Microscopic interpretation of neutron star structure

Technical Report · Mon Mar 01 00:00:00 EST 1976

DOI:https://doi.org/10.2172/7282365· OSTI ID:7282365

Arnett, W. D.; Bowers, R. L.

Because of the uncertainties in current understanding of the interaction at supernuclear densities, the structure of slowly rotating neutron stars was calculated for each of fifteen equations of state. (JFP)

• Research Organization: Univ. of Texas, Austin, TX (United States). Center for Particle Theory
• OSTI ID: 7282365
• Report Number(s): ORO-3992-257; TRN: 76-015228
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
NEUTRON STARS
STRUCTURAL MODELS
EQUATIONS OF STATE
INTERACTIONS
ROTATION
EQUATIONS
MOTION
STARS
640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources