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We argue that in the simplest version of the KKLT model, the maximal value of the Hubble constant during inflation cannot exceed the present value of the gravitino mass, H< m_{3/2}. This may have important implications for string cosmology…

高能物理 - 理论 · 物理学 2010-04-06 Renata Kallosh , Andrei Linde

We reconsider an inflationary model that inflaton field is non-minimally coupled to gravity. We study parameter space of the model up to the second ( and in some cases third ) order of the slow-roll parameters. We calculate inflation…

广义相对论与量子宇宙学 · 物理学 2014-11-21 Kourosh Nozari , S. Shafizadeh

We explore a model of two-field inflation with nonminimal kinetic terms in which two identical matter sectors decoupled from each other may reheat to different temperatures while preserving the symmetry of the Lagrangian. This scenario is…

宇宙学与河外天体物理 · 物理学 2022-02-16 James M. Cline , Jean-Samuel Roux

We explore a new class of supersymmetric models of inflation where the inflaton is realised as a combination of a Higgs field and (gauge non-singlet) matter fields, using a "tribrid" structure of the superpotential. Inflation is associated…

高能物理 - 唯象学 · 物理学 2015-03-20 Stefan Antusch , David Nolde , Mansoor Ur Rehman

Supersymmetric Unified theories which incorporate a renormalizable Type I seesaw mechanism for small neutrino masses can also provide slow roll inflection point inflation along a flat direction associated with a gauge invariant combination…

高能物理 - 唯象学 · 物理学 2012-09-21 Charanjit S. Aulakh , Ila Garg

We discuss the phenomenology of the minimal inflation scenario. We concentrate on two aspects: inflationary trajectories and particle production. Our findings can be summarized in two main results: first, that inflationary trayectories that…

宇宙学与河外天体物理 · 物理学 2015-05-30 Luis Alvarez-Gaume , Cesar Gomez , Raul Jimenez

Long standing themes in inflation include the issue of large field vs. small field inflation as well as the question what fraction of phase space leads to sufficient inflation, and furthermore is compatible with the experimental data. In…

高能物理 - 理论 · 物理学 2022-04-13 Rolf Schimmrigk

Cosmological inflation gives a natural answer for a variety of cosmological questions, including the horizon problem, the flatness problem, and others. However, inflation yields new questions relating to the flatness of the inflaton…

高能物理 - 唯象学 · 物理学 2009-11-10 David E. Kaplan , Neal Weiner

We study classes of inflation models driven by antisymmetric tensor field, with minimal and nonminimal couplings to gravity, that address known issues of such models considered in the past. First we show that with a different choice of the…

广义相对论与量子宇宙学 · 物理学 2022-04-25 Sandeep Aashish , Abhijith Ajith , Sukanta Panda , Rahul Thakur

We propose a simple but effective mechanism to realize an inflationary early universe consistent with the observed WMAP, Planck and/or BICEP2 data, which would be incorporated in various supersymmetric models of elementary particles…

高能物理 - 理论 · 物理学 2015-06-19 Hiroyuki Abe , Hajime Otsuka

It is well known that in manifestly Lorentz invariant theories with nontrivial kinetic terms, perturbations around some classical backgrounds can travel faster than light. These exotic "supersonic" models may have interesting consequences…

天体物理学 · 物理学 2009-09-29 Alexander Vikman

We introduce a new class of models of chaotic inflation inspired by the superconformal approach to supergravity. This class of models allows a functional freedom of choice of the inflaton potential V = |f(\phi)|^2. The simplest model of…

高能物理 - 理论 · 物理学 2010-11-22 Renata Kallosh , Andrei Linde

One common approach for cosmic inflation consists in couple Einstein's gravity with a scalar field, often referred to inflaton field. In order to derive analytic simple scenarios, we usually work in the {\it slow-roll} regime. In such an…

广义相对论与量子宇宙学 · 物理学 2021-01-01 J. R. L. Santos , P. H. R. S. Moraes

We study cosmological gravitational particle production as applied to "rapid-turn" models of inflation involving two scalar fields. We are interested in the production of massive spin-0 particles that only interact gravitationally and…

高能物理 - 理论 · 物理学 2023-06-08 Edward W. Kolb , Andrew J. Long , Evan McDonough , Guillaume Payeur

We present the supersymmetric extension of the unified model for inflation and Dark Matter studied in Ref. arXiv:1811.02302. The scenario is based on the incomplete decay of the inflaton field into right-handed (s)neutrino pairs. By…

高能物理 - 唯象学 · 物理学 2025-02-14 Mar Bastero-Gil , António Torres Manso

The smallness of the neutrino masses may be related to inflation. The minimal supersymmetric Standard Model (MSSM) with small Dirac neutrino masses already has all the necessary ingredients for a successful inflation. In this model the…

高能物理 - 唯象学 · 物理学 2010-10-27 Rouzbeh Allahverdi , Alexander Kusenko , Anupam Mazumdar

We study preheating in theories where the inflaton couples derivatively to scalar and gauge fields. Such couplings may dominate in natural models of inflation, in which the flatness of the inflaton potential is related to an approximate…

高能物理 - 唯象学 · 物理学 2008-11-26 Cristian Armendariz-Picon , Mark Trodden , Eric J. West

We consider low scale slow roll inflation driven by the gauge invariant flat directions {\bf udd} and {\bf LLe} of the Minimally Supersymmetric Standard Model at the vicinity of a saddle point of the scalar potential. We study the stability…

高能物理 - 唯象学 · 物理学 2010-10-27 Rouzbeh Allahverdi , Kari Enqvist , Juan Garcia-Bellido , Asko Jokinen , Anupam Mazumdar

We discuss the hybrid inflation model where the inflaton field is nonminimally coupled to gravity. In the Jordan frame, the potential contains $\phi^4$ term as well as terms in the original hybrid inflation model. In our model, inflation…

高能物理 - 理论 · 物理学 2011-02-22 Seoktae Koh , Masato Minamitsuji

A supergravity extension of the $(R+R^2)$ gravity with the additional (Born-Infeld) structure of a massive vector multiplet gives rise to the specific $F(R)$ gravity, whose structure is investigated in detail. The massive vector multiplet…

高能物理 - 理论 · 物理学 2018-10-17 Yermek Aldabergenov , Ryotaro Ishikawa , Sergei V. Ketov , Sergey I. Kruglov
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