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Prospects of identifying the presence of Strange Stars using Gravitational Waves from binary systems
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SSs still remain degenerate with NSs in high mass range (see fig. 1), making them indistinguishable even with future precise mass-radius measurements.
Current astronomical observations cannot definitively distinguish strange quark stars from neutron stars
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- Link
- https://arxiv.org/abs/2311.15745
- Archived copy
- https://web.archive.org/web/20250829180226/https://arxiv.org/abs/2311.15745
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- Facts checked
- Nov 9, 2026
History 2
- Nov 9, 2026FactsFacts fetcher · Facts looked up
- Aug 4, 2026Entered the graphEntered the graph; no copy stored