Moment of inertia–mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field

Abstract We are investigating universal relations between different normalisations of the moment of inertia and the compactness of neutron stars in slow rotation approximation. We study the relations in particular class of massive scalar-sensor theories with self-interaction, for which significant d...

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Main Authors: Dimitar Popchev, Kalin V. Staykov, Daniela D. Doneva, Stoytcho S. Yazadjiev
Format: Article
Language:English
Published: SpringerOpen 2019-02-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-019-6691-x
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spelling doaj-22459683607442b39ea380ca450c9dd62020-11-25T02:21:17ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522019-02-0179211110.1140/epjc/s10052-019-6691-xMoment of inertia–mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar fieldDimitar Popchev0Kalin V. Staykov1Daniela D. Doneva2Stoytcho S. Yazadjiev3Department of Theoretical Physics, Faculty of Physics, Sofia UniversityDepartment of Theoretical Physics, Faculty of Physics, Sofia UniversityTheoretical Astrophysics, Eberhard Karls University of TübingenDepartment of Theoretical Physics, Faculty of Physics, Sofia UniversityAbstract We are investigating universal relations between different normalisations of the moment of inertia and the compactness of neutron stars in slow rotation approximation. We study the relations in particular class of massive scalar-sensor theories with self-interaction, for which significant deviations from General Relativity are allowed for values of the parameters that are in agreement with the observations. Moment of inertia-compactness relations are examined for different normalisation of the moment of inertia. It is shown that for all studied cases the deviations from EOS universality are small for the examined equations of state. On the other hand the scalarization can lead to large deviations from the general relativistic universal relations for values of the parameters that are in agreement with the current observations that can be potentially used to set further test the scalar-tensor theories.http://link.springer.com/article/10.1140/epjc/s10052-019-6691-x
collection DOAJ
language English
format Article
sources DOAJ
author Dimitar Popchev
Kalin V. Staykov
Daniela D. Doneva
Stoytcho S. Yazadjiev
spellingShingle Dimitar Popchev
Kalin V. Staykov
Daniela D. Doneva
Stoytcho S. Yazadjiev
Moment of inertia–mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field
European Physical Journal C: Particles and Fields
author_facet Dimitar Popchev
Kalin V. Staykov
Daniela D. Doneva
Stoytcho S. Yazadjiev
author_sort Dimitar Popchev
title Moment of inertia–mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field
title_short Moment of inertia–mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field
title_full Moment of inertia–mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field
title_fullStr Moment of inertia–mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field
title_full_unstemmed Moment of inertia–mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field
title_sort moment of inertia–mass universal relations for neutron stars in scalar-tensor theory with self-interacting massive scalar field
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2019-02-01
description Abstract We are investigating universal relations between different normalisations of the moment of inertia and the compactness of neutron stars in slow rotation approximation. We study the relations in particular class of massive scalar-sensor theories with self-interaction, for which significant deviations from General Relativity are allowed for values of the parameters that are in agreement with the observations. Moment of inertia-compactness relations are examined for different normalisation of the moment of inertia. It is shown that for all studied cases the deviations from EOS universality are small for the examined equations of state. On the other hand the scalarization can lead to large deviations from the general relativistic universal relations for values of the parameters that are in agreement with the current observations that can be potentially used to set further test the scalar-tensor theories.
url http://link.springer.com/article/10.1140/epjc/s10052-019-6691-x
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AT danieladdoneva momentofinertiamassuniversalrelationsforneutronstarsinscalartensortheorywithselfinteractingmassivescalarfield
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