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Paper Citation Record · LEDGER

Constraining properties of asymmetric dark matter candidates from gravitational-wave observations

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2210.15739.

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pith.paper-citation-record.v1
2210.15739 v1

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measured 8 of 8 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T15:34:12.327013Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T08:54:15.189327Z

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Pith citing papers

Observation 0cdb7ce5-9ea0-41eb-9e54-a6d0b0561f41 · inbound

Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter cites this paper.

Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter Constraining properties of asymmetric dark matter candidates from gravitational-wave observations

Reference 148

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arxiv_id, observed 2026-05-24T08:54:15.192212Z

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Observation 3e9c9e83-911b-4dd5-8770-7186415035be · inbound

Template bank for sub solar mass compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA cites this paper.

Template bank for sub solar mass compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA Constraining properties of asymmetric dark matter candidates from gravitational-wave observations

Reference 79

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Observation 9826028f-8d8d-4e28-ab2b-8fb0955c6827 · inbound

Tidal Love numbers and quasi-normal modes of the Schwarzschild-Hernquist black hole cites this paper.

Tidal Love numbers and quasi-normal modes of the Schwarzschild-Hernquist black hole Constraining properties of asymmetric dark matter candidates from gravitational-wave observations

Reference 42

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Observation a4074b35-0f55-472a-bbea-e417842e156e · inbound

Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter? cites this paper.

Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter? Constraining properties of asymmetric dark matter candidates from gravitational-wave observations

Reference 33

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Observation 3cc7cdb6-66d1-4488-b6b4-918370de961e · inbound

A case study of GW190425 for classifying binary neutron star versus binary black hole mergers and constraining asymmetric dark matter with gravitational wave detectors cites this paper.

A case study of GW190425 for classifying binary neutron star versus binary black hole mergers and constraining asymmetric dark matter with gravitational wave detectors Constraining properties of asymmetric dark matter candidates from gravitational-wave observations

Reference 33

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Observation df618dad-d7f1-49d9-9d74-b5a7c004f878 · inbound

Effect of Dark matter and $\sigma$-cut potential on radial and non-radial oscillation modes in neutron stars cites this paper.

Effect of Dark matter and $\sigma$-cut potential on radial and non-radial oscillation modes in neutron stars Constraining properties of asymmetric dark matter candidates from gravitational-wave observations

Reference 51

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Observation 3f794875-2a6a-46bd-817c-76e1e82586b5 · inbound

Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter cites this paper.

Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter Constraining properties of asymmetric dark matter candidates from gravitational-wave observations

Reference 47

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arxiv_id, observed 2026-05-19T03:47:02.350012Z

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Observation 926640d1-2d71-461b-b5d2-a1a573f538b6 · inbound

Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer cites this paper.

Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer Constraining properties of asymmetric dark matter candidates from gravitational-wave observations

Reference 121

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