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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2019-02-01
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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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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 |
work_keys_str_mv |
AT dimitarpopchev momentofinertiamassuniversalrelationsforneutronstarsinscalartensortheorywithselfinteractingmassivescalarfield AT kalinvstaykov momentofinertiamassuniversalrelationsforneutronstarsinscalartensortheorywithselfinteractingmassivescalarfield AT danieladdoneva momentofinertiamassuniversalrelationsforneutronstarsinscalartensortheorywithselfinteractingmassivescalarfield AT stoytchosyazadjiev momentofinertiamassuniversalrelationsforneutronstarsinscalartensortheorywithselfinteractingmassivescalarfield |
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