Özet
We study the structure of spherically symmetric and static objects in the presence of a nonminimally coupled scalar field having a potential of the form V(ϕ)=−μ2ϕ2∕2+λϕ4∕4. We numerically solve equations of the system using two different realistic equations of state for neutron matter and give the mass-radius relations as well as the radial profiles of the scalar field, densities and the mass function for a sample configuration. We show that a specific solution type encountered in such systems causes characteristic neutron star mass-radius relations to turn into the ones belonging to strange quark stars.
| Orijinal dil | İngilizce |
|---|---|
| Makale numarası | 100488 |
| Dergi | Physics of the Dark Universe |
| Hacim | 28 |
| DOI'lar | |
| Yayın durumu | Yayınlandı - May 2020 |
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Publisher Copyright:© 2020 Elsevier B.V.
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