Static and slowly rotating neutron stars in scalar–tensor theory with self-interacting massive scalar field

Binary pulsar observations and gravitational wave detections seriously constrained scalar–tensor theories with massless scalar field allowing only small deviations from general relativity. If we consider a nonzero mass of the scalar field, though, significant deviations from general relativity are a...

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Published inThe European physical journal. C, Particles and fields Vol. 78; no. 7; pp. 586 - 8
Main Authors Staykov, Kalin V., Popchev, Dimitar, Doneva, Daniela D., Yazadjiev, Stoytcho S.
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 01.07.2018
Springer
Springer Nature B.V
SpringerOpen
Subjects
Astronomy
Astrophysics and Cosmology
Binary stars
Elementary Particles
Gravitation theory
Gravitational waves
Hadrons
Heavy Ions
Measurement Science and Instrumentation
Neutron stars
Nuclear Energy
Nuclear Physics
Parameters
Physics
Physics and Astronomy
Pulsars
Quantum Field Theories
Quantum Field Theory
Regular - Theoretical Physics
Regular Article - Theoretical Physics
Relativity
Stellar rotation
Stratosphere
String Theory
Theory of relativity
Online AccessGet full text
ISSN1434-6044
1434-6052
DOI10.1140/epjc/s10052-018-6064-x

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Abstract Binary pulsar observations and gravitational wave detections seriously constrained scalar–tensor theories with massless scalar field allowing only small deviations from general relativity. If we consider a nonzero mass of the scalar field, though, significant deviations from general relativity are allowed for values of the parameters that are in agreement with the observations. In the present paper we extend this idea and we study scalar–tensor theory with massive field with self-interaction term in the potential. The additional term suppresses the scalar field in the neutron star models in addition to the effect of the mass of the scalar field but still, large deviations from pure GR can be observed for values of the parameters that are in agreement with the observations.
AbstractList Binary pulsar observations and gravitational wave detections seriously constrained scalar–tensor theories with massless scalar field allowing only small deviations from general relativity. If we consider a nonzero mass of the scalar field, though, significant deviations from general relativity are allowed for values of the parameters that are in agreement with the observations. In the present paper we extend this idea and we study scalar–tensor theory with massive field with self-interaction term in the potential. The additional term suppresses the scalar field in the neutron star models in addition to the effect of the mass of the scalar field but still, large deviations from pure GR can be observed for values of the parameters that are in agreement with the observations.
Binary pulsar observations and gravitational wave detections seriously constrained scalar-tensor theories with massless scalar field allowing only small deviations from general relativity. If we consider a nonzero mass of the scalar field, though, significant deviations from general relativity are allowed for values of the parameters that are in agreement with the observations. In the present paper we extend this idea and we study scalar-tensor theory with massive field with self-interaction term in the potential. The additional term suppresses the scalar field in the neutron star models in addition to the effect of the mass of the scalar field but still, large deviations from pure GR can be observed for values of the parameters that are in agreement with the observations.Binary pulsar observations and gravitational wave detections seriously constrained scalar-tensor theories with massless scalar field allowing only small deviations from general relativity. If we consider a nonzero mass of the scalar field, though, significant deviations from general relativity are allowed for values of the parameters that are in agreement with the observations. In the present paper we extend this idea and we study scalar-tensor theory with massive field with self-interaction term in the potential. The additional term suppresses the scalar field in the neutron star models in addition to the effect of the mass of the scalar field but still, large deviations from pure GR can be observed for values of the parameters that are in agreement with the observations.
Abstract Binary pulsar observations and gravitational wave detections seriously constrained scalar–tensor theories with massless scalar field allowing only small deviations from general relativity. If we consider a nonzero mass of the scalar field, though, significant deviations from general relativity are allowed for values of the parameters that are in agreement with the observations. In the present paper we extend this idea and we study scalar–tensor theory with massive field with self-interaction term in the potential. The additional term suppresses the scalar field in the neutron star models in addition to the effect of the mass of the scalar field but still, large deviations from pure GR can be observed for values of the parameters that are in agreement with the observations.
ArticleNumber 586
Audience Academic
Author Popchev, Dimitar
Staykov, Kalin V.
Doneva, Daniela D.
Yazadjiev, Stoytcho S.
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  surname: Popchev
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  organization: Theoretical Astrophysics, Eberhard Karls University of Tübingen, INRNE, Bulgarian Academy of Sciences
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  givenname: Stoytcho S.
  surname: Yazadjiev
  fullname: Yazadjiev, Stoytcho S.
  organization: Department of Theoretical Physics, Faculty of Physics, Sofia University, Institute of Mathematics and Informatics, Bulgarian Academy of Sciences
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Snippet Binary pulsar observations and gravitational wave detections seriously constrained scalar–tensor theories with massless scalar field allowing only small...
Binary pulsar observations and gravitational wave detections seriously constrained scalar-tensor theories with massless scalar field allowing only small...
Abstract Binary pulsar observations and gravitational wave detections seriously constrained scalar–tensor theories with massless scalar field allowing only...
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SubjectTerms Astronomy
Astrophysics and Cosmology
Binary stars
Elementary Particles
Gravitation theory
Gravitational waves
Hadrons
Heavy Ions
Measurement Science and Instrumentation
Neutron stars
Nuclear Energy
Nuclear Physics
Parameters
Physics
Physics and Astronomy
Pulsars
Quantum Field Theories
Quantum Field Theory
Regular - Theoretical Physics
Regular Article - Theoretical Physics
Relativity
Stellar rotation
Stratosphere
String Theory
Theory of relativity
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Title Static and slowly rotating neutron stars in scalar–tensor theory with self-interacting massive scalar field
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