Physics
Scientific paper
Mar 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..33...49d&link_type=abstract
Astrophysics and Space Science, vol. 33, Mar. 1975, p. 49-73.
Physics
12
Cosmology, Elementary Particle Interactions, Gravitation Theory, Hubble Diagram, Space-Time Functions, Universe, Astronomical Models, Background Radiation, Einstein Equations, Field Theory (Physics), Thermodynamic Equilibrium
Scientific paper
It is shown that the space-time singularity in the Einstein-Friedmann cosmology can be avoided if the negative potential energy of the strong interaction of elementary particles in the earliest stage of the universe is taken into account and if a homogeneous and isotropic world model, an upper temperature limit of about 1.9 by 10 to the 12th power deg K, and thermodynamic equilibrium between radiation and matter are assumed. Under these assumptions, the Friedmann equation is integrated numerically with the integration constant fitted by the present values of the mass density, the Hubble constant, and the background radiation temperature, and a singularity-free solution is obtained. The early evolution of the universe is described qualitatively.-
Dehnen Heinz
Hoenl H.
No associations
LandOfFree
The influence of strong interactions on the early stages of the universe 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 The influence of strong interactions on the early stages of the universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The influence of strong interactions on the early stages of the universe will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1518749