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Rescaling strange-cluster stars and its implications on gravitational-wave echoes

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arxiv 2305.13323 v2 pith:E5G2KT6X submitted 2023-05-16 astro-ph.HE gr-qchep-phnucl-th

classification astro-ph.HEgr-qchep-phnucl-th
keywords strangeonstarsmatterrescalingcompactdimensionlessechoechoes
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abstract

Solid states of strange-cluster matter called strangeon matter can form strangeon stars that are highly compact. We show that strangeon matter and strangeon stars can be recast into dimensionless forms by a simple reparametrization and rescaling, through which we manage to maximally reduce the number of degrees of freedom. With this dimensionless scheme, we find that strangeon stars are generally compact enough to feature a photon sphere that is essential to foster gravitational-wave (GW) echoes. Rescaling the dimension back, we illustrate its implications on the expanded dimensional parameter space, and calculate the GW echo frequencies associated with strangeon stars, showing that the minimum echo frequency is $\sim 8$ kHz for empirical parameter space that satisfies the GW170817 constraint, and can reduce to $\mathcal O(100)$ Hertz at the extended limit.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Tidal deformation and strain accumulation of solid compact stars

    astro-ph.HE 2026-07 conditional novelty 5.5 of 10

    Solid strangeon stars of 1.4 Msun differ by ~40% in tidal deformability from fluid counterparts and release up to 10^46 erg via central-peaking strain fracture at hundreds of Hz.

  2. Echoes and quasinormal modes for static loop quantum black bounces

    gr-qc 2026-07 conditional novelty 4.0 of 10

    Scalar perturbations of the loop quantum black bounce spacetime produce echoes in traversable-wormhole configurations with a double-barrier effective potential, but not in regular-black-hole configurations with a sing...

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