Results 51 to 60 of about 41,225 (263)
QUARK-CLUSTER STARS: THE STRUCTURE [PDF]
International Journal of Modern Physics: Conference Series, 2013 The nature of pulsar-like compact stars is still in controversy although the first pulsar was found more than 40 years ago. Generally speaking, conventional neutron stars and non-mainstream quark stars are two types of models to describe the inner structure of pulsars, with the former composed mainly of hadrons and the latter of a peculiar kind of ...
Renxin Xu, Xiaoyu Lai
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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
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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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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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Quark phases in neutron stars and a "third family" of compact stars as a signature for phase transitions [PDF]
, 2000 The appearance of quark phases in the dense interior of neutron stars provides one possibility to soften the equation of state (EOS) of neutron star matter at high densities.
Akmal +76 more
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Strange Quark Stars — A Review [PDF]
Symposium - International Astronomical Union, 2003 A pedagogical overview of strange quark matter and strange stars is presented. After a historical notation of the research and an introduction to quark matter, a major part is devoted to the physics and astrophysics of strange stars, with attention being paid to the possible ways by which neutron stars and strange stars can be distinguished in ...
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European Physical Journal C: Particles and Fields, 2020 The phase diagram of dense quark matter with chiral imbalance is considered with the conditions of electric neutrality and $$\beta $$ β -equilibrium. It has been shown recently that chiral imbalance can generate charged pion condensation (PC) in dense ...
T. G. Khunjua +2 more
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Binary Neutron-Star Mergers with a Crossover Transition to Quark Matter
Universe, 2023 This paper summarizes recent work on the possible gravitational-wave signal from binary neutron-star mergers in which there is a crossover transition to quark matter.
Grant J. Mathews +3 more
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Thermal Evolution and Light Curves of Young Bare Strange Stars [PDF]
, 2002 The cooling of a young bare strange star is studied numerically by solving the equations of energy conservation and heat transport for both normal and superconducting strange quark matter inside the star.
Ch. Schaab +14 more
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Quark-Novae in massive binaries : a model for double-humped, hydrogen-poor, superluminous Supernovae
, 2015 LSQ14bdq and SN 2006oz are super-luminous, hydrogen-poor, SNe with double-humped light curves. We show that a Quark-Nova (QN; explosive transition of the neutron star to a quark star) occurring in a massive binary, experiencing two Common Envelope (CE ...
Koning, Nico +2 more
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