Viscous phenomena in cosmology I. Lepton era

Details Viscous phenomena in cosmology I. Lepton era Viscous phenomena in cosmology I. Lepton era

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phya..134..458h&link_type=abstract

Physica A, Volume 134, Issue 2, p. 458-473.

Physics

10

Scientific paper

Shear and volume viscosity of the cosmic fluid in the lepton era are calculated with the help of relativistic kinetic theory. The cosmic fluid is taken to be a mixture of neutrinos (νe, νμ, ντ), electrons (e-) and their antiparticles. The differential cross-sections are determined on the basis of the Weinberg-Salam model in the current-current coupling approximation.

Affiliated with

Also associated with

No associations

Rating

Viscous phenomena in cosmology I. Lepton era does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Viscous phenomena in cosmology I. Lepton era, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Viscous phenomena in cosmology I. Lepton era will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1847797