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Macroscopic properties of the XTE J1814-338 as a dark matter admixed strange star

Luiz L. LopesAstrophysics and Space SciencePublished Aug 2025doi 10.1007/s10509-025-04472-1 Original︎ ↗

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24 August 20230 passages

Multi-messenger and cosmological constraints on dark matter through two-fluid neutron star modeling1 passage

A unified thermodynamic framework for coextensive dark matter admixed strange stars1 passage

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Bodmer, A.R.: Collapsed nuclei. Phys. Rev. D 4 , 1601–1606 (1971). https://doi.org/10.1103/PhysRevD.4.16011 passage

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Received : 16 April 20250 passages

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DOI : https://doi.org/10.1007/s10509-025-04472-10 passages

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As quoted

In this paper, I discuss the macroscopic properties of the ultracompact object XTE J1814-338, whose inferred mass and radius read M = 1.21 ± 0.05 M⊙ and R = 7.0 ± 0.4 km, as a dark matter-admixed strange star.

Pulse profile modeling of XTE J1814-338's thermonuclear burst oscillations yields a radius near 7 km and a mass near 1.2 solar massesVerified

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Record

Kind: journal article
Authors: Luiz L. Lopes
Publisher: Astrophysics and Space Science
Published: Aug 2025
DOI: 10.1007/s10509-025-04472-1
Link: https://link.springer.com/article/10.1007/s10509-025-04472-1
Archived copy: None found
Stored text: 16,924 characters, retrieved Nov 11, 2026 · 196 sections, 131 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 327 parts by its own structure
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