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We estimate the production of gravitinos during and after the end of a period of warm inflation, a model in which radiation is produced continuously as the field rolls down the potential producing dissipation. We find that gravitino…

Astrophysics · Physics 2009-10-31 A. N. Taylor , Andrew R. Liddle

We point out that supergravity effects enable the inflaton to decay into all matter fields, including the visible and the supersymmetry breaking sectors, once the inflaton acquires a non-vanishing vacuum expectation value. The new decay…

High Energy Physics - Phenomenology · Physics 2009-11-11 Motoi Endo , Masahiro Kawasaki , Fuminobu Takahashi , T. T. Yanagida

The gravitational waves measured at LIGO are presumed here to come from merging primordial black holes. We ask how these primordial black holes could arise through inflationary models while not conflicting with current experiments. Among…

Cosmology and Nongalactic Astrophysics · Physics 2017-04-11 Nicholas Orlofsky , Aaron Pierce , James D. Wells

A small tensor-to-scalar ratio $r$ may lead to distinctive phenomenology of high-scale supersymmetry. Assuming the same origin of SUSY breaking between the inflation and visible sector, we show model independent features. The simplest…

High Energy Physics - Phenomenology · Physics 2015-08-26 Sibo Zheng

Using a no-scale supergravity framework, we construct an SO(10) model that makes predictions for cosmic microwave background observables similar to those of the Starobinsky model of inflation, and incorporates a double-seesaw model for…

High Energy Physics - Phenomenology · Physics 2016-11-15 John Ellis , Marcos A. G. Garcia , Natsumi Nagata , Dimitri V. Nanopoulos , Keith A. Olive

We study a class of non-local, action-based, and purely gravitational models. These models seek to describe a cosmology in which inflation is driven by a large, bare cosmological constant that is screened by the self-gravitation between the…

General Relativity and Quantum Cosmology · Physics 2016-08-17 N. C. Tsamis , R. P. Woodard

We extend our previous study of supersymmetric Higgs inflation in the context of no-scale supergravity and grand unification, to include models based on the flipped SU(5) and the Pati-Salam group. Like the previous SU(5) GUT model, these…

High Energy Physics - Phenomenology · Physics 2016-09-01 John Ellis , Hong-Jian He , Zhong-Zhi Xianyu

We construct a hybrid-inflation model where the inflaton potential is generated radiatively, as gauge symmetries guarantee it to be accidentally flat at tree level. The model can be regarded as a small-field version of Natural Inflation,…

Cosmology and Nongalactic Astrophysics · Physics 2024-11-18 Felix Brümmer , Giacomo Ferrante , Michele Frigerio

In general the gravitino mass and/or the soft supersymmetry breaking masses in the observable sector can be much larger than the TeV scale. Depending on the relation between the masses, new important channels for gravitino production in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Rouzbeh Allahverdi , Steen Hannestad , Asko Jokinen , Anupam Mazumdar , Silvia Pascoli

Effects of the unstable gravitino on the big-bang nucleosynthesis (BBN) and its implications to particle cosmology are discussed. If the gravitino mass is smaller than \sim 20 TeV, lifetime of the gravitino becomes longer than \sim 1sec and…

High Energy Physics - Phenomenology · Physics 2009-11-11 Takeo Moroi

Recent theoretical results indicate that the detection of primordial gravity waves from inflation may be a hopeless task. First, foregrounds from lensing put a strict lower limit on the detectability of the B-mode polarization signal in the…

Astrophysics · Physics 2015-06-24 William H. Kinney

The primordial Universe can be used as a laboratory to set constraints on quantum gravity. In the framework of Loop Quantum Cosmology, we show that such a proposal for quantum gravity not only solves for the big bang singularity issue but…

General Relativity and Quantum Cosmology · Physics 2012-06-08 Julien Grain

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

Primordial black holes (PBHs) are one of the candidates to explain the gravitational wave (GW) signals observed by the LIGO detectors. Among several phenomena in the early Universe, cosmic inflation is a major example to generate PBHs from…

Cosmology and Nongalactic Astrophysics · Physics 2017-06-14 Keisuke Inomata , Masahiro Kawasaki , Kyohei Mukaida , Yuichiro Tada , Tsutomu T. Yanagida

Cosmological production of scalar, non-minimally coupled dark matter depends on the specifics of the inflationary model under consideration. We analyze both Starobinsky inflation and a quadratic potential, solve the full background…

General Relativity and Quantum Cosmology · Physics 2026-02-24 Jose A. R. Cembranos , Luis J. Garay , Álvaro Parra-López , Javier Ortega del Río

We show that the gravitino-overproduction problem is prevalent among inflation models in supergravity. An inflaton field \phi generically acquires (effective) non-vanishing auxiliary field G_\phi, if the K\"ahler potential is non-minimal.…

High Energy Physics - Phenomenology · Physics 2009-11-11 Masahiro Kawasaki , Fuminobu Takahashi , T. T. Yanagida

Motivated by the absence of signals of new physics in both searches for new particles at LHC and for a Weakly Interacting Massive Particle (WIMP) dark matter candidate, we consider a scenario where supersymmetry is broken at a scale above…

High Energy Physics - Phenomenology · Physics 2017-05-10 Karim Benakli , Yifan Chen , Emilian Dudas , Yann Mambrini

We critically review the role of cosmological moduli in determining the post-inflationary history of the universe. Moduli are ubiquitous in string and M-theory constructions of beyond the Standard Model physics, where they parametrize the…

High Energy Physics - Theory · Physics 2015-08-06 Gordon Kane , Kuver Sinha , Scott Watson

Recent anomalies in cosmic rays could be due to dark matter annihilation in our galaxy. In order to get the required large cross-section to explain the data while still obtaining the right relic density, we rely on a non standard thermal…

High Energy Physics - Phenomenology · Physics 2009-09-02 Bhaskar Dutta , Louis Leblond , Kuver Sinha

In all supersymmetric theories, gravitinos, with mass suppressed by the Planck scale, are an obvious candidate for dark matter; but if gravitinos ever reached thermal equilibrium, such dark matter is apparently either too abundant or too…

High Energy Physics - Phenomenology · Physics 2017-08-03 Raymond T. Co , Francesco D'Eramo , Lawrence J. Hall , Keisuke Harigaya