Results 111 to 120 of about 648,957 (221)
EPJ Web of Conferences, 2010 We introduce the theoretical basis for modeling the cooling evolution of compact stars starting from Boltzmann equations in curved space-time. We open a discussion on observational verification of different neutron star models by consistent statistics ...
Grigorian H.
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Quark matter and quark stars at finite temperature in Nambu–Jona-Lasinio model
European Physical Journal C: Particles and Fields, 2017 We extend the SU(3) Nambu–Jona-Lasinio (NJL) model to include two types of vector interaction. Using these two types of vector interaction in NJL model, we study the quark symmetry free energy in asymmetric quark matter, the constituent quark mass, the ...
Peng-Cheng Chu +6 more
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Finite corrections to quark fragmentation functions in perturbative QCD [PDF]
, 1979 Baier R, Fey K. Finite corrections to quark fragmentation functions in perturbative QCD. Zeitschrift für Physik C: Particles and fields.
Baier, Rudolf, Fey, K.
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The European Physical Journal C, 2012 From an analogy with non-relativistic degenerate QED plasma we make an estimate of the coupling strength of QGP hypothesized to be present in compact star interiors. At densities ranging from 3ρ 0–10ρ 0 (normal nuclear density ρ 0=0.16 fm−3), quark matter is found to be strongly to intermediately coupled.
Sineeba Ramadas, Vishnu M. Bannur
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QCD Equations of State in Hadron–Quark Continuity
Universe, 2018 The properties of dense matter in quantum chromodynamics (QCD) are delineated through equations of state constrained by the neutron star observations. The two solar mass constraint, the radius constraint of ≃11–13 km, and the causality constraint on the ...
Toru Kojo
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Fluctuations and correlations from microscopic transport theory [PDF]
, 2009 The multiplicity fluctuations in A+A collisions at SPS and RHIC energies are studied within the HSD transport approach. We find a dominant role of the fluctuations in the nucleon participant number for the final fluctuations. In order to extract physical
Bratkovskaya, Elena L. +3 more
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Materia de quarks a temperatura finita [PDF]
, 2013 Dissertação (mestrado) - Universidade Federal de Santa Catarina, Centro de Ciências Físicas e Matemáticas, Programa de Pós-Graduação em Física, Florianópolis, 2013A constitução dos objetos estelares continua sendo fonte de especulação.
Agudelo, David Felipe Tamayo
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Quark Matter and Quark Stars [PDF]
Proceedings of the Workshop on Quarks and Compact Stars 2017 (QCS2017), 2018 Guangxiong Peng +2 more
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Stars and quark stars in bumblebee gravity
Annals of PhysicsIn this work, the interior spacetime of stars is built in a Lorentz symmetry breaking model called bumblebee gravity. Firstly, we calculated the modified Tolman-Oppenheimer-Volkoff equation in this context of modified gravity. Then we show that the bumblebee field, responsible for the symmetry breaking, increases the star mass-radius relation when it ...
Juliano C.S. Neves, Fernando G. Gardim
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On the conversion of neutron stars into quark stars
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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