Rate of the weak reaction s+u-->u+d in quark matter

Details Rate of the weak reaction s+u-->u+d in quark matter Rate of the weak reaction s+u-->u+d in quark matter

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvd..47..325m&link_type=abstract

Physical Review D (Particles and Fields), Volume 47, Issue 1, 1 January 1993, pp.325-330

Statistics

Applications

28

Quark-Gluon Plasma, Applications Of Electroweak Models To Specific Processes, Elementary Particle Processes, Neutron Stars

Scientific paper

The weak reaction s+u-->u+d and its inverse play important roles in the attempts to detect strangelets from relativistic heavy-ion collisions, in the burning of neutron stars into strange stars, in the formation and evaporation of quark nuggets in the early Universe, and, through the bulk viscosity, in determining the stability properties and maximum rotation velocity of neutron stars and/or strange stars. Exact expressions for these rates are given in the case of zero temperature and strange quark mass, and numerical calculations and fits to analytic approximations are given for the general case. Pauli blocking and finite-temperature effects are crucial. There is no ``typical'' time scale for the reactions.

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