104,482 research outputs found
AdS/CFT For Non-Boundary Manifolds
In its Euclidean formulation, the AdS/CFT correspondence begins as a study of
Yang-Mills conformal field theories on the sphere, S^4. It has been
successfully extended, however, to S^1 X S^3 and to the torus T^4. It is
natural to hope that it can be made to work for any manifold on which it is
possible to define a stable Yang-Mills conformal field theory. We consider a
possible classification of such manifolds, and show how to deal with the most
obvious objection : the existence of manifolds which cannot be represented as
boundaries. We confirm Witten's suggestion that this can be done with the help
of a brane in the bulk.Comment: 21 pages, 1 eps figure (1000x500), remarks on p-brane stress-tensor
clarifie
Modeling-Free Bounds on Nonrenormalizable Isotropic Lorentz and CPT Violation in QED
The strongest bounds on some forms of Lorentz and CPT violation come from
astrophysical data, and placing such bounds may require understanding and
modeling distant sources of radiation. However, it is also desirable to have
bounds that do not rely on these kinds of detailed models. Bounds that do not
rely on any modeling of astrophysical objects may be derived both from
laboratory experiments and certain kinds of astrophysical observations. The
strongest such bounds on isotropic modifications of electron, positron, and
photon dispersion relations of the form E^2 = p^2 + m^ 2 + epsilon p^3 come
from data on cosmological birefringence, the absence of photon decay, and
radiation from lepton beams. The bounds range in strength from the 4 x 10^(-13)
to 6 x 10^(-33) (GeV)^(-1) levels.Comment: New title, 12 pages, version to appear in Phys. Rev.
There is No Ambiguity in the Radiatively Induced Gravitational Chern-Simons Term
Quantum corrections to Lorentz- and CPT-violating QED in flat spacetime
produce unusual radiative corrections, which can be finite but of undetermined
magnitude. The corresponding radiative corrections in a gravitational theory
are even stranger, since the term in the fermion action involving a preferred
axial vector would give rise to a gravitational Chern-Simons term
that is proportional , yet which actually does not break Lorentz
invariance. Initially, the coefficient of this gravitational Chern-Simons term
appears to have the same ambiguity as the coefficient for the analogous term in
QED. However, this puzzle is resolved by the fact that the gravitational theory
has more stringent gauge invariance requirements. Lorentz symmetry in a metric
theory of gravity can only be broken spontaneously, and when the vector
arises from spontaneous symmetry breaking, these specific radiative
corrections are no longer ambiguous but instead must vanish identically.Comment: 16 page
How Does the Quark-Gluon Plasma Know the Collision Energy?
Heavy ion collisions at the LHC facility generate a Quark-Gluon Plasma (QGP)
which, for central collisions, has a higher energy density and temperature than
the plasma generated in central collisions at the RHIC. But sufficiently
peripheral LHC collisions give rise to plasmas which have the \emph{same}
energy density and temperature as the "central" RHIC plasmas. One might assume
that the two versions of the QGP would have very similar properties (for
example, with regard to jet quenching), but recent investigations have
suggested that \emph{they do not}: the plasma "knows" that the overall
collision energy is different in the two cases. We argue, using a gauge-gravity
analysis, that the strong magnetic fields arising in one case (peripheral
collisions), but not the other, may be relevant here. If the residual magnetic
field in peripheral LHC plasmas is of the order of at least , then the model predicts modifications of the relevant
quenching parameter which approach those recently reported.Comment: 16 pages, one figure; version to appear in Nuclear Physics
ADVANCING THE SEPARATION SCIENCES THROUGH THE DELIVERY OF NEW MATERIALS, TECHNOLOGY AND METHODOLOGY.
A thesis and collection of works submitted to Plymouth University in partial fulfilment for the degree of
DOCTOR OF SCIENC
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