You need JavaScript to view this

Thermodynamics of quark gas

Abstract

The application of quantum statistical mechanics to a system of particles consisting of quarks is considered. Realistic theoretical investigations have been underway to understand highly dense objects such as white dwarfs and neutron stars. The various possibilities in the case of very high densities such as 10/sup 15/ or 10/sup 16/ g/cm/sup 3/ are enumerated. The thermodynamics of a phase transition from neutron matter phase to quark matter phase is analysed. Preliminary results based on quantum chromodynamics and other phenomenological models are reported.
Authors:
Publication Date:
Jul 01, 1980
Product Type:
Conference
Report Number:
CONF-781260-
Reference Number:
AIX-12-598143; ERA-06-038535; EDB-81-125741
Resource Relation:
Conference: 4. high energy physics symposium, Jaipur, Rajasthan, India, 5 Dec 1978; Related Information: In: Proceedings of the fourth high energy physics symposium (held at) Jaipur, December 5-9, 1978.
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; QUANTUM CHROMODYNAMICS; QUARKS; THERMODYNAMICS; DENSITY; NEUTRON STARS; PHASE TRANSFORMATIONS; STATISTICAL MECHANICS; WHITE DWARF STARS; DWARF STARS; ELEMENTARY PARTICLES; FIELD THEORIES; MECHANICS; PHYSICAL PROPERTIES; POSTULATED PARTICLES; QUANTUM FIELD THEORY; STARS; 645400* - High Energy Physics- Field Theory
OSTI ID:
8467115
Research Organizations:
Delhi Univ. (India). Dept. of Physics and Astrophysics
Country of Origin:
India
Language:
English
Submitting Site:
INIS
Size:
Pages: 186-205
Announcement Date:
Apr 01, 1981

Citation Formats

Biswas, S. N. Thermodynamics of quark gas. India: N. p., 1980. Web.
Biswas, S. N. Thermodynamics of quark gas. India.
Biswas, S. N. 1980. "Thermodynamics of quark gas." India.
@misc{etde_8467115,
title = {Thermodynamics of quark gas}
author = {Biswas, S. N.}
abstractNote = {The application of quantum statistical mechanics to a system of particles consisting of quarks is considered. Realistic theoretical investigations have been underway to understand highly dense objects such as white dwarfs and neutron stars. The various possibilities in the case of very high densities such as 10/sup 15/ or 10/sup 16/ g/cm/sup 3/ are enumerated. The thermodynamics of a phase transition from neutron matter phase to quark matter phase is analysed. Preliminary results based on quantum chromodynamics and other phenomenological models are reported.}
place = {India}
year = {1980}
month = {Jul}
}