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Sound Velocity Bound and Neutron Stars

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It has been conjectured that the velocity of sound in any medium is smaller than the velocity of light in vacuum divided by 3~(1/2). Simple arguments support this bound in nonrelativistic and/or weakly coupled theories. The bound has been demonstrated in several classes of strongly coupled theories with gravity duals and is saturated only in conformal theories. We point out that the existence of neutron stars with masses around two solar masses combined with the knowledge of the equation of state of hadronic matter at "low" densities is in strong tension with this bound.

neutron stars

Paulo Bedaque、Andrew W. Steiner

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Department of Physics, University of Maryland, College Park, Maryland 20742, USA

Institute for Nuclear Theory, University of Washington, Seattle, Washington 98195, USA Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA and Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA

2015

Physical review letters

Physical review letters

ISSN:0031-9007
年,卷(期):2015.114(3)
  • 110
  • 33