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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

On the radial stability of ultra-compact Schwarzschild stars beyond the Buchdahl limit

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Posada, Camilo [1, 2] ; Chirenti, Cecilia [3]
Total Authors: 2
[1] Silesian Univ Opava, Fac Philosophy & Sci, Inst Phys, Bezrucovo Nam 13, CZ-74601 Opava - Czech Republic
[2] Silesian Univ Opava, Res Ctr Theoret Phys & Astrophys, Bezrucovo Nam 13, CZ-74601 Opava - Czech Republic
[3] Univ Fed Abc, Ctr Math Computat & Cognit, Av Estados 5001, BR-09210580 Santo Andre, SP - Brazil
Total Affiliations: 3
Document type: Journal article
Source: Classical and Quantum Gravity; v. 36, n. 6 MAR 21 2019.
Web of Science Citations: 5

In this paper we used the theory of adiabatic radial oscillations developed by Chandrasekhar to study the conditions for dynamical stability of constant energy-density stars, or Schwarzschild stars, in the unstudied ultra compact regime beyond the Buchdahl limit, that is, for configurations with radius R in the range R-S < R < (9/8)R-S, where R-S is the Schwarzschild radius of the star. These recently found analytical solutions exhibit a negative pressure region in their centre and, in the limit when R -> R-S, the full interior region of the star becomes filled with negative pressure. Here we present a systematic analysis of the stability of these configurations against radial perturbations. We found that, contrary to the usual expectation found in many classical works, the ultra compact Schwarzschild star is stable against radial oscillations. We computed values of the critical adiabatic index gamma(c) for several stellar models with varying radius R/Rs and found that it also approaches a finite value as R/R-S -> 1. (AU)

FAPESP's process: 15/50421-8 - Gravitational waves and neutron star oscillations
Grantee:Cecilia Bertoni Martha Hadler Chirenti
Support type: Regular Research Grants