Results 31 to 40 of about 41,644 (263)
On the conversion of neutron stars into quark stars [PDF]
EPJ Web of Conferences, 2014 The possible existence of two families of compact stars, neutron stars and quark stars, naturally leads to a scenario in which a conversion process between the two stellar objects occurs with a consequent release of energy of the order of $10^{53}$ erg.
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Three-layered compact star in modified Buchdahl-I spatial metric with distinct equations of state
Physics Letters B, 2023 We present a singularity free and smoothly connected complete solution for a three-layered compact star with deconfined quark matter core surrounded by coherent quantum fluid of a Bose-Einstein condensate, all enclosed under a thin envelope of a ...
Shweta Saklany +2 more
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Neutron stars and massive quark matter [PDF]
Progress in Particle and Nuclear Physics, 1996 Using the Color-Dielectric model to describe quark confinement, including strange quarks and accounting for beta--equilibrium, we get masses for a static neutron star in the range $1.3\leq M/M_{\odot}\leq 1.54 $ for a radius $R\approx 9$ km. Rapid cooling through the direct URCA mechanism is obtained.
DRAGO, Alessandro +2 more
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Quark matter in compact stars? [PDF]
Nature, 2007 Ozel, in a recent reanalysis of EXO 0748-676 observational data (astro-ph/0605106), concluded that quark matter probably does not exist in the center of compact stars. We show that the data is actually consistent with the presence of quark matter in compact stars.
Thomas Klähn +6 more
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Constant entropy hybrid stars: a first approximation of cooling evolution [PDF]
, 2017 We aim to study the possibility of a hadron-quark phase transition in the interior of neutron stars, taking into account different schematic evolutionary stages at finite temperature. We also discuss the strange quark matter stability in the quark matter
Mariani, M., Orsaria, M., Vucetich, H.
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Observability of neutron stars with quarks [PDF]
Nuclear Physics A, 2003 4 pages, 1 figure, uses espcrc1.sty (included)
Dany Page +3 more
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Gravitational waves from binary compact star mergers in the context of strange matter
EPJ Web of Conferences, 2018 In this article we will focus on the appearance of the hadron-quark phase transition and the formation of strange matter in the interior region of the hypermassive neutron star and its conjunction with the spectral properties of the emitted gravitational
Hanauske Matthias +4 more
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Particles, 2020 The relativistic mean field (RMF) model of the nuclear matter equation of state was modified by including the effect of Pauli-blocking owing to quark exchange between the baryons.
David Blaschke +2 more
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Recent results on cold-QCD from RHIC [PDF]
EPJ Web of Conferences, 2020 Polarized proton-proton collisions at the Relativistic Heavy Ion Collider (RHIC) provide unique opportunities to study the spin structure of the nucleon.
Xu Qinghua
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Effects of quark matter and color superconductivity in compact stars [PDF]
, 2003 The equation of state for quark matter is derived for a nonlocal, chiral quark model within the mean field approximation. We investigate the effects of a variation of the form factors of the interaction on the phase diagram of quark matter under the ...
Aguilera, D. N. +4 more
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