Results 11 to 20 of about 1,345 (236)
Quark formation and phenomenology in binary neutron-star mergers using V-QCD [PDF]
SciPost Physics, 2022 Samuel D. Tootle +5 more
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Hybrid and quark star matter based on a nonperturbative equation of state [PDF]
Physical Review D, 2020 Konstantin Otto +2 more
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Quark condensate and chiral symmetry restoration in neutron stars
Physics Letters B, 2022 Based on an equivparticle model, we investigate the in-medium quark condensate in neutron stars. Carrying out a Taylor expansion of the nuclear binding energy to the order of ρ3, we obtain a series of EOSs for neutron star matter, which are confronted ...
Hao-Miao Jin +3 more
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Structure of Quark Stars [PDF]
Proceedings of the International Astronomical Union, 2012 AbstractThis paper gives an brief overview of the structure of hypothetical strange quarks stars (quark stars, for short), which are made of absolutely stable 3-flavor strange quark matter. Such objects can be either bare or enveloped in thin nuclear crusts, which consist of heavy ions immersed in an electron gas.
Weber, Fridolin +3 more
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From quark stars to hybrid stars [PDF]
Physics Letters B, 2001 10 pages, 4 figures, 1 ...
DRAGO, Alessandro, A. Lavagno
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Dark matter effects on hybrid star properties
European Physical Journal C: Particles and Fields, 2023 In the present work, we investigate the effects of dark matter (DM) on hybrid star properties. We assume that dark matter is mixed with both hadronic and quark matter and interacts with them through the exchange of a Higgs boson.
C. H. Lenzi +4 more
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Strange Quark Star (SQS) in Tolman IV potential with density dependent B-parameter and charge
European Physical Journal C: Particles and Fields, 2022 In this paper, the solutions of Einstein–Maxwell Field Equations for relativistic strange quark star in Tolman-IV potential considering MIT bag model EoS $$p=\frac{1}{3}(\rho -4B)$$ p = 1 3 ( ρ - 4 B ) of interior matter in presence of charge in higher ...
K. B. Goswami +3 more
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MASSIVE COMPACT STARS AS QUARK STARS [PDF]
The Astrophysical Journal, 2011 26 pages, 8 figures,The Astrophysical Journal (2011)
Rodrigues, Hilario +2 more
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DISTINGUISHING BARE QUARK STARS FROM NEUTRON STARS [PDF]
International Journal of Modern Physics A, 2004 Observations to date cannot distinguish neutron stars from self-bound bare quark stars on the basis of their gross physical properties such as their masses and radii alone. However, their surface luminosity and spectral characteristics can be significantly different.
Jaikumar, P. +3 more
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QUARK MATTER SYMMETRY ENERGY AND QUARK STARS [PDF]
The Astrophysical Journal, 2013 We extend the confined-density-dependent-mass (CDDM) model to include isospin dependence of the equivalent quark mass. Within the confined-isospin-density-dependent-mass (CIDDM) model, we study the quark matter symmetry energy, the stability of strange quark matter, and the properties of quark stars.
Chu, Peng-Cheng, Chen, Lie-Wen
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