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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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Title: XTE J1814-338 as a dark matter admixed neutron star0 passages
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As quoted
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.
Pulse profile modeling of XTE J1814-338's thermonuclear burst oscillations yields a radius near 7 km and a mass near 1.2 solar masses
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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
- Nov 11, 2026DividedSegmenter · Divided into 110 parts by its own structure
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- Nov 11, 2026Entered the graphEntered the graph; copy stored
- Nov 4, 2026Correction watchCorrection watcher · Watched by DOI; no notice found