The superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models

Details The superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models The superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976foph....6..717s&link_type=abstract

Foundations of Physics, Volume 6, Issue 6, pp.717-726

Physics

10

Scientific paper

Some cosmological consequences of the superfluid vacuum state developed previously by the authors are discussed, particularly with regard to the initial stages of the universe. The transition temperature of the hadronic superfluid (superfluid during the hadron era) is estimated to be 10 13 K, which is the same as the Hagedorn temperature, giving a physical basis of the thermodynamic bootstrap model.

Affiliated with

Also associated with

No associations

Rating

The superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models 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 superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1049408