410 research outputs found
Low energy effective action on a self-gravitating D-brane
Recently the study of braneworld on the self-gravitating D-brane has been
initiated and derived the gravitational equation on the brane by holographic
and geometrical projection methods. Surprisingly, in common with these two
methods, the matter on the brane cannot be the source of the gravity on the
brane at leading order. In this paper we will propose the low energy effective
action on the D-brane coupled with gravity which derives the same results.Comment: 8 pages, minor corrections, accepted for publication in Physical
Review
A Probe Particle in Kerr-Newman-deSitter Cosmos
We consider the force acting on a spinning charged test particle (probe
particle) with the mass m and the charge q in slow rotating the
Kerr-Newman-deSitter(KNdS) black hole with the mass M and the charge Q. We
consider the case which the spin vector of the probe particle is parallel to
the angular momentum vector of the KNdS space-time. We take account of the
gravitational spin-spin interaction under the slow rotating limit of the KNdS
space-time. When Q=M and q=m, we show that the force balance holds including
the spin-spin interaction and the motion is approximately same as that of a
particle in the deSitter space-time. This force cancellation suggests the
possibility of the existence of an exact solution of spinning multi-KNdS black
hole.Comment: 7 pages, Classical and Quantum Gravity accepte
Soccer: is scoring goals a predictable Poissonian process?
The non-scientific event of a soccer match is analysed on a strictly
scientific level. The analysis is based on the recently introduced concept of a
team fitness (Eur. Phys. J. B 67, 445, 2009) and requires the use of
finite-size scaling. A uniquely defined function is derived which
quantitatively predicts the expected average outcome of a soccer match in terms
of the fitness of both teams. It is checked whether temporary fitness
fluctuations of a team hamper the predictability of a soccer match.
To a very good approximation scoring goals during a match can be
characterized as independent Poissonian processes with pre-determined
expectation values. Minor correlations give rise to an increase of the number
of draws. The non-Poissonian overall goal distribution is just a consequence of
the fitness distribution among different teams. The limits of predictability of
soccer matches are quantified. Our model-free classification of the underlying
ingredients determining the outcome of soccer matches can be generalized to
different types of sports events
Cosmological constant and gravitational theory on D-brane
In a toy model we derive the gravitational equation on a self-gravitating
curved D-brane. The effective theory on the brane is drastically changed from
the ordinal Einstein equation. The net cosmological constant on the brane
depends on a tuning between the brane tension and the brane charges. Moreover,
non-zero matter stress tensor exists if the net cosmological constant is not
zero. This fact indicates a direct connection between matters on the brane and
the dark energy.Comment: 6 pages, minor corrections, accepted for publication in Physical
Review
Spacetime dynamics and baryogenesis in braneworld
We point out that the effective theory for the Randall-Sundrum braneworld
models with bulk fields contains the baryon number violation process depending
on the spacetime dynamics. Combining to the curvature-current interaction, the
net baryon number observed today may be explained. The resultant baryon to
entropy ratio is determined by the ratio of the Planck scales in four
dimensional and five dimensional spacetime except for the parameter for CP
violation.Comment: 8 pages, references adde
Can we live on a D-brane? -- Effective theory on a self-gravitating D-brane --
We consider a D-brane coupled with gravity in type IIB supergravity on S^5
and derive the effective theory on the D-brane in two different ways, that is,
holographic and geometrical projection methods. We find that the effective
equations on the brane obtained by these methods coincide. The theory on the
D-brane described by the Born-Infeld action is not like Einstein-Maxwell theory
in the lower order of the gradient expansion, i.e., the Maxwell field does not
appear in the theory. Thus the careful analysis and statement for cosmology on
self-gravitating D-brane should be demanded in realistic models.Comment: 13 pages, accepted for publication in Physical Review
Cosmology and two-body problem of D-branes
In this paper, we investigate the dynamics and the evolution of the scale
factor of a probe Dp-brane which move in the background of source Dp-branes.
Action of the probe brane is described by the Born-Infeld action and the
interaction with the background R-R field. When the probe brane moves away from
the source branes, it expands by power law, whose index depends on the
dimension of the brane. If the energy density of the gauge field on the brane
is subdominant, the expansion is decelerating irrespective of the dimension of
the brane. On the other hand, when the probe brane is a Nambu-Goto brane, the
energy density of the gauge field can be dominant, in which case accelerating
expansion occurs for . The accelerating expansion stops when the
brane has expanded sufficiently so that the energy density of the gauge field
become subdominant.Comment: 6 pages, 7 figures, reference added, accepted for publication in PR
Space Noncommutativity Corrections to the Cardy-Verlinde Formula
In this letter we compute the corrections to the Cardy-Verlinde formula of
Schwarzschild black holes. These corrections stem from the space
noncommutativity. Because the Schwarzschild black holes are non rotating, to
the first order of perturbative calculations, there is no any effect on the
properties of black hole due to the noncommutativity of space.Comment: 7 pages, no figures, accepted for publication in Int. J. Mod. Phys.
Semiclassical instability of the brane-world: Randall-Sundrum bubbles
We discuss the semiclassical instability of the Randall-Sundrum brane-world
model against a creation of a kind of Kaluza-Klein bubble. An example
describing such a bubble space-time is constructed from the five-dimensional
AdS-Schwarzschild metric. The induced geometry of the brane looks like the
Einstein-Rosen bridge, which connects the positive and the negative tension
branes. The bubble rapidly expands and there also form a trapped region around
it.Comment: 4 pages, 3 figures, two references adde
Cosmology of Brane-Bulk Models in Five Dimensions
We study the cosmology of models with four space and one time dimension where
our universe is a 3-brane and report a few results which extend existing work
in several directions. Assuming a stable fifth dimension, we obtain a solution
for the metric, which does not depend on any arbitrary parameters. We discuss
some implications of this result.Comment: Minor changes: brane energy conservation law and some typos
corrected. All main results unchanged. 11 pages, no figures, LaTeX fil
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