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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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Detalles Bibliográficos
Autores principales: Staykov, Kalin V., Popchev, Dimitar, Doneva, Daniela D., Yazadjiev, Stoytcho S.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Berlin Heidelberg 2018
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6061109/
https://www.ncbi.nlm.nih.gov/pubmed/30100815
http://dx.doi.org/10.1140/epjc/s10052-018-6064-x