Maximum rotation frequency of strange stars

Journal Article · Sun Jul 15 00:00:00 EDT 1990 · Physical Review, D (Particles Fields); (USA)

DOI:https://doi.org/10.1103/PhysRevD.42.710· OSTI ID:6710806

Zdunik, J L; Haensel, P ^[1]

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1. Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, PL-00-716 Warsaw (Poland)

Using the MIT bag model of strange-quark matter, we calculate the maximum angular frequency of the uniform rotation of strange stars. After studying a broad range of the MIT bag-model parameters, we obtain an upper bound of 12.3 kHz.

• OSTI ID: 6710806
• Journal Information: Physical Review, D (Particles Fields); (USA), Vol. 42:2; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
QUARK MATTER
BAG MODEL
STARS
ROTATION
STRANGENESS
EQUATIONS OF STATE
NEUTRON STARS
QUANTUM CHROMODYNAMICS
COMPOSITE MODELS
EQUATIONS
EXTENDED PARTICLE MODEL
FIELD THEORIES
MATHEMATICAL MODELS
MATTER
MOTION
PARTICLE MODELS
PARTICLE PROPERTIES
QUANTUM FIELD THEORY
QUARK MODEL
640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources
645400 - High Energy Physics- Field Theory