Results 41 to 50 of about 200,989 (232)
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
doaj +1 more source
Model study of a quark star [PDF]
Physical Review D, 2011 14 pages, 6 figures, 1 ...
Xin-Lian Luo +3 more
openaire +3 more sources
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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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.
openaire +4 more sources
ANALYTICAL MODELS FOR QUARK STARS [PDF]
International Journal of Modern Physics D, 2007 We find two new classes of exact solutions to the Einstein–Maxwell system of equations. The matter content satisfies a linear equation of state consistent with quark matter; a particular form of one of the gravitational potentials is specified to generate solutions.
Komathiraj, K., Maharaj, S.D.
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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
doaj +1 more source
The Hadron-quark Crossover in Neutron Star within Gaussian Process Regression Method
The Astrophysical Journal, 2022 The equations of state of the neutron star at the hadron-quark crossover region are interpolated with the Gaussian process regression (GPR) method, which can reduce the randomness of present interpolation schemes.
Kaixuan Huang +3 more
doaj +1 more source
Can stellar mass black holes be quark stars? [PDF]
MNRAS, 400, pp. 1632-1642 (2009), 2009 We investigate the possibility that stellar mass black holes, with masses in the range of $3.8M_{\odot}$ and $6M_{\odot}$, respectively, could be in fact quark stars in the Color-Flavor-Locked (CFL) phase. Depending on the value of the gap parameter, rapidly rotating CFL quark stars can achieve much higher masses than standard neutron stars, thus ...
arxiv +1 more source
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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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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