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XTE J1814-338: A potential hybrid star candidate

P. Laskos-Patkos, Ch. C. MoustakidisPhysical Review DPublished Mar 21, 2025doi 10.1103/physrevd.111.063058Original︎ ↗Archived copy

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As quoted

A recent analysis on the properties of the XTE J1814-338 pulsar yielded a small radius value around ~ 7 km. Notably, this estimation is significantly lower compared to the currently inferred values for the radius of neutron stars

As quoted

A recent analysis on the properties of the XTE J1814-338 pulsar yielded a small radius value around ~ 7 km. Notably, this estimation is significantly lower compared to the currently inferred values for the radius of neutron stars.

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Record

Kind
journal article
Authors
P. Laskos-Patkos, Ch. C. Moustakidis
Publisher
Physical Review D
Published
Mar 21, 2025
DOI
10.1103/physrevd.111.063058
Link
https://arxiv.org/abs/2410.18498
Archived copy
https://web.archive.org/web/20260101171959/https://arxiv.org/abs/2410.18498
Stored text
None; quoted passages only
Claims extracted
Not recorded
Versions
One known
Copies
None recorded
Corrections
None recorded
Facts checked
Nov 11, 2026

History 2

  1. Nov 9, 2026FactsFacts fetcher · Facts looked up
  2. Aug 5, 2026Entered the graphEntered the graph; no copy stored
XTE J1814-338: A potential hybrid star candidate · Minerval