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New exact solutions of brane-world cosmology are given. These solutions include an arbitrary constant C, which is determined by the geometry outside the brane and which affects the cosmological evolution in the brane-world. If C is zero,…

High Energy Physics - Theory · Physics 2009-10-31 Shinji Mukohyama

Exact global solutions of five-dimensional cosmological models compactified on a $S_1/Z_2$ orbifold with two 3-branes are presented, and evolution of a simple model is studied. It is found that on all 4D spacetime hypersurfaces, except a…

High Energy Physics - Theory · Physics 2014-11-18 Hongya Liu

We consider the cosmology of a ``3-brane universe'' in a five dimensional (bulk) space-time with a cosmological constant. We show that Einstein's equations admit a first integral, analogous to the first Friedmann equation, which governs the…

High Energy Physics - Theory · Physics 2009-10-07 Pierre Binetruy , Cedric Deffayet , Ulrich Ellwanger , David Langlois

We study brane-world solutions of five-dimensional supergravity in singular spaces. We exhibit a self-tuned four-dimensional cosmological constant when five-dimensional supergravity is broken by an arbitrary tension on the brane-world. The…

High Energy Physics - Theory · Physics 2009-10-31 Ph. Brax , A. C. Davis

Recently a brane world perspective on the cosmological constant and the hierarchy problems was presented. Here, we elaborate on some aspects of that particular scenario and discuss the stability of the stationary brane solution and the…

High Energy Physics - Theory · Physics 2009-11-07 Eanna Flanagan , Richard J. Hill , Nicholas Jones , S. -H. Henry Tye , Ira Wasserman

We study the stabilization of one spatial dimension in (p+1+1)-dimensional spacetime in the presence of $p$-dimensional brane(s), a bulk cosmological constant and the Casimir force generated by a conformally coupled scalar field. We find…

High Energy Physics - Phenomenology · Physics 2009-10-31 Ralf Hofmann , Panagiota Kanti , Maxim Pospelov

We develop a possible cosmology for a Universe with n additional spatial dimensions of variable scale, and an associated scalar field, the radion, which is distinct from the field responsible for inflation, the inflaton. Based on a…

High Energy Physics - Phenomenology · Physics 2009-10-31 Eanna E. Flanagan , S. -H. Henry Tye , Ira Wasserman

We discuss cosmology of models with universal extra dimensions, where the Standard Model degrees of freedom live in a $4+n$ dimensional brane, with $n$ compact and small extra spatial dimensions. In these models, the simplest way to obtain…

High Energy Physics - Phenomenology · Physics 2008-11-26 Anupam Mazumdar , R. N. Mohapatra , A. Pérez-Lorenzana

In these lectures, we present cosmological vacuum solutions of Horava-Witten theory and discuss their physical properties. We begin by deriving the five-dimensional effective action of strongly coupled heterotic string theory by performing…

High Energy Physics - Theory · Physics 2007-05-23 Andre Lukas , Burt A. Ovrut , Daniel Waldram

One of the central points of the ekpyrotic cosmological scenario based on Horava-Witten theory is that we live on a negative tension brane. However, the tension of the visible brane is positive in the usual HW phenomenology with stronger…

High Energy Physics - Theory · Physics 2009-09-29 Renata Kallosh , Lev Kofman , Andrei Linde

We address the problem of the cosmological constant within the Randall-Sundrum scenario with a brane stabilization mechanism. We consider brane tensions of general form. We examine the conditions under which a small change of the positive…

High Energy Physics - Theory · Physics 2009-10-31 N. Tetradis

We discuss the stability of the higher-dimensional de Sitter (dS) brane solutions with two-dimensional internal space in the Einstein-Maxwel theory. We show that an instability appears in the scalar-type perturbations with respect to the dS…

High Energy Physics - Theory · Physics 2008-11-26 Masato Minamitsuji

We study two $(4+n)$-dimensional branes embedded in $(5+n)$-dimensional spacetime. Using the gradient expansion approximation, we find that the effective theory is described by $(4+n)$-dimensional scalar-tensor gravity with a specific…

High Energy Physics - Theory · Physics 2014-11-20 S. Feranie , Arianto , Freddy P. Zen

We derive a general formalism for constructing a four-dimensional effective action for the radion field in 5 dimensions, taking into account the possible dependence of the scale factor on the internal coordinate. First and second variations…

High Energy Physics - Phenomenology · Physics 2008-11-26 Panagiota Kanti , Keith A. Olive , Maxim Pospelov

The combined Einstein equations and scalar equation of motion in the Horava-Witten scenario of the strongly coupled heterotic string compactified on a Calabi-Yau manifold are solved in the presence of additional matter densities on the…

High Energy Physics - Theory · Physics 2009-01-07 U. Ellwanger

Low-energy effective theories provide the natural description of four-dimensional physics in higher-dimensional geometries, where the imprint of the bulk appears as parameters of the lower dimensional theory. Motivated by the recent…

High Energy Physics - Theory · Physics 2026-03-11 Soham Bhattacharyya , Soumitra SenGupta

We consider the static domain wall braneworld scenario constructed from the Palatini formalism $f(\mathcal{R})$ theory. We check the self-consistency under scalar perturbations. By using the scalar-tensor formalism we avoid dealing with the…

High Energy Physics - Theory · Physics 2018-07-25 Bao-Min Gu , Yu-Xiao Liu , Yuan Zhong

We consider the cosmology of the reduced 5D Horava-Witten M-Theory (HW) with volume modulus and treating matter on the orbifold planes to first order. It is seen that one can recover the FRW cosmology in the Hubble expansion era with…

High Energy Physics - Theory · Physics 2007-05-23 R. Arnowitt , J. Dent , B. Dutta

The cosmology of the Randall-Sundrum scenario for a positive tension brane in a 5-D Universe with localized gravity has been studied previously. In the radiation-dominated Universe, it was suggested that there are two solutions for the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Eanna E. Flanagan , S. -H. Henry Tye , Ira Wasserman

We consider a D3-brane as boundary of a five dimensional charged anti de Sitter black hole. We show that the charge of the black hole induces a regular cosmological evolution for the scale factor of the brane, with a smooth transition…

High Energy Physics - Theory · Physics 2010-04-05 Sudipta Mukherji , Marco Peloso
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