Relativistic Processes and the Internal Structure of Neutron Stars

Journal Article · Fri Oct 14 00:00:00 EDT 2011 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.3647541· OSTI ID:21611882

Alvarez-Castillo, D E; Kubis, S ^[1]

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1. Institute of Nuclear Physics, Radzikowskiego 152, 31-342 Krakow (Poland)

Models for the internal composition of Dense Compact Stars are reviewed as well as macroscopic properties derived by observations of relativistic processes. Modeling of pure neutron matter Neutron Stars is presented and crust properties are studied by means of a two fluid model.

• OSTI ID: 21611882
• Journal Information: AIP Conference Proceedings, Vol. 1396, Issue 1; Conference: 8. workshop of the gravitation and mathematical physics division of the Mexican Physical Society, Tuxtla Gutierrez, Chiapas (Mexico), 22-26 Nov 2010; Other Information: DOI: 10.1063/1.3647541; (c) 2011 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ASTROPHYSICS
COMPUTERIZED SIMULATION
EQUATIONS OF STATE
NEUTRON SOURCES
NEUTRON STARS
NUCLEAR MATTER
PHASE TRANSFORMATIONS
RELATIVISTIC RANGE
STAR EVOLUTION
ENERGY RANGE
EQUATIONS
EVOLUTION
MATTER
PARTICLE SOURCES
PHYSICS
RADIATION SOURCES
SIMULATION
STARS