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We consider supersymmetry breaking models with a purely constant superpotential in supergravity. The supersymmetry breaking is induced for the vanishing cosmological constant. As a hidden mediation sector of supersymmetry breaking, it…

High Energy Physics - Phenomenology · Physics 2011-05-09 K. -I. Izawa , T. Kugo , T. T. Yanagida

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 show that heavy supersymmetric particles around O(100) TeV to O(1) PeV naturally appear in new inflation in which the Higgs boson responsible for the breaking of U(1)B-L plays the role of inflaton. Most important, the supersymmetric…

High Energy Physics - Phenomenology · Physics 2012-05-30 Kazunori Nakayama , Fuminobu Takahashi

The inflationary paradigm has enjoyed phenomenological success, however, a compelling particle physics realization is still lacking. The key obstruction is that the requirement of a suitably flat scalar potential is sensitive to…

High Energy Physics - Phenomenology · Physics 2011-05-12 Neil Barnaby , Marco Peloso

We reconsider a class of well motivated supersymmetric models in which inflation is associated with the breaking of a gauge symmetry G to H, with the symmetry breaking scale M~10^16 GeV. Starting with a renormalizable superpotential, we…

High Energy Physics - Phenomenology · Physics 2008-11-26 V. N. Senoguz , Q. Shafi

In F-term supergravity inflation models, scalar fields other than the inflaton generically receive a Hubble induced mass, which may restore gauge symmetries during inflation and phase transitions may occur during or after inflation as the…

High Energy Physics - Phenomenology · Physics 2013-05-30 Kohei Kamada , Kazunori Nakayama , Jun'ichi Yokoyama

Supersymmetry breaking may be linked to the formation of gaugino condensates in a hidden sector. In this work, the process of formation of the condensate is examined in a cosmological context, using an effective field theory of the gaugino…

High Energy Physics - Theory · Physics 2009-10-28 Haim Goldberg

We study an extension of the natural inflation model comprising a non-Abelian gauge sector coupled to the axion-inflaton kinetic term. We show how such non-minimal coupling serves as a source of friction for the rolling inflaton granting…

Cosmology and Nongalactic Astrophysics · Physics 2024-12-02 Martino Michelotti , Rodrigo Gonzalez Quaglia , Ema Dimastrogiovanni , Matteo Fasiello , Diederik Roest

We consider a natural new inflationary model in broken supergravity based on an R symmetry. The model predicts a concrete relation between the amplitude of primordial density fluctuations and the scale of supersymmetry breaking. The…

High Energy Physics - Phenomenology · Physics 2011-07-19 K. -I. Izawa , T. Yanagida

We show how we can implement chaotic inflation in the context of supergravity by conveniently selecting the functional form of a strong enough non-minimal coupling between the inflaton and the Ricci scalar curvature. The procedure can be…

High Energy Physics - Phenomenology · Physics 2014-12-12 C. Pallis

We revisit Higgs inflation in the framework of a minimal extension of the Standard Model gauge symmetry by a $U(1)_{B-L}$ factor. Various aspects are taken into account with particular focus on the role of the supersymmetry breaking (SUSY)…

High Energy Physics - Phenomenology · Physics 2021-09-29 Waqas Ahmed , Athanasios Karozas , George K. Leontaris

We show how we can implement within Supergravity chaotic inflation in the presence of a pole of order one or two in the kinetic mixing of the inflaton sector. This pole arises due to the selected logarithmic Kahler potentials K, which…

High Energy Physics - Phenomenology · Physics 2022-11-28 C. Pallis

Motivated by the coincidence between the Hubble scale during inflation and the typical see-saw neutrino mass scale, we present a supergravity model where the inflaton is identified with a linear combination of right-handed sneutrino fields.…

High Energy Physics - Phenomenology · Physics 2015-07-29 Jason L. Evans , Tony Gherghetta , Marco Peloso

All generic, calculable models of dynamical supersymmetry breaking have a spontaneously broken $R$ symmetry and therefore contain an $R$ axion. We show that the axion is massive in any model in which the cosmological constant is fine-tuned…

High Energy Physics - Phenomenology · Physics 2019-08-17 Jonathan Bagger , Erich Poppitz , Lisa Randall

Reheating after inflation can proceed even if the inflaton couples to Standard Model (SM) particles only gravitationally. However, particle production during the transition between de-Sitter expansion and a decelerating Universe is rather…

Cosmology and Nongalactic Astrophysics · Physics 2018-05-02 Michał Artymowski , Olga Czerwińska , Zygmunt Lalak , Marek Lewicki

We discuss models where N=1 global supersymmetry is spontaneously broken, at the classical level, in the presence of non-anomalous gauge interactions. We take such models as effective theories, valid up to some suitable scale and arising…

High Energy Physics - Phenomenology · Physics 2009-10-30 Andrea Brignole , Ferruccio Feruglio , Fabio Zwirner

We study models of inflation where the inflaton corresponds to a flat direction in field space and its mass term is generated by gravity mediated soft supersymmetry breaking at high scale. Assuming the inflaton to have non negligible…

High Energy Physics - Phenomenology · Physics 2007-05-23 Laura Covi

We review our recent results on dark matter from Starobinsky supergravity. In this context, a natural candidate for Cold Dark Matter is the gravitino. On the other hand, assuming the supersymmetry broken at scales much higher than the…

General Relativity and Quantum Cosmology · Physics 2017-05-24 Andrea Addazi , Maxim Yu. Khlopov

We show that reheating of the universe occurs spontaneously in a broad class of inflation models with f(phi)R gravity (phi is inflaton). The model does not require explicit couplings between phi and bosonic or fermionic matter fields. The…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Yuki Watanabe , Eiichiro Komatsu

In natural inflation models, the inflaton is a pseudo Nambu-Goldstone boson and the flatness of the potential is protected by shift symmetries. In this framework, a successful inflation requires the global symmetry to be spontaneously…

High Energy Physics - Phenomenology · Physics 2009-11-10 R. Gonzalez Felipe
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