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Related papers: A brane world cosmological solution to the graviti…

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In the present work we discuss baryon asymmetry in the non-thermal leptogenesis scenario and gravitino cosmology for an unstable gravitino with inflaton decay. We take into account two production mechanisms for gravitino, namely thermal…

High Energy Physics - Phenomenology · Physics 2009-12-15 Grigoris Panotopoulos

We investigate the light gravitino regeneration rate in the early Universe in models based on $N=1$ supergravity. Motivated by a recent claim by Fischler, we evaluate finite-temperature effects on the gravitino regeneration rate due to the…

High Energy Physics - Phenomenology · Physics 2009-09-11 John Ellis , D. V. Nanopoulos , Keith A. Olive , Soo-Jong REY

We derive big-bang nucleosynthesis (BBN) constraints on both unstable and stable gravitino taking account of recent progresses in theoretical study of the BBN processes as well as observations of primordial light-element abundances. In the…

High Energy Physics - Phenomenology · Physics 2009-01-28 Masahiro Kawasaki , Kazunori Kohri , Takeo Moroi , Akira Yotsuyanagi

Gravitinos are expected to be produced in any local supersymmetric model. Using their abundance prediction as a function of the reheating energy scale, it is argued that the next generation of Cosmic Microwave Background experiments could…

High Energy Physics - Phenomenology · Physics 2009-11-10 A. Barrau , N. Ponthieu

We summarise the approach to brane cosmology known as ``mirage cosmology'' and use it to determine the Friedmann equation on a 3-brane embedded in different bulk spacetimes all with one or more extra dimensions. Usually, when there is more…

High Energy Physics - Theory · Physics 2007-05-23 D. A. Steer , M. F. Parry

We review a solution of the cosmological constant problem in a brane-world model with infinite-volume extra dimensions. The solution is based on a nonlinear generally covariant theory of a metastable graviton that leads to a large-distance…

High Energy Physics - Theory · Physics 2017-08-23 Gia Dvali , Gregory Gabadadze , M. Shifman

We investigate the so-called superWIMP scenario with gravitino as the lightest supersymmetric particle (LSP) in the context of non-standard cosmology, in particular, brane world cosmology. As a candidate of the next-to-LSP (NLSP), we…

High Energy Physics - Phenomenology · Physics 2008-11-26 Nobuchika Okada , Osamu Seto

In this work, we explore the "degenerate gravitino" scenario where the mass difference between the gravitino and the lightest MSSM particle is much smaller than the gravitino mass itself. In this case, the energy released in the decay of…

High Energy Physics - Phenomenology · Physics 2010-05-27 Lotfi Boubekeur , Ki Young Choi , Roberto Ruiz de Austri , Oscar Vives

We consider a single 3-brane situated between two bulk spacetimes that posses the same cosmological constant, but whose metrics do not posses a $Z_{2}$-symmetry. On each side of the brane, the bulk is a solution to Gauss-Bonnet gravity.…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Kenichiro Konya

Gravitinos are generically produced by inflaton decays, which place tight constraints on inflation models as well as supersymmetry breaking scale. We revisit the gravitino production from decays of the inflaton and the supersymmetry…

High Energy Physics - Phenomenology · Physics 2014-07-15 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

Gravitino produced in the inflationary universe are studied. When the gravitino decays into a neutrino and a sneutrino, the emitted high energy neutrinos scatter off the background neutrinos and produce charged leptons (mainly electrons and…

High Energy Physics - Phenomenology · Physics 2009-10-28 M. Kawasaki , T. Moroi

We study the curvaton dynamics in brane-world cosmologies. Assuming that the inflaton field survives without decay after the end of inflation, we apply the curvaton reheating mechanism to Randall-Sundrum and to its curvature corrections:…

General Relativity and Quantum Cosmology · Physics 2009-11-11 Eleftherios Papantonopoulos , Vassilios Zamarias

Starting with the vacuum fluctuation, it is known that gravitinos will be created just after inflation, with number density $\sim 10^{-2}M^3$ where $M$ is the mass of the inflaton. Here, we argue that creation may be expected to continue,…

High Energy Physics - Phenomenology · Physics 2009-10-31 David H Lyth

We reconsider cosmological constraints on extra dimension theories from the excess production of Kaluza-Klein gravitons. We point out that, if the normalcy temperature is above 1 GeV, then graviton states produced at this temperature will…

High Energy Physics - Phenomenology · Physics 2009-11-10 Cosmin Macesanu , Mark Trodden

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

One proposed solution of the moduli problem of string cosmology requires that the moduli are quite heavy, their decays reheating the universe to temperatures above the scale of nucleosynthesis. In many of these scenarios, the moduli are…

High Energy Physics - Phenomenology · Physics 2009-11-11 Michael Dine , Ryuichiro Kitano , Alexander Morisse , Yuri Shirman

The self-tuning brane scenario is an attempt to solve the cosmological constant problem in the context of extra dimensions. Rather than making the vacuum energy small, this approach proceeds by removing the gravitational effect of vacuum…

High Energy Physics - Theory · Physics 2009-11-07 Sean M. Carroll , Laura Mersini

The Friedmann equation for a positive tension brane situated between two bulk spacetimes that posses the same 5D cosmological constant, but which does not posses a Z_2 symmetry of the metric itself is derived, and the possible effects of…

High Energy Physics - Phenomenology · Physics 2008-11-26 Anne-Christine Davis , Ian Vernon , Stephen C. Davis , Warren B. Perkins

We study the consequences of the gravitino decay into dark matter. We suppose that the lightest neutralino is the main component of dark matter. In our framework gravitino is heavy enough to decay before Big Bang Nucleosynthesis starts. We…

High Energy Physics - Phenomenology · Physics 2007-06-29 David Gherson

We discuss the creation of massless particles in a Universe, which transits from a radiation-dominated era to any other expansion law. We calculate in detail the generation of gravitons during the transition to a matter dominated era. We…

Cosmology and Nongalactic Astrophysics · Physics 2010-08-13 Ruth Durrer , Massimiliano Rinaldi
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