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Title: Superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models

Abstract

Some cosmological consequences of the superfluid vacuum state developed previously 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/sup 13/ K, which is the same as the Hagedorn temperature, giving a physical basis of the thermodynamic bootstrap model.

Authors:
; ;
Publication Date:
Research Org.:
Indian Inst. of Science, Bangalore
OSTI Identifier:
7330050
Resource Type:
Journal Article
Journal Name:
Found. Phys.; (United States)
Additional Journal Information:
Journal Volume: 6:6
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; BOOTSTRAP MODEL; COSMOLOGY; COSMOLOGICAL MODELS; SUPERFLUIDITY; HADRONS; THERMODYNAMIC MODEL; TIME DEPENDENCE; UNIVERSE; COMPOSITE MODELS; ELEMENTARY PARTICLES; MATHEMATICAL MODELS; PARTICLE MODELS; STATISTICAL MODELS; 640106* - Astrophysics & Cosmology- Cosmology; 645201 - High Energy Physics- Particle Interactions & Properties-Theoretical- General & Scattering Theory

Citation Formats

Sinha, K P, Sivaram, C, and Sudarshan, E C.G. Superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models. United States: N. p., 1976. Web. doi:10.1007/BF00708950.
Sinha, K P, Sivaram, C, & Sudarshan, E C.G. Superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models. United States. https://doi.org/10.1007/BF00708950
Sinha, K P, Sivaram, C, and Sudarshan, E C.G. 1976. "Superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models". United States. https://doi.org/10.1007/BF00708950.
@article{osti_7330050,
title = {Superfluid vacuum state, time-varying cosmological constant, and nonsingular cosmological models},
author = {Sinha, K P and Sivaram, C and Sudarshan, E C.G.},
abstractNote = {Some cosmological consequences of the superfluid vacuum state developed previously 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/sup 13/ K, which is the same as the Hagedorn temperature, giving a physical basis of the thermodynamic bootstrap model.},
doi = {10.1007/BF00708950},
url = {https://www.osti.gov/biblio/7330050}, journal = {Found. Phys.; (United States)},
number = ,
volume = 6:6,
place = {United States},
year = {Wed Dec 01 00:00:00 EST 1976},
month = {Wed Dec 01 00:00:00 EST 1976}
}