Radial stability analysis of the continuous pressure gravastar (CROSBI ID 173970)
Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Horvat, Dubravko ; Ilijić, Saša ; Marunović, Anja
engleski
Radial stability analysis of the continuous pressure gravastar
Radial stability of the continuous pressure gravastar is studied using the conventional Chandrasekhar method. The equation of state for the static gravastar solutions is derived and Einstein equations for small perturbations around the equilibrium are solved as an eigenvalue problem for radial pulsations. Within the model there exists a set of parameters leading to a stable fundamental mode, thus proving the radial stability of the continuous pressure gravastar. It is also shown that the central energy density possesses an extremum in ρ_c(R) curve which represents a splitting point between stable and unstable gravastar configurations. As such the ρ_c(R) curve for the gravastar mimics the famous M(R) curve for a polytrope. Together with the former axial stability calculations this work completes the stability problem of the continuous pressure gravastar.
gravastar; radial stability; pulsations; anisotropic pressures
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Podaci o izdanju
28 (19)
2011.
195008-195021
objavljeno
0264-9381
10.1088/0264-9381/28/19/195008