84 research outputs found
Rotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations
The electrostatic potential that keeps approximate charge neutrality in
neutron star matter is self-consistently introduced into the formalism for
rotochemical heating presented in a previous paper by Fernandez and
Reisenegger. Although the new formalism is more rigorous, we show that its
observable consequences are indistinguishable from those of the previous one,
leaving the conclusions of the previous paper unchanged.Comment: 14 pages, including 4 eps figures. Accepted for publication in The
Astrophysical Journa
Damping of sound waves in superfluid nucleon-hyperon matter of neutron stars
We consider sound waves in superfluid nucleon-hyperon matter of massive
neutron-star cores. We calculate and analyze the speeds of sound modes and
their damping times due to the shear viscosity and non-equilibrium weak
processes of particle transformations. For that, we employ the dissipative
relativistic hydrodynamics of a superfluid nucleon-hyperon mixture, formulated
recently [M.E. Gusakov and E.M. Kantor, Phys. Rev. D78, 083006 (2008)]. We
demonstrate that the damping times of sound modes calculated using this
hydrodynamics and the ordinary (nonsuperfluid) one, can differ from each other
by several orders of magnitude.Comment: 15 pages, 5 figures, Phys. Rev. D accepte
On matrix realizations of the Lie superalgebra D(2, 1 ; \alpha)
We obtain a realization of the Lie superalgebra in
differential operators on the supercircle and in matrices
over a Weyl algebra. A contraction of is isomorphic to the
universal central extension \hat{\p\s\l}(2|2) of \p\s\l(2|2). We realize it
in matrices over the associative algebra of pseudodifferential
operators on . Correspondingly, there exists a three-parameter family of
irreducible representations of \hat{\p\s\l}(2|2) in a --dimensional
complex superspace.Comment: 15 pages, to be published in Journal of Geometry and Physics 60
(2010), 1656-166
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