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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...
| Autores principales: | , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Springer Berlin Heidelberg
2018
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| 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 |