Electromagnetic signal of the QCD phase transition in neutron star mergers

Mergers of binary neutron stars create conditions of supranuclear density n [> ~] n sub(nuc) [Asymptotically = to] 0.17 fm super(-3) and moderate temperature 50 [

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Bibliographic Details
Published in:Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2013-10, Vol.88 (8), Article 083006
Main Authors: Chen, Pisin, Labun, Lance
Format: Article
Language:English
Subjects:
Acquisitions
Asymptotic properties
Density
Neutron stars
Photons
Quantum chromodynamics
Quarks
Thermal conductivity
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Description
Summary:Mergers of binary neutron stars create conditions of supranuclear density n [> ~] n sub(nuc) [Asymptotically = to] 0.17 fm super(-3) and moderate temperature 50 [
ISSN:1550-7998
1550-2368
DOI:10.1103/PhysRevD.88.083006