Published December 2011 | Version v1
Journal article

Properties of magnetized quark-hybrid stars

  • 1. Department of Physics, San Diego State University, 5500 Campanile Drive, San Diego, CA 92182 (United States)
  • 2. CONICET, Rivadavia 1917, 1033 Buenos Aires (Argentina)
  • 3. Gravitation, Astrophysics and Cosmology Group, Facultad de Ciencias Astronomicas y Geofsicas, Paseo del Bosque S/N (1900), Universidad Nacional de La Plata UNLP, La Plata (Argentina)

Description

The structure of a magnetized quark-hybrid stars (QHS) is modeled using a standard relativistic mean-field equation of state (EoS) for the description of hadronic matter. For quark matter we consider a bag model EoS which is modified perturbatively to account for the presence of a uniform magnetic field. The mass-radius (M-R) relationship, gravitational redshift and rotational Kepler periods of such stars are compared with those of standard neutron stars (NS). (author)

Availability note (English)

Available from DOI: http://dx.doi.org/10.1142/S0218301311040542

Additional details

Publishing Information

Journal Title
International Journal of Modern Physics E
Journal Volume
20
Journal Issue
supp.2
Journal Page Range
p. 25-28
ISSN
0218-3013

Conference

Title
2. international symposium on strong electromagnetic fields and neutron stars
Acronym
SMFNS 2011
Dates
5-7 May 2011
Place
Varadero (Cuba)

INIS

Country of Publication
Singapore
Country of Input or Organization
Singapore
INIS RN
46046072
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
BAG MODEL; EQUATIONS OF STATE; MAGNETIC FIELDS; MEAN-FIELD THEORY; NEUTRON STARS; NUCLEAR RADII; QUARKS; RED SHIFT
Descriptors DEC
COMPOSITE MODELS; EQUATIONS; EXTENDED PARTICLE MODEL; FERMIONS; MATHEMATICAL MODELS; NUCLEAR PROPERTIES; PARTICLE MODELS; QUARK MODEL; STARS