Strange Quark Matter in Stars: A General Overview
arXiv:astro-ph/0412215 · doi:10.1088/0954-3899/31/6/004
Abstract
The physics of strange quark matter in the core of compact stars and recent compact star data is reviewed. Emphasis is put on the possible existence of a third family of strange quark stars.
8 pages, 1 figure, plenary talk given at the 8th International Conference on Strangeness in Quark Matter (SQM2004), Cape Town, South Africa, 15-20 September 2004
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- The Physics of Neutron Stars
- Effects of color superconductivity on the structure and formation of compact stars
- Discovery of the Neutron Star Spin Frequency in EXO 0748-676
- Phase diagram of dense neutral three-flavor quark matter
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Cited by in corpus (23)
- Equation of State of a Dense and Magnetized Fermion System
- Cold uniform matter and neutron stars in the quark-mesons-coupling model
- Too massive neutron stars: The role of dark matter?
- Droplets in the cold and dense linear sigma model with quarks
- Binding of Hypernuclei in the Latest Quark-Meson Coupling Model
- The Surface Tension of Quark Matter in a Geometrical Approach
- Hadronic and hybrid stars subject to density dependent magnetic fields
- Compact Stars for Undergraduates
- A study of Lambda hypernuclei within the Skyrme-Hartree-Fock Model
- The Surface Tension of Magnetized Quark Matter
- Pulsar kicks by anisotropic neutrino emission from quark matter in strong magnetic fields
- Analysis of White Dwarfs with Strange-Matter Cores
- Lattice QCD Constraints on Hybrid and Quark Stars
- The importance of the mixed phase in hybrid stars built with the Nambu-Jona-Lasinio model
- Neutron Stars and Dark Matter
- Pulsar kicks by anisotropic neutrino emission from quark matter
- Mass radius relation of compact stars in the braneworld
- Phase transition from quark-meson coupling hyperonic matter to deconfined quark matter
- Gravastar under the framework of braneworld gravity II: effect of the Kuchowicz metric function
- Neutron star mass in dark matter clumps
- Strange quark matter as dark matter: 40 years later, a reappraisal
- A new approach to bulk viscosity in strange quark matter at high densities
- Surface structure of Quark stars with magnetic fields