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Related papers: Dilatonic Inflation, Gravitino and Reheating in Mo…

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Reheating after R^2 inflation proceeds through gravitational particle production of conformally noninvariant fields. We argue that the nonvanishing expectation value of flat directions generic in supersymmetric theories break conformal…

High Energy Physics - Theory · Physics 2013-06-05 Yuki Watanabe , Jun'ichi Yokoyama

We propose a new mechanism to generate density perturbations in inflationary models. Spatial fluctuations in the decay rate of the inflaton field to ordinary matter lead to fluctuations in the reheating temperature. We argue that in most…

Astrophysics · Physics 2009-11-07 Gia Dvali , Andrei Gruzinov , Matias Zaldarriaga

We study reheating after the end of inflation in models where the inflaton is the superpartner of goldstino and is charged under a gauged $U(1)$ R-symmetry. We consider two classes of models -- one is small field characterized by an almost…

High Energy Physics - Theory · Physics 2021-12-10 Yermek Aldabergenov , Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono

We present a realistic supergravity inflation model which is free from the overproduction of potentially dangerous relics in cosmology, namely moduli and gravitinos which can lead to the inconsistencies with the predictions of baryon…

High Energy Physics - Phenomenology · Physics 2009-09-29 Patrick B. Greene , Kenji Kadota , Hitoshi Murayama

We present a two-field inflation model where inflaton field has a non-canonical kinetic term due to the presence of a dilaton field. It is a two-parameter generalization of one-parameter Brans-Dicke gravity in the Einstein frame. We show…

High Energy Physics - Phenomenology · Physics 2016-08-03 Girish Kumar Chakravarty , Suratna Das , Gaetano Lambiase , Subhendra Mohanty

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

We present a unified model where the same scalar field can drive inflation and account for the present dark matter abundance. This scenario is based on the incomplete decay of the inflaton field into right-handed neutrino pairs, which is…

High Energy Physics - Phenomenology · Physics 2025-02-14 Antonio Torres Manso , Joao G. Rosa

Supergravity provides the natural supersymmetric framework for early universe cosmology. A broad class of inflationary models in no-scale supergravity yields tree-level predictions for cosmic microwave background (CMB) observables that…

High Energy Physics - Phenomenology · Physics 2026-03-04 John Ellis , Tony Gherghetta , Kunio Kaneta , Wenqi Ke , Keith A. Olive

We propose a cosmological inflationary scenario based on the supergravity-embedded Standard Model supplemented by the right-handed neutrinos. We show that with an appropriate Kahler potential the L-H_u direction gives rise to successful…

High Energy Physics - Phenomenology · Physics 2013-05-30 Masato Arai , Shinsuke Kawai , Nobuchika Okada

We propose a simple model where a {\it gauge invariant inflaton} is responsible for cosmic inflation and generates the seed for structure formation, while its relic {\it thermal} abundance explains the missing matter of the universe in the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Rouzbeh Allahverdi , Bhaskar Dutta , Anupam Mazumdar

Many models of supersymmetry breaking, in the context of either supergravity or superstring theories, predict the presence of particles with weak scale masses and Planck-suppressed couplings. Typical examples are the scalar moduli and the…

High Energy Physics - Phenomenology · Physics 2009-10-31 G. F. Giudice , A. Riotto , I. Tkachev

We investigate the warm inflationary scenario within the context of the linear version of f (Q, T ) gravity, coupled with both the inflaton scalar field and the radiation field, under the conditions of the strong dissipation regime. First,…

General Relativity and Quantum Cosmology · Physics 2024-08-14 Maryam Shiravand , Mehrdad Farhoudi , Parviz Goodarzi

It has been previously shown that the linear inflation appears naturally as a solution of Coleman-Weinberg inflation, provided that the inflaton has a non-minimal coupling to gravity and the Planck scale is dynamically generated. We revisit…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-09 Antonio Racioppi

After a period of inflationary expansion, the Universe reheated and reached full thermal equilibrium at the reheating temperature. In this talk, based on the paper, arXiv:0710.3349, we point out that, in the context of effective low-energy…

High Energy Physics - Phenomenology · Physics 2009-05-01 Ki-Young Choi , Leszek Roszkowski , Roberto Ruiz de Austri

A compelling way to address the inflationary period is via the warm inflation scenario, where the interaction of the inflaton field with other degrees of freedom affects its dynamics in such a way that slow-roll inflation is maintained by…

High Energy Physics - Phenomenology · Physics 2025-04-25 Rayff de Souza , Jamerson G. Rodrigues , Clarissa Siqueira , Felipe B. M. dos Santos , Jailson Alcaniz

A novel realization of the Starobinsky inflationary model within a moderate extension of the Minimal Supersymmetric Standard Model (MSSM) is presented. The proposed superpotential is uniquely determined by applying a continuous R and a Z_2…

High Energy Physics - Phenomenology · Physics 2017-07-14 C. Pallis

Unimodular gravity is an alternative theory of gravity to general relativity. The gravitational field equations are given by the trace-free version of Einstein's field equations. Due to the structure of the theory, unimodular gravity admits…

Cosmology and Nongalactic Astrophysics · Physics 2023-07-18 M. P. Piccirilli , G. León

A new scheme for lightest supersymmetric particle (LSP) dark matter is introduced and studied in theories of TeV supersymmetry with a QCD axion, $a$, and a high reheat temperature after inflation, $T_R$. A large overproduction of axinos…

High Energy Physics - Phenomenology · Physics 2017-03-20 Raymond T. Co , Francesco D'Eramo , Lawrence J. Hall

We investigate chaotic inflation models with two scalar fields, such that one field (the inflaton) rolls while the other is trapped in a false vacuum state. The false vacuum becomes unstable when the inflaton field falls below some critical…

Astrophysics · Physics 2009-10-22 Edmund J Copeland , Andrew R Liddle , David H Lyth , Ewan D Stewart , David Wands

The theory of inflation will be investigated as well as supersymmetry breaking in the context of supergravity, incorporating the target-space duality and the nonperturbative gaugino condensation in the hidden sector. We found an…

High Energy Physics - Phenomenology · Physics 2014-11-17 Mitsuo J. Hayashi , Tomoki Watanabe , Ichiro Aizawa , Koichi Aketo
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