116 research outputs found
Alternative Derivation of the Correspondence Between Rindler and Minkowski Particles
We develop an alternative derivation of Unruh and Wald's seminal result that
the absorption of a Rindler particle by a detector as described by uniformly
accelerated observers corresponds to the emission of a Minkowski particle as
described by inertial observers. Actually, we present it in an inverted
version, namely, that the emission of a Minkowski particle corresponds in
general to either the emission or the absorption of a Rindler particle.Comment: 7 pages, no-figures, REVTE
Elementary particles under the lens of the black holes
After a brief review of the historical development and CLASSICAL properties
of the BLACK HOLES, we discuss how our present knowledge of some of their
QUANTUM properties shed light on the very concept of ELEMENTARY PARTICLE. As an
illustration, we discuss in this context the decay of accelerated protons,
which may be also relevant to astrophysics.Comment: 6 pages, Proceedings of the XXIII Brazilian National Meeting on
Particles Physics and Fields. To appear in special issue of the Brazilian
Journal of Physic
Search for semiclassical-gravity effects in relativistic stars
We discuss the possible influence of gravity in the neutronization process,
, which is particularly important as a cooling mechanism
of neutron stars. Our approach is semiclassical in the sense that leptonic
fields are quantized on a classical background spacetime, while neutrons and
protons are treated as excited and unexcited nucleon states, respectively. We
expect gravity to have some influence wherever the energy content carried by
the in-state is barely above the neutron mass. In this case the emitted
neutrinos would be soft enough to have a wavelength of the same order as the
space curvature radius.Comment: 10 pages (REVTEX
Decay of protons and neutrons induced by acceleration
We investigate the decay of accelerated protons and neutrons. Calculations
are carried out in the inertial and coaccelerated frames. Particle
interpretation of these processes are quite different in each frame but the
decay rates are verified to agree in both cases. For sake of simplicity our
calculations are performed in a two-dimensional spacetime since our conclusions
are not conceptually affected by this.Comment: 18 pages (REVTEX), 3 figure
The Unruh effect and its applications
It has been thirty years since the discovery of the Unruh effect. It has
played a crucial role in our understanding that the particle content of a field
theory is observer dependent. This effect is important in its own right and as
a way to understand the phenomenon of particle emission from black holes and
cosmological horizons. Here, we review the Unruh effect with particular
emphasis to its applications. We also comment on a number of recent
developments and discuss some controversies. Effort is also made to clarify
what seems to be common misconceptions.Comment: 53 pages, 11 figures, submitted to Reviews of Modern Physic
Interaction of Hawking radiation and a static electric charge
We investigate whether the equality found for the response of static scalar
sources interacting (i) with {\em Hawking radiation in Schwarzschild spacetime}
and (ii) with the Fulling-Davies-Unruh thermal bath in the Rindler wedge is
maintained in the case of electric charges. We find a finite result in the
Schwarzschild case, which is computed exactly, in contrast with the divergent
result associated with the infrared catastrophe in the Rindler case, i.e. in
the case of uniformly accelerated charges in Minkowski spacetime. Thus, the
equality found for scalar sources does not hold for electric charges.Comment: 8 pages (REVTEX
Low-frequency absorption cross section of the electromagnetic waves for the extreme Reissner-Nordstrom black holes in higher dimensions
We investigate the low-frequency absorption cross section of the
electromagnetic waves for the extreme Reissner-Nordstrom black holes in higher
dimensions. We first construct the exact solutions to the relevant wave
equations in the zero-frequency limit. In most cases it is possible to use
these solutions to find the transmission coefficients of partial waves in the
low-frequency limit. We use these transmission coefficients to calculate the
low-frequency absorption cross section in five and six spacetime dimensions. We
find that this cross section is dominated by the modes with l=2 in the
spherical-harmonic expansion rather than those with l=1, as might have been
expected, because of the mixing between the electromagnetic and gravitational
waves. We also find an upper limit for the low-frequency absorption cross
section in dimensions higher than six.Comment: 7 pages, 1 figure, Phys. Rev. D (to appear
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