A statistical mechanical approach to the mass density fluctuations between 1 KE V and 1 eV in the early universe

Details A statistical mechanical approach to the mass density fluctuations between 1 KE V and 1 eV in the early universe A statistical mechanical approach to the mass density fluctuations between 1 KE V and 1 eV in the early universe

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nciml..44..270s&link_type=abstract

Nuovo Cimento, Lettere, Serie 2, vol. 44, Nov. 1, 1985, p. 270-274.

Physics

Condensed Matter

Statistical Mechanics

Big Bang Cosmology, Density Distribution, Mass Distribution, Statistical Mechanics, Adiabatic Conditions, Baryons, Expansion

Scientific paper

A rigorous, nonperturbative, statistical mechanical approach is being proposed to calculate the mass-density fluctuations in the cosmological context. The analysis done here applies to an era shortly before radiation-matter decoupling. The expression for delta-rho/rho indicates that such fluctuations increase in a complicated fashion as the universe expands.

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