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Related papers: Hilltop Supernatural Inflation and Gravitino Probl…

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We study a leptogenesis scenario in which the heavy Majorana neutrinos are produced non-thermally in inflaton decays in the supersymmetric economical SU(3)_C X SU(3)_L X U(1)_X model with inflationary scenario, and for this purpose neutrino…

High Energy Physics - Phenomenology · Physics 2010-12-17 D. T. Huong , H. N. Long

We study the consequences of reheating in quintessential inflation. From simple inflationary quintessential models introduced in cite{hap, hap2}, we show that when the reheating is due to the production of heavy massive particles…

General Relativity and Quantum Cosmology · Physics 2017-06-06 Jaume de Haro , Llibert Aresté Saló

We review the main aspects of the warm inflation scenario, focusing on the inflationary dynamics and the predictions related to the primordial spectrum of perturbations, to be compared with the recent cosmological observations. We study in…

High Energy Physics - Phenomenology · Physics 2010-04-21 Mar Bastero-Gil , Arjun Berera

Particle production from vacuum fluctuations during inflation is briefly revisited. The moduli problem occurring with light particles produced at the end of inflation is addressed, namely the fact that some results are in disagreement with…

General Relativity and Quantum Cosmology · Physics 2015-06-03 Jaume de Haro , Emilio Elizalde

We analyse the shifted hybrid inflation in a no-scale SU(5) model with supersymmetry, which naturally circumvents the monopole problem. The no-scale framework is derivable as the effective field theory of the supersymmetric (SUSY)…

High Energy Physics - Phenomenology · Physics 2023-05-12 Waqas Ahmed , Muhammad Moosa , Shoaib Munir , Umer Zubair

We implement a procedure by which the parameters present in the potential of Quartic Hilltop Inflation (QHI) are eliminated in favor of the scalar spectral index $n_s$ and the tensor-to-scalar ratio $r$. By doing this it is posible to…

Cosmology and Nongalactic Astrophysics · Physics 2021-03-03 Gabriel German

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

The temperature fluctuations in the cosmic microwave background observed by COBE provide strong support for an inflationary phase in the early universe, below the GUT scale. We argue that a singlet field in a hidden sector of an effective…

High Energy Physics - Phenomenology · Physics 2007-05-23 Subir Sarkar

We discuss two cosmological issues in a generic gauge-mediated supersymmetry (SUSY)-breaking model, namely the Universe's baryon asymmetry and the gravitino dark-matter density. We show that both problems can be simultaneously solved if…

High Energy Physics - Phenomenology · Physics 2009-11-07 Masaaki Fujii , T. Yanagida

We analyse non-thermal leptogenesis after models of Majoron hilltop inflation, where the scalar field that provides masses for the right-handed neutrinos and sneutrinos via its vacuum expectation value acts as the inflaton. We discuss…

High Energy Physics - Phenomenology · Physics 2018-05-16 Stefan Antusch , Kenneth Marschall

We discuss leptogenesis in a realistic supersymmetric model of inflation with a low reheat temperature 1-10 GeV. The lepton asymmetry is generated by a decaying right handed sneutrino, which is produced after inflation during preheating.…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Bastero-Gil , S. F. King

We investigate for viable models of inflation that can successfully produce dark matter (DM) from inflaton decay process, satisfying all the constraints from Cosmic Microwave Background (CMB) and from some other observations. In particular,…

High Energy Physics - Phenomenology · Physics 2022-10-19 Anish Ghoshal , Gaetano Lambiase , Supratik Pal , Arnab Paul , Shiladitya Porey

We present a minimal UV complete framework to embed inflation and dark matter by extending the standard model with a singlet real scalar field (the inflaton) and a singlet fermonic field acting as dark matter. The inflaton features the most…

High Energy Physics - Phenomenology · Physics 2022-07-27 Nicolás Bernal , Yong Xu

The production and the final abundance of gravitino dark matter appear to depend crucially on the restoration of the global U(1) $R$-symmetry of GMSB sectors in a threefold way. An $R$-symmetric phase effectively suppresses the production…

High Energy Physics - Phenomenology · Physics 2015-06-15 Iannis Dalianis

Supernatural inflation is an attractive model based just on a flat direction with soft SUSY breaking mass terms in the framework of supersymmetry. The beauty of the model is inferred from its name that the model needs no fine-tuning.…

High Energy Physics - Phenomenology · Physics 2013-05-29 Chia-Min Lin , Kingman Cheung

We review work on the formation of gravitino condensates via the super-Higgs effect in the early Universe. This is a scenario for both inflating the early universe and breaking local supersymmetry (supergravity), entirely independent of any…

General Relativity and Quantum Cosmology · Physics 2014-12-23 Nick E. Mavromatos

We argue that a non-thermal leptogenesis occurs spontaneously, without direct couplings of the inflaton with right-handed neutrinos, in a wide class of high-scale inflation models such as the chaotic and hybrid inflation. It is only a…

High Energy Physics - Phenomenology · Physics 2008-11-26 Motoi Endo , Fuminobu Takahashi , T. T. Yanagida

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 identify a new mechanism in supergravity theories which leads to successful inflation without any need for fine tuning. The simplest model yields a spectrum of density fluctuations tilted away from scale-invariance and negligible…

High Energy Physics - Phenomenology · Physics 2014-11-17 Jennifer A. Adams , Graham G. Ross , Subir Sarkar

In this paper, we consider a model of quintessential inflation based upon inverse hyperbolic potential. We employ curvaton mechanism for reheating which is more efficient than gravitational particle production; the mechanism complies with…

General Relativity and Quantum Cosmology · Physics 2018-07-25 Abhineet Agarwal , Sabit Bekov , Kairat Myrzakulov