82 research outputs found
Boson-boson effective nonrelativistic potential for higher-derivative electromagnetic theories in D dimensions
The problem of computing the effective nonrelativistic potential for
the interaction of charged scalar bosons within the context of D-dimensional
electromagnetism with a cutoff, is reduced to quadratures. It is shown that
cannot bind a pair of identical charged scalar bosons; nevertheless,
numerical calculations indicate that boson-boson bound states do exist in the
framework of three-dimensional higher-derivative electromagnetism augmented by
a topological Chern-Simons term.Comment: 6 page
Photon Mass and Very Long Baseline Interferometry
A relation between the photon mass, its frequency, , and the deflection
parameter, , determined by experimentalists (which characterizes the
contribution of space curvature to gravitational deflection) is found. This
amazing result allows us to conclude that the knowledge of the parameters
and is all we need to set up gravitational bounds on the photon mass.
By considering as inputs the most recent measurements of the solar
gravitational deflection of radio waves obtained via the Very Long Baseline
Interferometry, upper bounds on the photon mass are estimated.Comment: Accepted for publication in International Journal of Modern Physics
Is it Physically Sound to Add a Topologically Massive Term to Three-Dimensional Massive Electromagnetic or Gravitational Models ?
The addition of a topologically massive term to an admittedly non-unitary
three-dimensional massive model, be it an electromagnetic system or a
gravitational one, does not cure its non-unitarity. What about the enlargement
of avowedly unitary massive models by way of a topologically massive term? The
electromagnetic models remain unitary after the topological augmentation but,
surprisingly enough, the gravitational ones have their unitarity spoiled. Here
we analyze these issues and present the explanation why unitary massive
gravitational models, unlike unitary massive electromagnetic ones, cannot
coexist from the viewpoint of unitarity with topologically massive terms. We
also discuss the novel features of the three-term effective field models that
are gauge-invariant
Unavoidable Conflict Between Massive Gravity Models and Massive Topological Terms
Massive gravity models in 2+1 dimensions, such as those obtained by adding to
Einstein's gravity the usual Fierz-Pauli, or the more complicated Ricci scalar
squared (), terms, are tree level unitary. Interesting enough these
seemingly harmless systems have their unitarity spoiled when they are augmented
by a Chern-Simons term. Furthermore, if the massive topological term is added
to gravity, or to gravity
(higher-derivative gravity), which are nonunitary at the tree level, the
resulting models remain nonunitary. Therefore, unlike the common belief, as
well as the claims in the literature, the coexistence between three-dimensional
massive gravity models and massive topological terms is conflicting.Comment: 13 pages, no figure
Born-Infeld Electrodynamics and Euler-Heisenberg-like Model: outstanding examples of the lack of commutativity among quantized truncated actions and truncated quantized actions
We calculate the lowest-order corrections to the static potential for both
the generalized Born-Infeld Electrodynamics and an Euler-Heisenberg-like model,
in the presence of a constant external magnetic field. Our analysis is carried
out within the framework of the gauge-invariant but path-dependent variables
formalism. The calculation reveals a long-range correction (
{\raise0.7ex\hbox{1} \mathord{\left/ {\vphantom {1
{r^5}}}\right.\kern-\nulldelimiterspace} \lower0.7ex\hbox{{r^5}}}-type) to
the Coulomb potential for the generalized Born-Infeld Electrodynamics.
Interestingly enough, in the Euler-Heisenberg-like model, the static potential
remains Coulombian. Therefore, contrary to popular belief, the quantized
truncated action and the truncated quantized action do not commute at all.Comment: 7 pages. Title changed, revised version. To appear in Int. J. Mod.
Phys.
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