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XTE J1814-338 as a dark matter admixed neutron star

Luiz L. Lopes, Adamu IssifuPhysics of the Dark UniversePublished May 2025doi 10.1016/j.dark.2025.101922Original︎ ↗Archived copy

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The recent work of Kini et al. [17], using pulse profile modeling technique to investigate the thermonuclear burst variations from accreting NSs has revealed a striking mass (M) and radius (R) measurement for XTE J1814-338 pulsar.

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Record

Kind
journal article
Authors
Luiz L. Lopes, Adamu Issifu
Publisher
Physics of the Dark Universe
Published
May 2025
DOI
10.1016/j.dark.2025.101922
Link
https://arxiv.org/abs/2411.17105
Archived copy
https://web.archive.org/web/20260708112707/https://arxiv.org/abs/2411.17105
Stored text
4,575 characters, retrieved Nov 11, 2026 · 49 sections, 61 passages
Claims extracted
Not recorded
Versions
One known
Copies
None recorded
Corrections
None recorded
Facts checked
Nov 11, 2026

History 4

  1. Nov 11, 2026DividedSegmenter · Divided into 110 parts by its own structure
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  4. Nov 4, 2026Correction watchCorrection watcher · Watched by DOI; no notice found