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On the Stability of Strange Dwarf Hybrid Stars

Journal Article · · Astrophysical Journal
;  [1]
  1. Physics Department, Washington University, St. Louis, MO 63130 (United States)

We investigate the stability of “strange dwarfs”: white-dwarf-sized stars with a density discontinuity between a small dense core of quark matter and a thick low-density mantle of degenerate electrons. Previous work on strange dwarfs suggested that such a discontinuity could stabilize stars that would have been classified as unstable by the conventional criteria based on extrema in the mass–radius relation. We investigate the stability of such stars by numerically solving the Sturm–Liouville equations for the lowest-energy modes of the star. We find that the conventional criteria are correct, and strange dwarfs are not stable.

OSTI ID:
22679803
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 847; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

References (3)

Possible new class of dense white dwarfs conference January 1995
Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity journal January 1964
Quark phases in neutron stars and a "third family" of compact stars as a signature for phase transitions text January 2000

Cited By (7)

Effects of Hadron-Quark Phase Transitions in Hybrid Stars within the NJL Model text January 2019
Tidal deformability with sharp phase transitions in (binary) neutron stars text January 2018
Radial oscillations of quark stars from perturbative QCD journal December 2019
Effects of Hadron-Quark Phase Transitions in Hybrid Stars within the NJL Model journal March 2019
Radial oscillations of quark stars from perturbative QCD text January 2019
Tidal deformability with sharp phase transitions in binary neutron stars journal April 2019
Dark compact objects: An extensive overview journal March 2019

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