J 2019

A causal Schwarzschild-deSitter interior solution by gravitational decoupling

GABBANELLI, Luciano; Jorge Iván OVALLE ARAYA; Adrián SOTOMAYOR; Zdeněk STUCHLÍK; Roberto CASADIO et. al.

Basic information

Original name

A causal Schwarzschild-deSitter interior solution by gravitational decoupling

Authors

GABBANELLI, Luciano (724 Spain); Jorge Iván OVALLE ARAYA (152 Chile, guarantor, belonging to the institution); Adrián SOTOMAYOR (152 Chile); Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution) and Roberto CASADIO (380 Italy)

Edition

European Physical Journal C, 2019, 1434-6044

Other information

Language

English

Type of outcome

Article in a journal

Field of Study

10308 Astronomy

Country of publisher

Germany

Confidentiality degree

is not subject to a state or trade secret

References:

Impact factor

Impact factor: 4.389

RIV identification code

RIV/47813059:19240/19:A0000419

Organization unit

Faculty of Philosophy and Science in Opava

UT WoS

000471346400004

EID Scopus

2-s2.0-85067174290

Keywords in English

gravitational decoupling; cosmological constant; interior solution; astrophysical object

Tags

International impact, Reviewed

Links

GB14-37086G, research and development project.
Changed: 20/3/2020 09:24, RNDr. Jan Hladík, Ph.D.

Abstract

V originále

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 cosmological 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 astrophysical object.