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Crossover transition to quark matter in heavy hybrid stars

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arxiv 1311.5112 v2 pith:ZAGFSHR4 submitted 2013-11-20 nucl-th astro-ph.HEhep-ph

D. E. Alvarez-Castillo , S. Benic , D. Blaschke , R. Lastowiecki This is my paper · ORCID
classification nucl-thastro-ph.HEhep-ph
keywords crossovermatterhybridquarktemperaturestransitionastrophysicalbehavior
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We study the possibility that the transition from hadron matter to quark matter at vanishing temperatures proceeds via crossover, similar to the crossover behavior found with lattice QCD studies at high temperatures. The purpose is to examine astrophysical consequences of this postulate by constructing hybrid star sequences fulfilling current experimental data.

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Cited by 1 Pith paper

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  1. Continuity from neutron matter to two-flavor quark matter with $^1 S_0$ and $^3 P_2$ superfluidity

    hep-ph 2019-08 conditional novelty 5.0 of 10

    The paper proposes that neutron 1S0 and 3P2 superfluidity map continuously to scalar and 3P2 d-quark pairing in a 2SC+⟨dd⟩ quark matter phase, extending quark-hadron continuity to two flavors.

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