Compact bifluid hybrid stars: hadronic matter mixed with self-interacting fermionic asymmetric dark matter
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 matter is ob...
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Published in | The European physical journal. C, Particles and fields Vol. 77; no. 7; pp. 1 - 9 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Berlin/Heidelberg
Springer Berlin Heidelberg
01.07.2017
Springer Springer Nature B.V SpringerOpen |
Subjects | |
Online Access | Get full text |
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