Quark Matter in Strong Magnetic Field

Abstract

The effect of strong magnetic field on the stability and gross properties of bulk as well as quasi-bulk quark matter has been investigated using the conventional MIT bag model. Both the Landau diamagnetism and the paramagnetism of quark matter has been studied. How the quark hadron phase transition is affected by the presence of strong magnetic field has also been investigated. The equation of state of strange quark matter changes significantly in strong magnetic field. It is also shown that the thermal nucleation of quark bubbles in compact metastable state of neutron matter is completely forbidden in presence of strong magnetic field.

31 Pages TEX file, with 9-figures available under request

References in corpus (8)

• Shell model versus liquid drop model for strangelets
• Constraints on the Strength of a Primordial Magnetic Field from Big Bang Nucleosynthesis
• Nucleation of quark matter bubbles in neutron stars
• Limits on possible magnetic fields at nucleosynthesis time
• Interaction Rates at High Magnetic Field Strengths and High Degeneracy
• Effect of magnetic field on the strange star
• The Polarization of a QED Plasma in a Strong Magnetic Field
• A Note on QED with Magnetic Field and Chemical Potentia

Cited by in corpus (112)

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• Thermodynamic consistency, quark mass scaling, and properties of strange matter
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• The influence of strong magnetic fields on proto-quark stars
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• Warm and dense stellar matter under strong magnetic fields
• D mesons in strongly magnetized asymmetric nuclear matter
• Crystalline chiral condensates as a component of compact stars
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• Magnetized strange quark matter in a quasiparticle description
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• Magnetic susceptibility and magnetization properties of asymmetric nuclear matter under a strong magnetic field
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• Investigation of the field-induced ferromagnetic phase transition in spin polarized neutron matter: a lowest order constrained variational approach
• Strange stars with different quark mass scalings
• Magnetized strange quark matter in a mass-density-dependent model
• Thermoelectric properties of (an-)isotropic QGP in magnetic fields
• Chiral Properties of QCD Vacuum in Magnetars- A Nambu-Jona-Lasinio Model with Semi-Classical Approximation
• Can There be Quark Matter Core in a Strongly Magnetized Neutron Star?
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• Neutrino opacity in magnetised hot and dense nuclear matter
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• Possibility of conversion of neutron star to quark star in presence of high magnetic field
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