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Related papers: UV Perturbations in Brane Gas Cosmology

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This investigation is concerned with cosmological scenarios based on particle physics theories that give rise to superconducting cosmic strings (whose subsequent evolution may produce stable loop configurations known as vortons). Cases in…

High Energy Physics - Phenomenology · Physics 2009-10-31 B. Carter , R. Brandenberger , A. -C. Davis , G. Sigl

An inhomogeneous version of pre--Big Bang cosmology emerges, within string theory, from quite generic initial conditions, provided they lie deeply inside the weak-coupling, low-curvature regime. Large-scale homogeneity, flatness, and…

High Energy Physics - Theory · Physics 2009-10-30 G. Veneziano

We demonstrate a first-principle analysis of the string theory landscapes in the framework of non-critical string/matrix models. In particular, we discuss non-perturbative instability, decay rate and the true vacuum of perturbative string…

High Energy Physics - Theory · Physics 2013-05-30 Chuan-Tsung Chan , Hirotaka Irie , Chi-Hsien Yeh

The present article analyses the impact on cosmology, in particular on the evolution of cosmological perturbations, of the existence of extra-dimensions. The model considered here is that of a five-dimensional Anti-de Sitter spacetime where…

High Energy Physics - Theory · Physics 2009-10-31 David Langlois

An unstable $D3$-brane universe governed by the DBI action of the tachyon field minimally coupled to a U(1) gauge boson is examined. The cosmological evolution of this coupled system, is further analyzed, in terms of the expansion rate of…

High Energy Physics - Theory · Physics 2009-11-11 Anastasios Psinas

We study the cosmological evolution based upon a $D$-dimensional action in low-energy effective string theory in the presence of second-order curvature corrections and a modulus scalar field (dilaton or compactification modulus). A…

High Energy Physics - Theory · Physics 2009-11-11 Gianluca Calcagni , Shinji Tsujikawa , M Sami

We discuss the semi-classical perturbation spectra produced in the massless fields of the low energy string action in a pre big bang type scenario. Axion fields may possess an almost scale-invariant spectrum on large scales dependent upon…

High Energy Physics - Theory · Physics 2009-10-31 E. J. Copeland , James E. Lidsey , David Wands

Cosmic strings are predicted in various extensions of the Standard Model, including grand unified theories. Depending on the symmetry-breaking pattern, they can be either topologically stable or metastable. Intriguingly, metastable strings…

High Energy Physics - Phenomenology · Physics 2025-07-17 Akifumi Chitose , Masahiro Ibe , Shunsuke Neda , Satoshi Shirai

The D-brane world is an idea that we are living on the D-brane imbedded in a 10- or 11-dimensional spacetime of string theories, aiming at the construction of realistic models from string theories. We investigate the cosmological aspects of…

High Energy Physics - Theory · Physics 2007-05-23 Inyong Cho , Eung Jin Chun , Hang Bae Kim , Yoonbai Kim

We analyze, within the framework of unified brane gravity, the weak-field perturbations caused by the presence of matter on a 3-brane. Although deviating from the Randall-Sundrum approach, the masslessness of the graviton is still…

High Energy Physics - Theory · Physics 2009-08-13 Ilya Gurwich , Aharon Davidson

We report that axions and photons exhibit instability in the presence of cosmic strings that are carrying magnetic flux in their core. The strength of the instability is determined by the symmetry breaking scale of the cosmic string theory.…

High Energy Physics - Theory · Physics 2008-10-28 Eduardo I. Guendelman , Idan Shilon

We study the perturbative stability of four settings that arise in String Theory, when dilaton potentials accompany the breaking of Supersymmetry, in the USp(32) and U(32) orientifold models, and also in the heterotic SO(16)xSO(16) model.…

High Energy Physics - Theory · Physics 2019-02-20 I. Basile , J. Mourad , A. Sagnotti

We study the cosmological impact of ultralight dark matter (ULDM) with a quadratic coupling to Standard Model particles. In addition to the suppression of small-scale power from ULDM itself, the coupling induces a variation of fundamental…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-19 Subhajit Ghosh , Kimberly K. Boddy , Tien-Tien Yu

We discuss the generation and evolution of density perturbations during the large curvature phase of string cosmology. We find that perturbations in the scalar components of the metric evolve with cosmic time as $\exp (\gamma H_st)$ where…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Michele Maggiore , Riccardo Sturani

Using some simple toy models, we explore the nature of the brane-bulk interaction for cosmological models with a large extra dimension. We are in particular interested in understanding the role of the bulk gravitons, which from the point of…

High Energy Physics - Theory · Physics 2008-11-26 Pierre Binetruy , Martin Bucher , Carla Carvalho

A broad class of two-dimensional loop-corrected dilaton gravity models exhibit cosmological solutions that interpolate between the string perturbative vacuum and a background with asymptotically flat metric and linearly growing dilaton. The…

High Energy Physics - Theory · Physics 2011-07-19 M. Gasperini , G. Veneziano

Based upon a novel paradigm of the galaxy formation under UV background, the evolutionary bifurcation of pregalactic clouds is confronted with observations on elliptical and spiral galaxies. The theory predicts that the dichotomy between…

Astrophysics · Physics 2009-10-31 Hajime Susa , Masayuki Umemura

We consider the evolution of scalar perturbations in a class of non-singular bouncing universes obtained with higher-order corrections to the low-energy bosonic string action. We show that previous studies have relied on a singular…

High Energy Physics - Theory · Physics 2007-05-23 Cyril Cartier

We study the dilaton stabilization in the D-brane world in which a D-brane constitutes our universe. The dilaton can be stabilized due to the interplay between the D-brane tension and the negative scalar curvature of extra dimensions.…

High Energy Physics - Theory · Physics 2009-11-11 Hang Bae Kim

After an introduction to the problem of cosmological structure formation, we develop gauge invariant cosmological perturbation theory. We derive the first order perturbation equations of Einstein's equations and energy momentum…

Astrophysics · Physics 2010-12-09 Ruth Durrer