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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 19 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 2026-08-19T06:32:44.657259+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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source=pdf_text observed=2026-08-14T04:20:55.617980Z digest=sha256:74b3db5e40d71c71b2b9d3a0ecfdb5e0456eeec96468687686318ada9d7220be

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=sha256:234b7558c5b8ca1495c68655ce268311225ca3964a8a4f35b03b9c5be359b353

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=sha256:8faf9bb98a995d56a0a57037a57bdde14f507e9b22c76fd26ec3c5d6a7d7be22

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:fdfb75cc5b9df9e7b81b6bec172892487b5a94f20ff649787739bed6307f2afe

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=sha256:4abc53f6470fc604d3ff6145e2970d6805cadf8a4bfd778f1df2b8c7c60649dd

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=sha256:56042f43b8c176c22f23bb9426c220caf9224723822f143193952704c91c21eb

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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source=pdf_text observed=2026-08-14T04:20:55.678876Z digest=sha256:a5325ddddd8cdfb4f451764bfb972d1082d284a65d702123d4d8c496db2b3c3f

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

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

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

Reference 14

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

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

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

Reference 15

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

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

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

Reference 16

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

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

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

Reference 17

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source=pdf_text observed=2026-08-14T04:20:55.701348Z digest=sha256:77d0d0b030620b8842a4921a91f91e79eeb5c561e39c49bdbb87aacf98ad56bb

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:c6c3723e43b3db5299c06f6c6e27becd6d33d6aa41c5928f25ccd783e5347b3c

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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source=pdf_text observed=2026-08-14T04:20:55.719612Z digest=sha256:72120b7773ab7289e34bed2042120f5a7cde44265a7559f7758f14db0f246035

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=sha256:4cae69d819b2a006a26e324b8b899952e79722f7b4ecb7513bd05c7eb18168cb

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=sha256:1ff4acc97888e74577847465b070428ceda61dd3f74edfb38cbf3d5c65c735a8

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:bb4fa4345ed36561974e4a566b19603cf48571623b33f37b813c4a3e2ac7cf29

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=sha256:4ede316bb64c8632e24dc2f040b42bf861136fe6aecf6180da51ef2d7ff5432c

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=sha256:31dafcbe277787cf577ec4671a2420f6add82835bcc15db28c00f32984a44907

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:d2ae4fe78315bee00377752d24646a89e9a67172eb172753b8304023a03c1fec

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=sha256:81a040ebf4d191725866c3a47d9e617730ec26259440f3b92e64c344d35e3432

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:ea9c7f130cf86c9fbddeabdd557f78fb97e093c2b66c4df2b576b5062c905eaa

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:a8353d1a12e9de9ed89b77786fb853fc740581cdc5f3f6d6b24ea3dd2976502e

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:f1aa47657014c2f47600a2e494a3b3c20ea1fd73f68ed5993b827599620eb522

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=sha256:39285359dd5ce2b590dd62116d1022254df2982e064644ac9adbdc6a25a7d52a

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=sha256:2aa1c8c4e81ba9aa174efcd0fa36574f2aeffdb86fb76f94ec05a43a8285645c

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=sha256:146bc472c861c4f01d6df1041e8e8a0c1613a290ce21fc0162eb3e67a5cf0329

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:b626561937a88c61c85ffab90ea1cafdfe4d9fd6f87bf755e6ed580bbd718b8a

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:f3b3dbbfcffa50a90e9afb541dcf0979a5cdd0b37a3435174e7074c53260349c

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=sha256:34fc5f5a4c5d8f09222624e80d63161d2fb6c13038a69f0b304e9ac881de12e7

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:ecca9f59757033fa7821e4fc86a32eeeda6af12ecd1acb5d9297fa8ad9731877

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=sha256:87d6c5de62757675a238a0b2bb1f75788912f34c20cfdbab0500fa544aead512

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:ba94adcb89df39cd13a6ccb20057f74a8fb35f9a1763426eda9d7aeb372f4324

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=sha256:0b5990259680e37da60ee65898affbe91bc16fc6fc1142f0066ae13dd2f2dda3

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:e6cd04b697aecf4ea12459f0d0ff2faf3925bca626a712019d7a67d8639e69df

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=sha256:59b3a05269bece2dbf0626584348f53e3bf55932ae2c637ea750e83040d26a6a

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=sha256:9e21d0cbb240aa45c6358038c3d0f63c72aec7e3cc492e5c206f39c407911488

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=sha256:38d1c9a5f99aed534455a6f0730da23f6c01f89ac73d3305669544a789931e9d

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=sha256:172f8e182d19e5ff6ab72886818c3f680d1bf4965cf0283e4a7de13bc2c2c687

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=sha256:17e5c1b2f4fe0a3a40db811e7bf83d5824d63df5dfd2c57ae37022ca20749fb5

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=sha256:430f6f64e88b7e3ebd30617fee1b95ee79cfd9ce1a1fc13c73da6223a41de893

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:a009765edcf158ef218f2aee4e6a474b2075c4d97db1e3693d6d1e3c9241c7bb

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-14T04:20:55.896534Z digest=sha256:eb88a11b0ed017509b099b93b8fae518dbd560d6366945d504563f1412478620

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-14T04:20:55.901458Z digest=sha256:a390b665ad1a65497bccc35b19a6d66ae3ba062c1d95dbfdb59822b28dcc2c30

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=sha256:739b029c59f18e35469117d130d29f0de1359312e71e2bb69872bc474a69cf32

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:cd6414bfb6511332715a189d0b5d00ffba6f68ac1bac80b8ef15d18cef843099

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=sha256:1c98e064e622267f92703bc14e932934884891c7c7b13bae7aae4874b3582840

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:a672ab8eb73bc48c409ded0f04870b1ea5f8096f5fc230cac720200c198d1405

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:c1b8c27ed333fc3f920cef8267b7a65de3f0874fe90c10d5f383d7966a28391d

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=sha256:4054cbda71d94005a89462fa32c68451c21f51bb64376e5ac49ac5907898818c

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=sha256:666e367194cbfab3c28fbc3c5a36b3b676588852152ba388454a6f55112586fb

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=sha256:77e72f4237af9093ac2d3e0464d6d91165a31b0b4b55594324358cd323ef6835

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:c487948634202051d8a6c7cfa0d322645897f4b603ed28b5e4147c5c91395647

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-14T04:20:55.957840Z digest=sha256:f525c55b489dd86ebc6e33e38cc9cf5e972164686cec48db149ada70f5f19fda

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=sha256:04b5f3a6b70107f269d8812487867be236154ee3e63849cfe735054c6b47df11

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=sha256:61276d4d91ac18007594825aee3a68e6a3e0c196b19260284206d1ef95a9708b

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=sha256:8ae2fbd1fc32505efb1eeb4783ca2f197c20be23fb32e50a709e30ead1b4fdb4

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:e120af8a3b412dfa1a25d02a4864b5504019c18cc4b04a436f311781473a5f4e

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=sha256:3bb5a3792296175d6bf498fccc936a0c09a9b7a0a6e9cfd3e63944594eb29584

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:d72cf95009df3f04b4de7b79d5edcdd8d129a968b60b0e5f2746ae10f8f705de

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:e12499dc4d06712ab40792b942b238ab5730a630fe3464a0e3ad8a0b32e651c0

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=sha256:70a7748a48473b6cf70a2a328d3ea173df5b6bea3fdfc3d80e994c67931b8fdb

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=sha256:62d36596ecd7ad60ea2b5330a71235a6961d2beef423950b49df7bfa9540bed0

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:a73a1ade2aa4e691c19046a25ceb9d60e52da08763e64d7d70b3f697d94b174d

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=sha256:1c027c6b34a1b36f69695709ff95163f68c628dff6bb445240b87687304de2d8

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

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source=pdf_text observed=2026-08-14T04:20:56.031848Z digest=sha256:e9a9c178c2b252e87dbba371a3131118e3827cb98a48d010827cde88382fc940

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=sha256:22fb645a605ce3eaa55a0ddb63509ff56b554d28fdb131895cb892243609ca2c

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=sha256:0fc15875efaccc2743b7f0d0b842f9ff2f168659ba11d40d7062e9a1cec4f8c0

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=sha256:9fb7c8c459bd616c58f05c5527baba2219aad7bd13147818151614a01b5da840

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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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=sha256:5dcb52eedc87e09c2d6ce9caea8a8a8f3d9db04779fa7e5b2133b7877889d337

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

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

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

Reference 78

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T04:20:56.061911Z digest=sha256:52c8f58d5a0d8e52936661b46d346b9d286e17dd1a900344074a923bac820b23

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:e354bfe978bb4692b9280958bd9191f26246df4fca666f41954b1d01550e5533

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=sha256:1a430985585e24ab5f047f99befb296ab37ab10d0634dbbc3979360bca7c025d

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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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:c4b6e8da8f1d8e570b49016932a47d1cf72275ba31cae08e4fa4e0399814acfd

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:d7cbf9a5a39badd761c00cd4824f305fe1585a35a48f4af2a5b6755c95aed282

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=sha256:2689a8c73cfd3adf567401be26c3947a3e4285a5fb97a71860689d8e39702aef

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-14T04:20:56.101186Z digest=sha256:c55d8c01bfd33dbf58c15ae32b62ee34cbe8c48db9501d3e3c79eb26f2ba6068

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

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source=pdf_text observed=2026-08-14T04:20:56.106943Z digest=sha256:603638328358830864d2205c1730121f643660036876d16da42c31823f5b3a7a

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:f31783e7d093328fe7f0b8864129f88dee23b803727b1c1dea4d907a01ad5b5e

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

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

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

Reference 87

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

Source-reported events for the cited work

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source=pdf_text observed=2026-08-14T04:20:56.119611Z digest=sha256:e8c5dedd3a3a318e8aa968f792e269838cb4764fdd138ed72f28e093c95fa1a7

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=sha256:57f15d83ee72a7fa8e00e5fae40b4355967bd0f025a0af20f0d4342b0454e356

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:cd511cceb6225d5836acfd11a5ff29a31a862a7fa1c418c474dc6825ef711423

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

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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:c2aac9619e0bd377a8b84896a73d81c7e2338c271f1305ff38c5dccd70fc1857

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=sha256:8798dd817f73e1589b2d993fa60cb1e3a35d569b3762697dbbff762e3e5d2cb1

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-14T04:20:56.145009Z digest=sha256:422d3de0e751521d5166db5070f06cd253397077b916b9fb1a04ec4a3b9993f7

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-14T04:20:56.150727Z digest=sha256:9b125d285f3bf60357f62bd4a493a7d990364f93de05eb157208aa43fda8f879

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-14T04:20:56.158128Z digest=sha256:da721f13b3dfa425632609f07176c7b33b61bb385a09db5bb0f0c909fa11b5cf

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:b7d47ea2d3b2b79443c7c8b26b11b16fe8dc3efb8f130baf3f27d9ebb2161440

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=sha256:2a50f7591bce1583a43612ff22bc74c620beca64d1ba4af1b46344013b78d4cb

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-14T04:20:56.174887Z digest=sha256:7c2bf418d361d9e5c1bd2067d03f773f0cbc559f90e8d4dc25d2d2e81b18b712

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:a73bde12cdb51e5d1d2fe4e174f808eb7cab5ee20e9a204f94e733b4ba4dd82d

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=sha256:58f36413e4f700158c93166a71cb192bd8fc06eb00419df81ffdf09540eefb73

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:f45eeeafa97d359e9dae13c7c4c01a2f2036515240efcd886faedb4c310b9765

Pith citing papers

No inbound Pith citation observations are available.