English
Related papers

Related papers: Moduli Decays and Gravitinos

200 papers

Moduli fields generically produce strong dark matter -- radiation and baryon -- radiation isocurvature perturbations through their decay if they remain light during inflation. We show that existing upper bounds on the magnitude of such…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-05 Martin Lemoine , Jerome Martin , Jun'ichi Yokoyama

Light moduli fields, gravitationally coupled scalar fields with no classical potential and which are expected to emerge as remnants from string theory compactification, are dangerous to cosmology in that 1. their late-time decays may…

High Energy Physics - Phenomenology · Physics 2021-12-24 Howard Baer , Vernon Barger , Robert Wiley Deal

Superstring theory, models with extra dimensions and other SUSY models generically predict that the coupling constants are in fact vacuum expectation values of fields like the dilaton, moduli etc. Assuming some of these fields are light…

Astrophysics · Physics 2007-05-23 Lev Kofman

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 investigate the cosmological gravitino problem in gauge-mediated supersymmetry breaking models, where the gravitino becomes in general the lightest supersymmetric particle (LSP). In order to avoid the overclosure of the stable gravitino,…

High Energy Physics - Phenomenology · Physics 2009-10-31 T. Asaka , K. Hamaguchi , Koshiro Suzuki

Gravitino problem is discussed in detail. We derive an upperbound on the reheating temperature from the constraints of the big-bang nucleosynthesis and the present mass density of the universe. Compared to previous works, we have improve…

High Energy Physics - Phenomenology · Physics 2016-09-01 Takeo Moroi

It is widely accepted that moduli in the mass range 10eV - $10^4$GeV which start to oscillate with an amplitude of the order of the Planck scale either jeopardize successful predictions of nucleosynthesis or overclose the Universe. It is…

High Energy Physics - Theory · Physics 2007-05-23 Natalia Shuhmaher , Robert Brandenberger

We study non-thermal gravitino production in the minimal supergravity inflation. In this minimal model utilizing orthogonal nilpotent superfields, the particle spectrum includes only graviton, gravitino, inflaton, and goldstino. We find…

High Energy Physics - Phenomenology · Physics 2017-02-23 Fuminori Hasegawa , Kyohei Mukaida , Kazunori Nakayama , Takahiro Terada , Yusuke Yamada

We propose the gravitino dark matter in the gravity mediated supersymmetry breaking scenario. The mass hierarchies between the gravitino and other superparticles can be achieved by the nontrivial K\"ahler metric of the supersymmetry…

High Energy Physics - Phenomenology · Physics 2015-08-05 Hajime Otsuka

We discuss the relic problem of string gas cosmology (SGC) using gravitinos and magnetic monopoles as examples. Since SGC operates near or at the Hagedorn temperature, relics are produced copiously; in the absence of dilution, their…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-06 Diana Battefeld , Thorsten Battefeld

We consider cosmological consequences of a heavy axino, decaying to the neutralino in R-parity conserving models. The importance and influence of the axino decay on the resultant abundance of neutralino dark matter depends on the lifetime…

High Energy Physics - Phenomenology · Physics 2008-06-19 Ki-Young Choi , Jihn E. Kim , Hyun Min Lee , Osamu Seto

By using a string-inspired modular invariant supergravity, which was proved well to explain WMAP observations appropriately, a mechanism of supersymmetry breaking (SSB) and Gravitino Production just after the end of inflation are…

High Energy Physics - Phenomenology · Physics 2010-03-17 Kenji Takagi , Yuta Koshimizu , Toyokazu Fukuoka , Hikoya Kasari , Mitsuo J. Hayashi

Various authors have noted that in particular models, the upper bound on the axion decay constant may not hold. We point out that within supersymmetry, this is a generic issue. For large decay constants, the cosmological problems associated…

High Energy Physics - Phenomenology · Physics 2009-11-07 T. Banks , M. Dine , M. Graesser

We estimate the abundance of the coherent oscillation of moduli, which linearly couple to matter fields through higher dimensional operators. During the (p)reheating after inflation, matter particles are efficiently produced and it can…

High Energy Physics - Phenomenology · Physics 2019-03-18 Daisuke Hagihara , Koichi Hamaguchi , Kazunori Nakayama

Moduli fields, which parameterize perturbative flat directions of the potential in supersymmetric theories, are natural candidates to act as inflatons. An inflationary potential on moduli space can result if the scale of dynamical SUSY…

High Energy Physics - Theory · Physics 2009-10-28 Scott Thomas

We show that the cosmological moduli problem is solved, without relying on huge late-time entropy production, if the universal cutoff scale of the theory is a few orders of magnitude smaller than the Planck scale. We obtain a general…

High Energy Physics - Phenomenology · Physics 2013-05-30 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

We study the cosmological inflation from the viewpoint of the moduli stabilization. We study the scenario that the superpotential has a large value during the inflation era enough to stabilize moduli, but it is small in the true vacuum.…

High Energy Physics - Theory · Physics 2015-05-20 Tatsuo Kobayashi , Manabu Sakai

We consider a recent model with sub-millimeter sized extra dimensions, where the field that determines the size of the extra dimensions (the radion) also acts as an inflaton. The radion is also a stable modulus, and its coherent…

High Energy Physics - Phenomenology · Physics 2009-09-17 Csaba Csaki , Michael Graesser , John Terning

Gravitinos are a fundamental prediction of supergravity, their mass ($m_{G}$) is informative of the value of the SUSY breaking scale, and, if produced during reheating, their number density is a function of the reheating temperature…

High Energy Physics - Phenomenology · Physics 2018-07-11 Emanuela Dimastrogiovanni , Lawrence M. Krauss

We consider the potential problems due to the production of inflatinos and gravitinos after inflation. Inflationary models with a single scale set by the microwave background anisotropies have a low enough reheat temperature to avoid…

High Energy Physics - Phenomenology · Physics 2009-09-15 Hans Peter Nilles , Keith A. Olive , Marco Peloso