Paper Citation Record · LEDGER

A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2306.15721.

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

pith.paper-citation-record.v1
2306.15721 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T00:43:19.007075Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T03:25:57.985957Z

Reference resolution

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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 54025213-8dfa-4550-a6c4-4dad11b0c4f3 · inbound

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

Neutrino pair annihilation driven jets from black-hole torus systems A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T11:41:25.596984Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 948bd4d9-8bd4-4fea-aa1f-41641fa81462 · 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 A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 118

Resolution: unresolved; no resolver link, observed 2026-08-05T15:52:56.778356Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 472a62ab-0264-4748-9349-c8839e4024b5 · inbound

Impact of rotation on magnetic field stability and orientation in isolated neutron stars cites this paper.

Impact of rotation on magnetic field stability and orientation in isolated neutron stars A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-05T15:20:07.250670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation efbb05a8-8fb6-4f5b-96e1-9418cbfe4193 · inbound

Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities cites this paper.

Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-18T15:51:34.905131Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 74f70d1a-15a5-4f41-95da-6922693d94ec · inbound

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

A magnetar formation in binary neutron star merger A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 64

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:37:44.741768Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation a08ae143-065a-4c0b-a9ca-1e352c513da7 · 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 A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-07-03T13:08:08.638650Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation cd099fd4-566d-4830-9968-e28f76c20cf5 · inbound

Impact of neutrino-electron scattering and an improved treatment of pair processes on binary neutron star mergers cites this paper.

Impact of neutrino-electron scattering and an improved treatment of pair processes on binary neutron star mergers A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-07-01T18:45:59.285966Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation e6a8e5b1-e4dd-4eb1-a46e-701e618a5330 · 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 A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 94

Resolution: verified exact; local_arxiv, observed 2026-07-09T03:25:57.987296Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 256f9135-e8dd-444b-8467-a40dfb0cdca3 · inbound

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity cites this paper.

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 28

Resolution: unresolved; no resolver link, observed 2026-07-14T15:02:35.854356Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 35cf3bd3-d109-453e-af1a-96b96af0e8c6 · inbound

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

Transport Properties of the MRI in Differentially Rotating Neutron Stars A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 15

Resolution: unresolved; no resolver link, observed 2026-07-31T14:28:12.579986Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a469e390-f80f-4f34-a5e4-35072b5ea4ca · 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 A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-08T00:43:19.007075Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.