We employ the minimal geometric deformation approach to gravitational decoupling (MGD-decoupling) in order to build an exact anisotropic version of the Schwarzschild interior solution in a space-time with cosmo- logical constant. Contrary to the well-known Schwarzschild interior, the matter density in the new solution is not uniform and possesses subluminal sound speed. It therefore satisfies all standard physical requirements for a candidate astrophys- ical object.
A causal Schwarzschild-de Sitter interior solution by gravitational decoupling / Gabbanelli, L.; Ovalle, J.; Sotomayor, A.; Stuchlik, Z.; Casadio, R.. - In: THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS. - ISSN 1434-6044. - ELETTRONICO. - 79:6(2019), pp. 486.1-486.9. [10.1140/epjc/s10052-019-7022-y]
A causal Schwarzschild-de Sitter interior solution by gravitational decoupling
Casadio, R.
2019
Abstract
We employ the minimal geometric deformation approach to gravitational decoupling (MGD-decoupling) in order to build an exact anisotropic version of the Schwarzschild interior solution in a space-time with cosmo- logical constant. Contrary to the well-known Schwarzschild interior, the matter density in the new solution is not uniform and possesses subluminal sound speed. It therefore satisfies all standard physical requirements for a candidate astrophys- ical object.File | Dimensione | Formato | |
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