Neutrino flow dominance during the cosmological quark-hadron transition

Details Neutrino flow dominance during the cosmological quark-hadron transition Neutrino flow dominance during the cosmological quark-hadron transition

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...176l...9b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 176, no. 1, April 1987, p. L9-L12.

Astronomy and Astrophysics

Astrophysics

2

Big Bang Cosmology, Hadrons, Neutrinos, Particle Motion, Quarks, Transition Temperature, Convection, Differential Equations, Phase Transformations, Temperature Profiles

Scientific paper

The detailed evolution of the thermal conditions, during the cosmological Q-H transition, are determined under the hypothesis that neutrino transport be the main mechanism driving the transition. The quark phase, the hadron phase and the neutrinos are found to have temperatures Ti ≅ Tc (1 - 10-4), slightly varying during the transition period. The authors briefly discuss the physical consequence of such dominance in relation with the part of the transition period during which it might occur.

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