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 |
|---|---|
| Main Authors | , , , , |
| Format | Journal Article |
| Language | English |
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Berlin/Heidelberg
Springer Berlin Heidelberg
01.07.2017
Springer Springer Nature B.V SpringerOpen |
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| 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 matter is obtained from the density dependent M3Y effective nucleon–nucleon interaction. We consider the dark matter particle mass of 1 GeV. The EoS of self-interacting dark matter is taken from two-body repulsive interactions of the scale of strong interactions. We explore the conditions of equal and different rotational frequencies of nuclear matter and dark matter and find that the maximum mass of differentially rotating stars with self-interacting dark matter to be
∼
1.94
M
⊙
with radius
∼
10.4
km. |
|---|---|
| AbstractList | 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 obtained from the density dependent M3Y effective nucleon–nucleon interaction. We consider the dark matter particle mass of 1 GeV. The EoS of self-interacting dark matter is taken from two-body repulsive interactions of the scale of strong interactions. We explore the conditions of equal and different rotational frequencies of nuclear matter and dark matter and find that the maximum mass of differentially rotating stars with self-interacting dark matter to be ∼1.94M⊙ with radius ∼10.4 km. 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 obtained from the density dependent M3Y effective nucleon–nucleon interaction. We consider the dark matter particle mass of 1 GeV. The EoS of self-interacting dark matter is taken from two-body repulsive interactions of the scale of strong interactions. We explore the conditions of equal and different rotational frequencies of nuclear matter and dark matter and find that the maximum mass of differentially rotating stars with self-interacting dark matter to be ∼ 1.94 M ⊙ with radius ∼ 10.4 km. 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 obtained from the density dependent M3Y effective nucleon-nucleon interaction. We consider the dark matter particle mass of 1 GeV. The EoS of self-interacting dark matter is taken from two-body repulsive interactions of the scale of strong interactions. We explore the conditions of equal and different rotational frequencies of nuclear matter and dark matter and find that the maximum mass of differentially rotating stars with self-interacting dark matter to be [Formula omitted] with radius [Formula omitted] km. 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 matter is obtained from the density dependent M3Y effective nucleon–nucleon interaction. We consider the dark matter particle mass of 1 GeV. The EoS of self-interacting dark matter is taken from two-body repulsive interactions of the scale of strong interactions. We explore the conditions of equal and different rotational frequencies of nuclear matter and dark matter and find that the maximum mass of differentially rotating stars with self-interacting dark matter to be $${\sim }1.94 \;\mathrm{M}_\odot $$ ∼ 1.94 M ⊙ with radius $${\sim }10.4$$ ∼ 10.4 km. |
| ArticleNumber | 440 |
| Audience | Academic |
| Author | Samanta, C. Imam, Kouser Basu, D. N. Atta, Debasis Mukhopadhyay, Somnath |
| Author_xml | – sequence: 1 givenname: Somnath surname: Mukhopadhyay fullname: Mukhopadhyay, Somnath organization: Variable Energy Cyclotron Centre, HBNI – sequence: 2 givenname: Debasis surname: Atta fullname: Atta, Debasis organization: Variable Energy Cyclotron Centre, HBNI, Government General Degree College – sequence: 3 givenname: Kouser surname: Imam fullname: Imam, Kouser organization: Variable Energy Cyclotron Centre, HBNI, Department of Physics, Aliah University – sequence: 4 givenname: D. N. surname: Basu fullname: Basu, D. N. email: dnb@vecc.gov.in organization: Variable Energy Cyclotron Centre, HBNI – sequence: 5 givenname: C. surname: Samanta fullname: Samanta, C. organization: Department of Physics and Astronomy, Virginia Military Institute |
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| Snippet | The masses and radii of non-rotating and rotating configurations of pure hadronic stars mixed with self-interacting fermionic asymmetric dark matter are... Abstract The masses and radii of non-rotating and rotating configurations of pure hadronic stars mixed with self-interacting fermionic asymmetric dark matter... |
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| SubjectTerms | Astronomy Astrophysics and Cosmology Dark matter Density Elementary Particles Equations of state Hadrons Heavy Ions Measurement Science and Instrumentation Nuclear Energy Nuclear matter Nuclear Physics Particle mass Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Regular Article - Theoretical Physics Relativity Stars Stellar rotation Stellar structure String Theory Strong interactions (field theory) |
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| Title | Compact bifluid hybrid stars: hadronic matter mixed with self-interacting fermionic asymmetric dark matter |
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