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Free-quark phases in dense stars

Journal Article:

Abstract

The possibility is examined that superdense matter can undergo a transition to a phase of free quarks within models which assume that the quark confinement potential is screened at high densities. The results imply that a phase of pure quarks of this type is unlikely to be found in stable stellar systems although they do not preclude the possible existence of a transition region which contains quarks and neutrons in equilibrium at the center of neutron stars.
Authors:
Keister, B D; Kisslinger, L S [1] 
  1. Carnegie-Mellon Univ., Pittsburgh, Pa. (USA). Dept. of Physics
Publication Date:
Aug 30, 1976
Product Type:
Journal Article
Reference Number:
AIX-07-276807; EDB-77-027444
Resource Relation:
Journal Name: Phys. Lett., B; (Netherlands); Journal Volume: 64:1
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; NEUTRON STARS; QUARKS; BAG MODEL; EQUATIONS OF STATE; FERMI GAS; NUCLEAR MATTER; QUARK MODEL; STABILITY; COMPOSITE MODELS; ELEMENTARY PARTICLES; EQUATIONS; EXTENDED PARTICLE MODEL; MATHEMATICAL MODELS; MATTER; PARTICLE MODELS; POSTULATED PARTICLES; STARS; 640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources
OSTI ID:
7327988
Country of Origin:
Netherlands
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: PYLBB
Submitting Site:
INIS
Size:
Pages: 117-120
Announcement Date:

Journal Article:

Citation Formats

Keister, B D, and Kisslinger, L S. Free-quark phases in dense stars. Netherlands: N. p., 1976. Web.
Keister, B D, & Kisslinger, L S. Free-quark phases in dense stars. Netherlands.
Keister, B D, and Kisslinger, L S. 1976. "Free-quark phases in dense stars." Netherlands.
@misc{etde_7327988,
title = {Free-quark phases in dense stars}
author = {Keister, B D, and Kisslinger, L S}
abstractNote = {The possibility is examined that superdense matter can undergo a transition to a phase of free quarks within models which assume that the quark confinement potential is screened at high densities. The results imply that a phase of pure quarks of this type is unlikely to be found in stable stellar systems although they do not preclude the possible existence of a transition region which contains quarks and neutrons in equilibrium at the center of neutron stars.}
journal = {Phys. Lett., B; (Netherlands)}
volume = {64:1}
journal type = {AC}
place = {Netherlands}
year = {1976}
month = {Aug}
}