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Paper Citation Record · LEDGER

Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2401.14419.

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

pith.paper-citation-record.v1
2401.14419 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T11:42:10.498108Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T10:26:51.931712Z

Reference resolution

0 of 0 outbound references displayed

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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 47848b48-bc81-4472-a4c2-ea184dad4fc7 · inbound

Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model cites this paper.

Role of density profile of sub-GeV dark matter in the properties of dark matter admixed quark stars with Bayesian analysis of dark-NJL model Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-05T11:42:10.498108Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T11:42:10.498108Z digest=sha256:850b8fbda7e2b7550e98cdb0534500b682e2cafcfe09273a20248ce8d6a9f9c9

Observation 86fd4488-9d14-4d40-bf3a-d47c25d4e928 · inbound

Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach cites this paper.

Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars

Reference 32

Resolution
verified exact
arxiv_id, observed 2026-05-17T23:12:12.107139Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

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Observation 1ed02391-5c73-4d77-b855-268e10f75cba · inbound

Bayesian analysis of density profile of light dark matter elucidating the properties of dark matter admixed neutron stars in the presence of hyperons cites this paper.

Bayesian analysis of density profile of light dark matter elucidating the properties of dark matter admixed neutron stars in the presence of hyperons Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars

Reference 55

Resolution
verified exact
arxiv_id, observed 2026-05-15T01:48:28.105554Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-15T01:47:28.438537Z digest=sha256:d9e86174864fa837a6676562cecd20bf384a058645a6f3f94c8f3a1e78cf0eaa

Observation c30a521c-ec8e-4c75-b09c-c65247c847c1 · inbound

First Constraints on the Ellipticities of Self-Interacting Fermionic Dark Matter Admixed Neutron Stars from Continuous Gravitational-Wave Searches cites this paper.

First Constraints on the Ellipticities of Self-Interacting Fermionic Dark Matter Admixed Neutron Stars from Continuous Gravitational-Wave Searches Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars

Reference 76

Resolution
metadata mismatch
arxiv_id, observed 2026-07-02T10:26:51.933241Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-28T05:03:42.639549Z digest=sha256:5d830c7f6b6a8f21eafae074f4d5621562ed761e2b74d4cc37d55c1f66bb1aef

Observation 70b6403c-7fc2-4704-bfbf-1cb7c93173f4 · inbound

A self-consistent single-fluid framework for neutron stars admixed with mirror dark matter cites this paper.

A self-consistent single-fluid framework for neutron stars admixed with mirror dark matter Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars

Reference 38

Resolution
verified exact
arxiv_id, observed 2026-07-02T08:46:48.757241Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-07-02T08:36:45.802728Z digest=sha256:28b05644e373c18eaef8174535b2040c2525c4687a1c135b7202e7b5a53494e6

Observation 251903a7-81a6-47fb-8c9a-f9709682393c · inbound

Effects of Differential Rotation on the Maximum Mass of Neutron Stars cites this paper.

Effects of Differential Rotation on the Maximum Mass of Neutron Stars Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars

Reference 31

Resolution
unresolved
no resolver link, observed 2026-07-13T00:48:43.602495Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T00:48:43.602495Z digest=sha256:37adafa2b0ff35b7602e44c0b5adb1f923c580c234bfe73aa28ba1f9b9b6e577

Observation 4f493561-2330-4b16-b51f-b34882b250a0 · inbound

Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach cites this paper.

Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars

Reference 48

Resolution
unresolved
no resolver link, observed 2026-07-13T05:17:12.889672Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T05:17:12.889672Z digest=sha256:4b9f06cf9eb7e4c8b66553749923694b899f0b0cc0bf76ad2b42d91e4bb13a5a