PROPERTIES OF MAGNETIZED QUARK-HYBRID STARS-Reference-Cited by-同舟云学术

PROPERTIES OF MAGNETIZED QUARK-HYBRID STARS

Published:2011-12 Issue:supp02 Volume:20 Page:25-28
ISSN:0218-3013
Container-title:International Journal of Modern Physics E
language:en
Short-container-title:Int. J. Mod. Phys. E

Author:

ORSARIA MILVA¹²³,RANEA-SANDOVAL IGNACIO F.¹²,VUCETICH H.¹,WEBER FRIDOLIN³

Affiliation:

1. Gravitation, Astrophysics and Cosmology Group, Facultad de Ciencias Astronómicas y Geofsicas, Paseo del Bosque S/N (1900), Universidad Nacional de La Plata UNLP, La Plata, Argentina

2. CONICET, Rivadavia 1917, 1033 Buenos Aires, Argentina

3. Department of Physics, San Diego State University, 5500 Campanile Drive, San Diego, CA 92182, USA

Abstract

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).

Publisher

World Scientific Pub Co Pte Lt

Subject

General Physics and Astronomy,Nuclear and High Energy Physics

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0218301311040542

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