HLADÍK, Jan, Zdeněk STUCHLÍK, Gabriel TÖRÖK and Martin URBANEC. Neutrino trapping in extremely compact objects described by the internal Schwarzschild-(anti-)de Sitter spacetimes. General Relativity and Gravitation. US - Spojené státy americké, 2012, vol. 44, No 6, p. 1393-1417. ISSN 0001-7701. Available from: https://dx.doi.org/10.1007/s10714-012-1346-3.
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Basic information
Original name Neutrino trapping in extremely compact objects described by the internal Schwarzschild-(anti-)de Sitter spacetimes
Authors HLADÍK, Jan, Zdeněk STUCHLÍK, Gabriel TÖRÖK and Martin URBANEC.
Edition General Relativity and Gravitation, US - Spojené státy americké, 2012, 0001-7701.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW URL
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1007/s10714-012-1346-3
UT WoS 000304163400002
Keywords in English Extremely compact stars; Neutrino trapping; S(a)dS spacetimes
Tags , GD205-09H033, LC06014, MSM4781305903
Tags International impact, Reviewed
Links GD205/09/H033, research and development project. LC06014, research and development project. MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 7/4/2021 08:25.
Abstract
Extremely compact stars (ECS) (having radius R < 3GM/c 2) contain captured null geodesics. Certain part of neutrinos produced in their interior will be trapped, influencing thus their neutrino luminosity and thermal evolution. The trapping effect has been previously investigated for the internal Schwarzschild spacetimes with the uniform distribution of energy density. Here, we extend our earlier study considering the influence of the cosmological constant ? on the trapping phenomena. Our model for the interior of ECS is based on the internal Schwarzschild-(anti-)de Sitter (S(a)dS) spacetimes with uniform distribution of energy density matched to the external vacuum S(a)dS spacetime with the same cosmological constant. Assuming uniform and isotropic distribution of local neutrino emissivity we determine behavior of the trapping coefficients, i. e., "global" one representing influence on the neutrino luminosity and "local" one representing influence on the cooling process. We demonstrate
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