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

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source=pdf_text observed=2026-08-14T04:20:56.073609Z digest=sha256:0310e52948321f736385027347361fda628f99560316c292b8986fbfc0a4a036

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

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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=sha256:812ede5e66c74c8bbb7f770cbb8871fcc6d9d0c3e85d431744bcef72ee3185e0

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=sha256:4582061ebeff6d4002d17b9e2df66f006a9bcd8413ce99a8a79526ceb28fe8cb

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

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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:b1adcb9a1702c9fffb1c2ec760fa31c26ee90a0a6e747f767b09ba9f99d61a42

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:c08fb83d835b8a69a2310fcd19ba97303dd0fbf7e8c1f0f88ddbe681f72de64c

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:a629a2fae4d65f823188becb4e2887d538967ebff32b74c42d162fef867d4cc8

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=sha256:04c4d0820113da09d48e1a9fd9e4e11f01d36c503bcbceb1fb75c40a2d0599c7

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

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.119611Z digest=sha256:cd7afd767c4e2b13d08c942e03b6c137c030d862e76223f9160ce3e604b9ad52

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:ce0124da10e4bf3b85b6dca33741c90c920b4aabc51920b305db9f3f49c0a760

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

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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=sha256:16bdbc531ea84aab2e99ff300cd5a49a3f4c9c156e06e4d9d1fdf08259d2be0c

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=sha256:780fbe239b90cd6000563f7526ab94ec0c9a4405e19357b386ba17253e1e3734

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=sha256:1911a6f41027b320459a14a428ead7fc9a9203b877a29809a7a4c43203b4cff6

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=sha256:7975e918236da8de9791d57540a0262e3bf31708ef97bc0b2806ae8986f53d7e

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:e532f4efe585cd74b14590fc185be0bb31c2f342aaa2f3f046a754a6c4620ea9

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:d21a3a529cd97da3adc73d9516e013ded50e57cdf562b2382be0bcfbd6093f1f

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=sha256:6280682be3c0bf523b082b65950b63b878d4bf03db8696ac7fb42c0701664655

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:abb8f65f1981eac7e3440ea0a4f845b1ffbaf9b5531af1a0a32bd65154479ce7

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:aa0958d5664229b1750ca2d19fc9ab66632bc78d746872c807a78935a90f00f3

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=sha256:44fd21163a93a5496d9ea7c601d64001eef266eac8a640c01bace2a3a9b7ad24

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

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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:e5489d6d47d8cd5e7e42011371b43ca0cb5067f48a6f4a75406158df1cf0cf2e

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:ea5eddac78add6112c7b0bde4fd7cbb0da5ef84ae02811d3633eadea8056edb5

Pith citing papers

No inbound Pith citation observations are available.