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Related papers: Preserving Flat Directions During Inflation

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We propose a new class of inflationary models in which the scalar field potential governing inflation is generated by the same non-perturbative gauge dynamics that may lead to supersymmetry breaking. Such models satisfy constraints from…

High Energy Physics - Phenomenology · Physics 2011-05-23 William H. Kinney , Antonio Riotto

We consider models of inflation in supergravity with a shift symmetry. We focus on models with one moduli and one inflaton field. The presence of this symmetry guarantees the existence of a flat direction for the inflaton field. Mildly…

High Energy Physics - Theory · Physics 2009-11-11 Philippe Brax , Jerome Martin

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, when connected with monopoles, the flat $D$-flat direction breaking the local $U(1)_{B-L}$ symmetry as an extension of the minimal supersymmetric standard model can be responsible for the signal of a stochastic gravitational…

High Energy Physics - Phenomenology · Physics 2023-12-15 Rinku Maji , Wan-Il Park

We argue that all necessary ingredients for successful inflation are present in the flat directions of the minimal supersymmetric standard model (MSSM). Out of many gauge invariant combinations of the squarks, sleptons and Higgses, there…

High Energy Physics - Phenomenology · Physics 2008-11-26 Rouzbeh Allahverdi

We consider a simple inflation model with a complex scalar field coupled to gravity non-minimally. Both the modulus and the angular directions of the complex scalar are slowly rolling, leading to two-field inflation. The modulus direction…

High Energy Physics - Phenomenology · Physics 2015-05-28 Jinn-Ouk Gong , Hyun Min Lee

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

We consider the supersymmetry breaking effects on typical inflation models with different types of K\"ahler potential. The critical size of supersymmetry-breaking scale, above which the flatness of the inflaton potential is spoiled,…

High Energy Physics - Theory · Physics 2015-06-22 Hiroyuki Abe , Shuntaro Aoki , Fuminori Hasegawa , Yusuke Yamada

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

We consider the Higgs inflation in the extension of the Standard Model with two Higgs doublets coupled to gravity non-minimally. In the presence of an approximate global U(1) symmetry in the Higgs sector, both radial and angular modes of…

High Energy Physics - Phenomenology · Physics 2015-06-04 Jinn-Ouk Gong , Sin Kyu Kang , Hyun Min Lee

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

We study Affleck-Dine leptogenesis via the L H_u flat direction in supersymmetric theories. We find that the baryon asymmetry is enhanced when the energy scale of the inflation is sufficiently low. Especially, we consider models of low…

High Energy Physics - Phenomenology · Physics 2009-11-07 T. Asaka

Inflation is a promising solution to many problems of the standard Big-Bang cosmology. Nevertheless, inflationary models have proved less compelling. In this chapter, we discuss why supersymmetry has led to more natural models of inflation.…

High Energy Physics - Phenomenology · Physics 2007-05-23 Lisa Randall

Flat directions in the Minimal Supersymmetric Standard Model (MSSM) can become unstable due to radiative corrections, and the global minimum of the (zero temperature) potential can lie at large values of the squark and/or slepton fields.…

High Energy Physics - Phenomenology · Physics 2009-09-15 Toby Falk , Keith A. Olive , Leszek Roszkowski , Anupam Singh , Mark Srednicki

Several recent proposals to embed inflation into high-energy physics rely on inflationary dynamics characterized by a strongly non-geodesic motion in negatively curved field space. This naturally leads to a transient instability of…

High Energy Physics - Theory · Physics 2019-11-20 Jacopo Fumagalli , Sebastian Garcia-Saenz , Lucas Pinol , Sébastien Renaux-Petel , John Ronayne

We show that the non-linear evolution of long wavelength perturbations may be important in a wide class of inflationary scenarios. We develop a solution for the evolution of such nonlinear perturbations which is exact to first order in a…

General Relativity and Quantum Cosmology · Physics 2009-08-29 Niayesh Afshordi , Robert Brandenberger

Flat manifold leptogenesis a la Affleck-Dine is investigated with the slepton and Higgs fields, L, H_u, H_d, in the supersymmetric standard model. The multi-dimensional motion of these scalar fields is realized in the case that the L H_u…

High Energy Physics - Phenomenology · Physics 2009-11-07 Masato Senami , Katsuji Yamamoto

We show that the natural presence of flat directions in supersymmetric theories allows for nonrestoration of global and/or gauge symmetries. This has important cosmological consequences for supersymmetric GUTs and in particular it offers a…

High Energy Physics - Phenomenology · Physics 2009-10-31 Borut Bajc , Goran Senjanovic

We focus on a simple, natural and predictive T model of inflation in Supergravity employing as inflaton the Higgs field which leads to the spontaneous breaking of a U(1)_(B-L) symmetry at the SUSY GUT scale. We use a renormalizable…

High Energy Physics - Phenomenology · Physics 2023-07-28 C. Pallis

In the Standard Model, the Higgs potential develops an instability at high field values when the quartic self-coupling runs negative. Large quantum fluctuations during cosmic inflation could drive the Higgs field beyond the potential…

High Energy Physics - Phenomenology · Physics 2026-01-07 G. Franciolini , A. Kehagias , A. Riotto
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