8,240 research outputs found
Effective Field Theory Approach to String Gas Cosmology
We derive the 4D low energy effective field theory for a closed string gas on
a time dependent FRW background. We examine the solutions and find that
although the Brandenberger-Vafa mechanism at late times no longer leads to
radion stabilization, the radion rolls slowly enough that the scenario is still
of interest. In particular, we find a simple example of the string inspired
dark matter recently proposed by Gubser and Peebles.Comment: 19 pages, 2 figures, comments adde
Linear Perturbations in Brane Gas Cosmology
We consider the effect of string inhomogeneities on the time dependent
background of Brane Gas Cosmology. We derive the equations governing the linear
perturbations of the dilaton-gravity background in the presence of string
matter sources. We focus on long wavelength fluctuations and find that there
are no instabilities. Thus, the predictions of Brane Gas Cosmology are robust
against the introduction of linear perturbations. In particular, we find that
the stabilization of the extra dimensions (moduli) remains valid in the
presence of dilaton and string perturbations.Comment: 17 pages, 1 figur
Late time evolution of brane gas cosmology and compact internal dimensions
We study the late-time behavior of a universe in the framework of brane gas
cosmology. We investigate the evolution of a universe with a gas of
supergravity particles and a gas of branes. Considering the case when different
dimensions are anisotropically wrapped by various branes, we have derived
Friedman-like equations governing the dynamics of wrapped and unwrapped
subvolumes. We point out that the compact internal dimensions are wrapped by
three or higher dimensional branes.Comment: 16 pages, typos, references, comment on the possibility of
stabilizing the internal dimensions with fluxe
Dynamical decompactification from brane gases in eleven-dimensional supergravity
Brane gas cosmology provides a dynamical decompactification mechanism that
could account for the number of spacetime dimensions we observe today. In this
work we discuss this scenario taking into account the full bosonic sector of
eleven-dimensional supergravity. We find new cosmological solutions that can
dynamically explain the existence of three large spatial dimensions
characterised by an universal asymptotic scaling behaviour and a large number
of initially unwrapped dimensions. This type of solutions enlarge the possible
initial conditions of the Universe in the Hagedorn phase and consequently can
potentially increase the probability of dynamical decompactification from
anisotropically wrapped backgrounds.Comment: 8 figures, JHEP3 styl
String windings in the early universe
We study string dynamics in the early universe. Our motivation is the
proposal of Brandenberger and Vafa, that string winding modes may play a key
role in decompactifying three spatial dimensions. We model the universe as a
homogeneous but anisotropic 9-torus filled with a gas of excited strings. We
adopt initial conditions which fix the dilaton and the volume of the torus, but
otherwise assume all states are equally likely. We study the evolution of the
system both analytically and numerically to determine the late-time behavior.
We find that, although dynamical evolution can indeed lead to three large
spatial dimensions, such an outcome is not statistically favored.Comment: 26 pages, LaTeX, 4 eps figure
Stabilization of Extra Dimensions at Tree Level
By considering the effects of string winding and momentum modes on a time
dependent background, we find a method by which six compact dimensions become
stabilized naturally at the self-dual radius while three dimensions grow large.Comment: 15 pages, 2 figures, minor typos correcte
Interaction Rates in String Gas Cosmology
We study string interaction rates in the Brandenberger-Vafa scenario, the
very early universe cosmology of a gas of strings. This cosmology starts with
the assumption that all spatial dimensions are compact and initially have
string scale radii; some dimensions grow due to some thermal or quantum
fluctuation which acts as an initial expansion velocity. Based on simple
arguments from the low energy equations of motion and string thermodynamics, we
demonstrate that the interaction rates of strings are negligible, so the common
assumption of thermal equilibrium cannot apply. We also present a new analysis
of the cosmological evolution of strings on compact manifolds of large radius.
Then we discuss modifications that should be considered to the usual
Brandenberger-Vafa scenario. To confirm our simple arguments, we give a
numerical calculation of the annihilation rate of winding strings. In
calculating the rate, we also show that the quantum mechanics of strings in
small spaces is important.Comment: 28pp, 3 figures, RevTeX
Volume Stabilization and Acceleration in Brane Gas Cosmology
We investigate toy cosmological models in (1+m+p)-dimensions with gas of
p-branes wrapping over p-compact dimensions. In addition to winding modes, we
consider the effects of momentum modes corresponding to small vibrations of
branes and find that the extra dimensions are dynamically stabilized while the
others expand. Adding matter, the compact volume may grow slowly depending on
the equation of state. We also obtain solutions with winding and momentum modes
where the observed space undergoes accelerated expansion.Comment: 20 pages, 3 figures, v2: comments and references added, to appear in
JCA
String Gas Cosmology
We present a critical review and summary of String Gas Cosmology. We include
a pedagogical derivation of the effective action starting from string theory,
emphasizing the necessary approximations that must be invoked. Working in the
effective theory, we demonstrate that at late-times it is not possible to
stabilize the extra dimensions by a gas of massive string winding modes. We
then consider additional string gases that contain so-called enhanced symmetry
states. These string gases are very heavy initially, but drive the moduli to
locations that minimize the energy and pressure of the gas. We consider both
classical and quantum gas dynamics, where in the former the validity of the
theory is questionable and some fine-tuning is required, but in the latter we
find a consistent and promising stabilization mechanism that is valid at
late-times. In addition, we find that string gases provide a framework to
explore dark matter, presenting alternatives to CDM as recently
considered by Gubser and Peebles. We also discuss quantum trapping with string
gases as a method for including dynamics on the string landscape.Comment: 55 pages, 1 figure, minor corrections, version to appear in Reviews
of Modern Physic
Stabilization of Extra Dimensions and The Dimensionality of the Observed Space
We present a simple model for the late time stabilization of extra
dimensions. The basic idea is that brane solutions wrapped around extra
dimensions, which is allowed by string theory, will resist expansion due to
their winding mode. The momentum modes in principle work in the opposite way.
It is this interplay that leads to dynamical stabilization. We use the idea of
democratic wrapping \cite{art5}-\cite{art6}, where in a given decimation of
extra dimensions, all possible winding cases are considered. To simplify the
study further we assumed a symmetric decimation in which the total number of
extra dimensions is taken to be where N can be called the order of the
decimation. We also assumed that extra dimensions all have the topology of
tori. We show that with these rather conservative assumptions, there exists
solutions to the field equations in which the extra dimensions are stabilized
and that the conditions do not depend on . This fact means that there exists
at least one solution to the asymmetric decimation case. If we denote the
number of observed space dimensions (excluding time) by , the condition for
stabilization is for pure Einstein gravity and for dilaton
gravity massaged by string theory parameters.Comment: Final versio
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