Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2008-02-21
Phys.Rev.Lett.101:091101,2008; Phys.Rev.Lett.101:119901,2008
Physics
High Energy Physics
High Energy Physics - Phenomenology
4 pages, 1 figure. Accepted for publication in PRL
Scientific paper
10.1103/PhysRevLett.101.091101 1
It is argued that a well measured double neutron star binary in which the two neutron stars are more than 4% different from each other in mass or a massive neutron star with mass M > 2 M_sun would put in serious doubt or simply falsify the following chain of predictions: (1) nearly vanishing vector meson mass at chiral restoration, (2) kaon condensation at a density n ~ 3 n_0, (3) the Brown-Bethe maximum neutron star mass M_max ~ 1.5 M_sun and (4) Smolin's `Cosmological Natural Selection' hypothesis.
Brown Gerald E.
Lee Chang Hoon
Rho Mannque
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