Paper Citation Record · LEDGER

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

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2211.07637.

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

pith.paper-citation-record.v1
2211.07637 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:20:55.787498Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T03:25:58.039339Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 044db788-ca5e-40e3-a6a6-3ab134d2b013 · inbound

Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers cites this paper.

Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers 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 101

Resolution: unresolved; no resolver link, observed 2026-08-11T21:29:52.840813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4ab0b023-e700-4257-9986-af1900a5bb36 · inbound

Neutrinos from explosive transients at the dawn of multi-messenger astronomy cites this paper.

Neutrinos from explosive transients at the dawn of multi-messenger astronomy 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 69

Resolution: unresolved; no resolver link, observed 2026-08-11T16:53:00.653267Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3f207911-8ca2-4b7e-a851-2ac53f9db1d3 · inbound

Self-consistent scenario for jet and stellar explosion in collapsar: General relativistic magnetohydrodynamics simulation with dynamo cites this paper.

Self-consistent scenario for jet and stellar explosion in collapsar: General relativistic magnetohydrodynamics simulation with dynamo 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 35

Resolution: unresolved; no resolver link, observed 2026-08-09T13:31:50.243812Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 496ab5c7-4e92-47e1-abf8-ba68bea9114d · inbound

Gravitational Waves from Accretion Disks: Turbulence, Mode Excitation and Prospects for Future Detectors cites this paper.

Gravitational Waves from Accretion Disks: Turbulence, Mode Excitation and Prospects for Future Detectors 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 77

Resolution: unresolved; no resolver link, observed 2026-08-08T11:43:23.424396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 366a9768-d6fc-4009-bde7-92f930f4cc4d · inbound

Neutrino pair annihilation driven jets from black-hole torus systems cites this paper.

Neutrino pair annihilation driven jets from black-hole torus systems 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 40

Resolution: unresolved; no resolver link, observed 2026-08-07T11:41:25.631036Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 31e77647-4eee-4ef8-906c-2552d1d9a0fe · inbound

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta cites this paper.

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta 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 19

Resolution: unresolved; no resolver link, observed 2026-08-05T15:52:56.239812Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 943b6e5d-de70-4e80-a334-e0712c9a1b3b · inbound

A magnetar formation in binary neutron star merger cites this paper.

A magnetar formation in binary neutron star merger 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 63

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:37:44.842095Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation dbfecd1d-5f00-47c7-9dd4-18f6c388d5d9 · inbound

Implementation of multi-grid Poisson solver in numerical relativity and its application to gravitational collapse of massive star cites this paper.

Implementation of multi-grid Poisson solver in numerical relativity and its application to gravitational collapse of massive star 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 11

Resolution: verified exact; arxiv_id, observed 2026-07-03T13:08:08.590532Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 98db1180-da77-4a05-9629-987e53593d30 · inbound

Subsolar-mass binary mergers of strange stars and neutron stars: gravitational waves and ejecta cites this paper.

Subsolar-mass binary mergers of strange stars and neutron stars: gravitational waves and ejecta 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 93

Resolution: verified exact; local_arxiv, observed 2026-07-09T03:25:58.040741Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 0ad88d85-2c63-4da5-8279-95c06d1ca2d8 · inbound

Transport Properties of the MRI in Differentially Rotating Neutron Stars cites this paper.

Transport Properties of the MRI in Differentially Rotating Neutron Stars 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 43

Resolution: unresolved; no resolver link, observed 2026-07-31T14:28:12.727566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b8236d0-a88d-4c27-8a73-4447d6ea4f2e · inbound

From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State cites this paper.

From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State 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 11

Resolution: unresolved; no resolver link, observed 2026-08-08T00:43:18.975565Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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

Reference 32

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.