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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 16 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 2026-08-15T06:32:42.880941+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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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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source=pdf_text observed=2026-08-14T04:20:55.617980Z digest=sha256:94da8d9e85de6e17a9d886de63f3942b08e066b10016fa571e2ffc95fb435af2

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:fe4b860ade57a416d162f434f7436985f5d3ac7f8d5485ddf7c9bd078608b81b

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:b560bd9a29c1741195a503df5b9f9a4bab2fcdbca2b1dccd1f6f7f064b7984b0

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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source=pdf_text observed=2026-08-14T04:20:55.638010Z digest=sha256:28004360aaa0974c332767ac2fce18bd28120662f2c6152ad329fa88138d2623

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=sha256:88e2146d06abe527f1a382bc0227edd8523f4c461f9fee91d25ac951e2005ee9

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:e4888815f8097264534a3221fdae699a6ce4330ca4144fb196e60756b347eef9

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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source=pdf_text observed=2026-08-14T04:20:55.686656Z digest=sha256:8126e49d4bd188d76bc3371f7f08ebd0bfadc858f58404f64d34b449c74e685d

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:e5830a708dba70d59c5921d6fc0684f3bbf6f855caa8e92a188e0d2330cecdb4

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:c0ab75e955d3d8e2d3a95d0866d33d9e534fad70a8b03902d9746489ac701460

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:b834b8591fc748eff38bb0bbc99880e91cd84f2256b448d43ae358ff32278b88

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=sha256:704dd12b2f385cff8957018598b1777a3bdb57d577d2ae327e06321d330f6d5e

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=sha256:5aaf9cdd41fbaefb7efcc159f270f164308044a2ac55cefcbe26e02b332b3906

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=sha256:58c01b7e55dc4eff18f8cb6eb1cbb785aa9c966f5dd96874d09329824ba2febb

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=sha256:21bf2536534f84a64a72d84e836c0127bdf79f26b8b00fb98161f495f36095f8

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=sha256:70030e854e3ae2679d70b0b9a84c513daabb422acca5636570a75deb03c55d7c

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:c53042170d38eeea869a25bb12a45c6583a63d0e777aac90c34eec933ae6a433

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=sha256:313c75d054a0f538d580e3ced6d4d919de745c6f630044e72462c2c00fcabe3b

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=sha256:2c113cad5ce814f74419d60d85697ea28f31d19b7782ee22fe4b3a55a47ba1b0

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=sha256:7e2d8f37d1e5729a3b6a67cd0ba2a281de77e567c9180109ef303cd7b65638db

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:bc689c8057f4762c13d411025deb29f036185fc3a34c7a1e0549562ba418d758

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=sha256:1e01555e5da5afacdf9eb5ac3c3d5620d3a7480d6aae9a6aec617748844902ac

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=sha256:4d9cc7addebe9ad5d549fc49f87279c8e0f29afbde73a66f7119ae5f60d6a5f6

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:f04475437322f26a1e0fffa7e94ed30c4e849dad124ca68f0f358972444e4a69

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:e96a3fc3c7cffffa1d243946ed1ba1089e240cd2acb8d6c3011bf0cbb4834b4c

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=sha256:34534eb42bfcb2f68175448ea8231f382da0b2ca8843ab5002a5373db9c78e8d

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=sha256:8118e81ab184d68eea2665ddcedec9760e3b90d13073e60f61273667d751d356

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

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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=sha256:20083a9935f7692460f7c6f9481376623c038b5ff879922f606dda0c004250a7

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=sha256:7751f3ff4cbf9e6d5c3d56973af64063028de4ef882178ef1aaeec7e1120f492

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=sha256:1a86b5098a70e8f4f17d0b7cfd06213df5f7527e6cdd75b8186b73bc3b8fe5f3

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:d1951df5ed2097a0ad75f13599b5f6e30b6c3feb962478d2d4c07a2437fe7525

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=sha256:6060f8e2a2c7f2bb22748cc521f0eefd947ca87eeb96e56ca66c1be7b586e8c2

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=sha256:63facc66367b1c3c82e54d068d3dc4d17fc7033f5b3d6aacfa7b08a861b3892c

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=sha256:8b21f70f6722df29f2dc531d4bb004d17478c96cd592477dd42d0cb7f795132a

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:fb706548622c4b7fe9a2a6bd408b7572ac6ac20a190779b29ce24ee7ce24073d

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=sha256:2fde465d32f6549139528ac7f89f07996b7a703f359db9a412f5621ffeb15e82

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=sha256:37837173424a2ec68cab638f04fb401ab997831c18b96082668b0bcf5729f48e

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:20:55.896534Z digest=sha256:ca2604a171bee4e63edc65be0803a85145483751148b262ceef0e0bb10597ffb

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:20:55.901458Z digest=sha256:a96d38d06a021e0cefd9d6f7ab80b419cb5a49a317098d81bde94fe74c86fd2d

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=sha256:2c9f7fe2cddbc294e627ba20d04945855fde6f399363f16f12c28600ac5c4339

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=sha256:9fe9b7e3f993e682e664561b6bee3a87512ae474a3396b6002667d5a927b96d4

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=sha256:7bb778d0747aa62cf5d965d11176f026fc8a2ccbbde0064ae578f362a7491f81

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=sha256:7bf6f505fcfeaac03c62898a14d5b296f381ff62625bcfc801fe73d4f88ffc84

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=sha256:8bccdfb4691d4af60e4b9dbaa811e029dceefae2fe717b08cbc58f694d972c5d

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:f1365efd4b969b22c715e36375910cd5ba3b9607553aa189eda2f3f9f3728816

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=sha256:1ea699e2835424ef499fd1faac1b0868a378327e5bcf0baaa7f9ff7ca4eadc8d

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:d84e0b1fe56dcb3c90fe4d15e858ebabe8cade93274c902682330167acd3bc4e

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=sha256:0cd69d7d1ce43e5a21663b7c61479d6753782f5e7632d4d84ad2442f313c3789

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:20:55.957840Z digest=sha256:f56f921efb7e6ae576450798446a43147be1a4e4040ac6d983fd04cf71679fda

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=sha256:8676fbf3dbac941f07cbc491af9bc71eaeca0a2c7f502838fa3e2c2ece52a036

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

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

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

Reference 63

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:55.970052Z digest=sha256:05edc956e04447749d6fc57b0f43738663c4d8b7a1114cc76e3d4588dec98f3a

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=sha256:0e439a9b5113b745fe286d438a2d0d573648cbe6739aee2afb6149ff4b872d1d

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=sha256:59c7e48b14ad7a88beccfd286b9a650cb2e7abede38d03b0287004beb1c2a64c

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=sha256:1c10837493e653923d28f6dceec729541d6c941c4f5130d4a6c7451fef5a5467

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:d29d9508997398c7cdef5b3d78be4c24695a4190c2b7c9f3788f530b915399b6

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=sha256:7f9e770febed60c67afde9b9ee65647a7d847ebd0a26e989b92c004c168932cd

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=sha256:29817daf3927a5abab440d0a29101d8938d1ea785cfe37de7b038ffb0217d5ea

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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source=pdf_text observed=2026-08-14T04:20:56.012920Z digest=sha256:c2a7b3fb3d022535af2abbbd5191d023a511a3c98ce07ea545a7d4c00c690da2

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:d5ce8b6dc90283b74480c1f961066d9652944cb84974bdce1cd0688c15fbc70b

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=sha256:36fd62d21cce1423ec6ca956ec32e2042a2b38a3cd165f0cc0c4f58038643048

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

Source-reported events for the cited work

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source=pdf_text observed=2026-08-14T04:20:56.031848Z digest=sha256:110ab7ddb113a860548e68977c9a24eb6809a0461c3399bf7129fc85ed06572a

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

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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:f62b4073fbe78647a3bc00d59d655da38e66ce7e6e89ed2509f24f09fae7d105

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:e1c0be3ab371a9b1c92fec3958e170aaf7a7c8703c10f4988ea099f3a516b73d

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

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source=pdf_text observed=2026-08-14T04:20:56.051029Z digest=sha256:a67159534e18bc12f65ba228bda4396d0a2649b8874a443488a29e5bce13b736

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:ae187d858cbc0dc427fbb2686f28f3a52728f73406273ab6a5ab1519f96ab224

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=sha256:0634b6ea8e9e7da8b801e5f6223b264ba34de30492ae40265222ae566650bcf2

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:cf8975f4778ac783755c716df737fd1bd4f1f61d6acf10369b9096eec16ff806

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=sha256:4ce62dbfcca3ef8bf25502060b070a5baf8ca9d84ffdb8793a5aa1817df70d80

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=sha256:3190cc00990e6142ad63a637d370fec691e50fa6baf62646e2b38760f5c4895e

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

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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=sha256:1fde8816f1390c5426e0f43a660b462b56bfcc2c3661928364bc341c9ae9a711

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

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source=pdf_text observed=2026-08-14T04:20:56.094626Z digest=sha256:cf338afff631bc9593edbf5344e2e6c83fad04363881664fd98d84b13c356ee0

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

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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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:20:56.101186Z digest=sha256:9f8583f931f61b229699f8428c72c4d948373c6fa7a018754c9d741d85d5eeed

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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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=sha256:1db72e4b993dd2c66ddb3d1f79037f14d80b3313d94b92d5da7e2a3d441c26a3

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

Source-reported events for the cited work

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source=pdf_text observed=2026-08-14T04:20:56.113963Z digest=sha256:16e99efb6e4d8c4066251de7c2000fc088b505932ea1ac86560eded4c8f3d5b7

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

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source=pdf_text observed=2026-08-14T04:20:56.119611Z digest=sha256:60dd030d374606c6a09bec6990aed14d64b25b07a55944e454f29607ef93daff

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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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=sha256:2268148a41fa6f82913d2d248ac730a46b616627bd180306c56e5c32f2880dc2

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:d057c49f30abfeba97daa49ef6277e00cf18140a6ea826e2635ceb1b94278eb6

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:b5e838acbd2f24987a224f0e23141dac4cc190699ddacfd55e28211d551f371c

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:cd374c94b716d81d53c60b8224077cd0451c777bc2f34a8db8914fe2772b39f1

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:20:56.145009Z digest=sha256:50dd0c123ebac79b0f942ee732f75d8070a04f688aa077baf8c1f1e173a05396

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:20:56.150727Z digest=sha256:6679b60254139af3868e7f5f60baa4a52929a550966add799b38b46c4c74246c

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

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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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:20:56.158128Z digest=sha256:ba2dc864afa38f2cf7db17dedeba917fb2fd872bed3ae4932a07bd9ce6dd8570

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=sha256:0f55df5cff797d007836051f4b910f270d925387fd59b34fa25eb0ea25947265

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

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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=sha256:0390ab5816ed001848183665eddaf117644e861be3cbd378e9fa2479e0772a40

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T04:20:56.174887Z digest=sha256:ad0de387d0c00a707bd865ed1e4fffa39199537564e830d00b41bc2d18c2d35f

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=sha256:8307b5e7f5be5b61794391e10f1badc2eaa6154085415787141c04b07079cea2

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:c3325d1ad281be34060657dc3f238b3379fcccc7ff807e0b5df61abc86b5a144

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:ca0fcec72d5fcd822dc2ccee85d13f4a1052eacc0d4e421a440cee99fa6ce5a2

Pith citing papers

No inbound Pith citation observations are available.