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astro-ph.HEOct 1, 2017
4
citations (OpenAlex)
authors
  • Niels-Uwe F. Bastian
  • David B. Blaschke
  • Mateusz Cierniak
  • Tobias Fischer
  • Mark A. R. Kaltenborn
  • Michał Marczenko
  • Stefan Typel
institutions
  • George Washington University
  • GSI Helmholtz Centre for Heavy Ion Research
  • Joint Institute for Nuclear Research
  • Los Alamos National Laboratory
  • National Research Nuclear University MEPhI
  • Technische Universität Darmstadt
  • University of Wrocław
arXiv abstractPDF
paper

Strange matter prospects within the string-flip model

arXiv:1710.09189 · doi:10.1051/epjconf/201817120002

Abstract

In this contribution we extend the recently developed two-flavor quark-matter string-flip model by including strange quarks. We discuss implications for compact stars.

4 pages, 4 figures, proceedings to SQM2017

References in corpus (5)

  • Shapiro delay measurement of a two solar mass neutron star
  • A Massive Pulsar in a Compact Relativistic Binary
  • A new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars
  • Modern compact star observations and the quark matter equation of state
  • Lattice QCD Constraints on the Nuclear Equation of State

Cited by in corpus (3)

  • Phases of dense matter in compact stars
  • Towards a Unified Quark-Hadron Matter Equation of State for Applications in Astrophysics and Heavy-Ion Collisions
  • A unified quark-nuclear matter equation of state from the cluster virial expansion within the generalized Beth-Uhlenbeck approach
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