26 research outputs found
Comment to "Fine structure constant in the spacetime of a cosmic string"
In the paper Phys. Lett. B614 (2005), 140-142, F. Nasseri shows that the
values of the fine structure constant reduces due to the presence of a cosmic
string. In this comment I want to point out that this conclusion is not
completely correct in the sense that the result obtained is valid only in a
very special situation.Comment: Accepted for publication in Physics Letters
Reply to "Comment on 'Gravitating Magnetic Monopole in the Global Monopole Spacetime' "
In this Reply I present some arguments in favor of the stability of the
topological defect composed by global and magnetic monopoles.Comment: 1 page, no figures. Revised version improves the theoretical analysis
about electrostatic self-interaction in the global monopole spacetim
Repulsive Casimir-Polder forces from cosmic strings
We investigate the Casimir-Polder force acting on a polarizable microparticle
in the geometry of a straight cosmic string. In order to develop this analysis
we evaluate the electromagnetic field Green tensor on the imaginary frequency
axis. The expression for the Casimir-Polder force is derived in the general
case of anisotropic polarizability. In dependence of the eigenvalues for the
polarizability tensor and of the orientation of its principal axes, the
Casimir-Polder force can be either repulsive or attractive. Moreover, there are
situations where the force changes the sign with separation. We show that for
an isotropic polarizability tensor the force is always repulsive. At large
separations between the microparticle and the string, the force varies
inversely as the fifth power of the distance. In the non-retarded regime,
corresponding to separations smaller than the relevant transition wavelengths,
the force decays as the inverse fourth power of the distance. In the case of
anisotropic polarizability, the dependence of the Casimir-Polder potential on
the orientation of the polarizability tensor principal axes also leads to the
moment of force acting on the particle.Comment: 16 pages, 2 figure
Electromagnetic Casimir densities induced by a conducting cylindrical shell in the cosmic string spacetime
We investigate the renormalized vacuum expectation values of the field square
and the energy-momentum tensor for the electromagnetic field inside and outside
of a conducting cylindrical shell in the cosmic string spacetime. By using the
generalized Abel-Plana formula, the vacuum expectation values are presented in
the form of the sum of boundary-free and boundary-induced parts. The asymptotic
behavior of the vacuum expectation values of the field square, energy density
and stresses are investigated in various limiting cases.Comment: 14 pages, 2 figures, discussion and references added, accepted for
publication in Phys. Lett.
Self-energy and Self-force in the Space-time of a Thick Cosmic String
We calculate the self-energy and self-force for an electrically charged
particle at rest in the background of Gott-Hiscock cosmic string space-time. We
found the general expression for the self-energy which is expressed in terms of
the matrix of the scattering problem. The self-energy continuously falls
down outward from the string's center with maximum at the origin of the string.
The self-force is repulsive for an arbitrary position of the particle. It tends
to zero in the string's center and also far from the string and it has a
maximum value at the string's surface. The plots of the numerical calculations
of the self-energy and self-force are shown.Comment: 15 pages, 4 Postscript figures, ReVTe
Vacuum polarization by a global monopole with finite core
We investigate the effects of a -dimensional global monopole core on
the behavior of a quantum massive scalar field with general curvature coupling
parameter. In the general case of the spherically symmetric static core,
formulae are derived for the Wightman function, for the vacuum expectation
values of the field square and the energy-momentum tensor in the exterior
region. These expectation values are presented as the sum of point-like global
monopole part and the core induced one. The asymptotic behavior of the core
induced vacuum densities is investigated at large distances from the core, near
the core and for small values of the solid angle corresponding to strong
gravitational fields. In particular, in the latter case we show that the
behavior of the vacuum densities is drastically different for minimally and
non-minimally coupled fields. As an application of general results the
flower-pot model for the monopole's core is considered and the expectation
values inside the core are evaluated.Comment: 22 pages, 4 figures, misprint is corrected, discussion is added,
figures are change
De Sitter Cosmic Strings and Supersymmetry
We study massive spinor fields in the geometry of a straight cosmic string in
a de Sitter background. We find a hidden N=2 supersymmetry in the fermionic
solutions of the equations of motion. We connect the zero mode solutions to the
heat-kernel regularized Witten index of the supersymmetric algebra.Comment: Version similar to the one accepted by General Relativity and
Gravitatio
Relativistic quantum dynamics of a charged particle in cosmic string spacetime in the presence of magnetic field and scalar potential
In this paper we analyze the relativistic quantum motion of charged spin-0
and spin-1/2 particles in the presence of a uniform magnetic field and scalar
potentials in the cosmic string spacetime. In order to develop this analysis,
we assume that the magnetic field is parallel to the string and the scalar
potentials present a cylindrical symmetry with their center on the string. Two
distinct configurations for the scalar potential, , are considered:
the potential proportional to the inverse of the polar distance, i.e.,
, and the potential proportional to this distance, i.e.,
. The energy spectra are explicitly computed for different physical
situations and presented their dependences on the magnetic field strength and
scalar coupling constants.Comment: New version with 20 pages and no figure. Some minor revisions and six
references added. Accepted for publication in EJP