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Rotating neutron star models with a magnetic field.
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This article is published in Astronomy and Astrophysics.The article was published on 1995-09-01 and is currently open access. It has received 181 citations till now. The article focuses on the topics: Neutron star & Theory of relativity.read more
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Effect of strong magnetic field on competing order parameters in two-flavor dense quark matter
TL;DR: In this paper, the effect of strong magnetic field on competing chiral and diquark order parameters in a regime of moderately dense quark matter was analyzed in a two-flavor Nambu-Jona-Lasinio (NJL) model.
Numerical models of isolated rotating compact stars
TL;DR: In this paper, a general-relativistic framework for the description of rotating compact stars is proposed and global observable quantities can be computed unambiguously, including the magnetic field and its effects on both global equilibrium and equation of state.
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Plasma influence on the neutrino — electron processes in a strong magnetic field
Alexander Kuznetsov,N.V. Mikheev +1 more
TL;DR: In this paper, an influence of the magnetized electron-positron plasma on the absorption and loss of the energy and momentum in a process of neutrino propagation is investigated.
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Highly Magnetized Neutron Stars in a Many-body Forces Formalism
TL;DR: In this article, the effects of different magnetic field configurations in neutron stars described by a many-body forces formalism (MBF model) were studied, where magnetic fields are taken into account both in the equation of state and in the structure of the stars by the selfconsistent solution of the Einstein-Maxwell equations.
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Radial oscillations of neutron stars in strong magnetic fields
Vinay Gupta,Vinay Gupta,Vinita Tuli,Vinita Tuli,Surya Prakash Singh,Surya Prakash Singh,J. D. Anand,J. D. Anand,Ashok Goyal,Ashok Goyal +9 more
TL;DR: In this article, the eigen frequencies of radial pulsations of neutron stars are calculated in a strong magnetic field and it is found that magnetized neutron stars support higher maximum mass whereas the effect of magnetic field on radial stability for observed neutron star masses is minimal.