Compact bifluid hybrid stars: hadronic matter mixed with self-interacting fermionic asymmetric dark matter
Abstract The masses and radii of non-rotating and rotating configurations of pure hadronic stars mixed with self-interacting fermionic asymmetric dark matter are calculated within the two-fluid formalism of stellar structure equations in general relativity. The Equation of State (EoS) of nuclear mat...
محفوظ في:
| المؤلفون الرئيسيون: | , , , , |
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| التنسيق: | Artigo |
| اللغة: | Inglês |
| منشور في: |
SpringerOpen
2017-07-01
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| سلاسل: | European Physical Journal C: Particles and Fields |
| الوصول للمادة أونلاين: | http://link.springer.com/article/10.1140/epjc/s10052-017-5006-3 |
| الوسوم: |
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