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Paper Citation Record · LEDGER

Magnetic energy production by turbulence in binary neutron star mergers

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1303.1450.

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

pith.paper-citation-record.v1
1303.1450 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T11:35:56.297860Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T11:35:57.809788Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 da9a478e-098d-4891-8f1b-36f4671847e7 · inbound

Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties cites this paper.

Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties Magnetic energy production by turbulence in binary neutron star mergers

Reference 64

Resolution
verified exact
local_arxiv, observed 2026-08-14T11:35:57.815472Z

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=2026-08-14T11:35:56.297860Z digest=sha256:81f53830ed8e413efa31ff5e3a86cff566be7e405d532b5f96cc623995e9138a

Observation 3d65ada6-a719-414c-8dc6-a6942cfe9603 · inbound

SPH methods in the modelling of compact objects cites this paper.

SPH methods in the modelling of compact objects Magnetic energy production by turbulence in binary neutron star mergers

Reference 207

Resolution
unresolved
no resolver link, observed 2026-08-02T01:02:23.410278Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T01:02:23.410278Z digest=sha256:ea789e9bfe81300b94b33adc626b40ad28e58d4f79bba942389ad1ef97375b3c