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Related papers: Supersymmetric Majoron Inflation

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Inflation with plateau potentials give the best fit to the CMB observables as they predict tensor to scalar ratio stringently bounded by the observations from Planck and BICEP2/Keck. In supergravity models it is possible to obtain plateau…

High Energy Physics - Phenomenology · Physics 2016-11-09 Girish Kumar Chakravarty , Ujjal Kumar Dey , Gaetano Lambiase , Subhendra Mohanty

We have realized non-minimal Higgs inflation and standard hybrid inflation in the supersymmetric flipped $SU(5)$ model with $U(1)_R$ symmetry using the no-scale form of the K\"{a}hler potential. In non-minimal Higgs inflation the waterfall…

High Energy Physics - Phenomenology · Physics 2021-10-12 Mian Muhammad Azeem Abid , Maria Mehmood , Mansoor Ur Rehman , Qaisar Shafi

We explore the possibility of obtaining inflation in weakly coupled heterotic string theory, where the model dependent axions are responsible for driving inflation. This model can be considered as a certain extrapolation of…

High Energy Physics - Theory · Physics 2010-10-27 Martin E. Olsson

The scale at which supersymmetry is broken and the mechanism by which supersymmetry breaking is fed down to the observable sector has rich implications on the way Nature may have chosen to accomplish inflation. We discuss a simple model for…

High Energy Physics - Phenomenology · Physics 2014-11-17 Antonio Riotto

We show that if global lepton number symmetry is spontaneously broken in a post inflation epoch, then it can lead to the formation of cosmological domain walls. This happens in the well-known "Majoron paradigm" for neutrino mass generation.…

High Energy Physics - Phenomenology · Physics 2019-04-17 George Lazarides , Mario Reig , Qaisar Shafi , Rahul Srivastava , José W. F. Valle

The minimal supersymmetric standard model, when extended to embed the seesaw mechanism, obtains two dimensionful parameters in its superpotential: the mu parameter and the right-handed neutrino mass M_N. These mass parameters, belonging to…

High Energy Physics - Phenomenology · Physics 2009-11-11 D. Demir , Y. Farzan

Natural (axionic) inflation provides a well-motivated and predictive scheme for the description of the early universe. It leads to sizeable primordial tensor modes and thus a high mass scale of the inflationary potential. Naively this seems…

High Energy Physics - Theory · Physics 2015-05-20 Rolf Kappl , Hans Peter Nilles , Martin Wolfgang Winkler

We investigate an inflation model with the inflaton being identified with a Higgs boson responsible for the breaking of U(1)B-L symmetry. We show that supersymmetry must remain a good symmetry at scales one order of magnitude below the…

High Energy Physics - Phenomenology · Physics 2012-03-13 Kazunori Nakayama , Fuminobu Takahashi

Supersymmetric compactification with moderately large radius (${\rm Re}< T > \sim {\cal O}(10)$ or more) not only accommodates supersymmetric unification, but also provides candidates for an inflaton in the form of geometric moduli; the…

High Energy Physics - Theory · Physics 2014-10-29 Hirotaka Hayashi , Ryo Matsuda , Taizan Watari

We propose a scenario for realizing inflation in the framework of supersymmetric B-L extension of the Standard Model. We find that one of the associated right-handed sneutrinos (the superpartner of the Standard Model singlet fermion) can…

High Energy Physics - Phenomenology · Physics 2013-05-29 Shaaban Khalil , Arunansu Sil

We present a mechanism for realizing hybrid inflation using two axion fields with a purely non-perturbatively generated scalar potential. The structure of scalar potential is highly constrained by the discrete shift symmetries of the…

High Energy Physics - Theory · Physics 2021-04-28 Federico Carta , Nicole Righi , Yvette Welling , Alexander Westphal

We investigate thermal leptogenesis in a supersymmetric neutrinophilic Higgs model by taking phenomenological constraints into account, where, in addition to the minimal supersymmetric standard model, we introduce an extra Higgs field with…

High Energy Physics - Phenomenology · Physics 2015-05-28 Naoyuki Haba , Osamu Seto

We show that the scalar field that drives inflation can have a dynamical origin, being a strongly coupled right handed neutrino condensate. The resulting model is phenomenologically tightly constrained, and can be experimentally (dis)probed…

High Energy Physics - Phenomenology · Physics 2009-03-31 Gabriela Barenboim

In the left-right symmetric models without bi-doublet Higgs scalars, the standard model fermions can obtain masses by integrating out heavy charged singlet fermions. We find the decays of heavy neutral singlet fermions, responsible for…

High Energy Physics - Phenomenology · Physics 2010-05-19 Pei-Hong Gu

The gravitino problem gives a severe constraint on the thermal leptogenesis scenario. This problem leads us to consider some alternatives to it if we try to keep the gravitino mass around the weak scale $m_{3/2} \sim 100$ GeV. We consider,…

High Energy Physics - Phenomenology · Physics 2009-11-11 Takeshi Fukuyama , Tatsuru Kikuchi , Toshiyuki Osaka

In this talk we present a mechanism for leptogenesis which is based on gravity waves produced during inflation. We show that when inflation is driven by a pseudo-scalar field the metric perturbations generated during inflation can become…

High Energy Physics - Phenomenology · Physics 2014-03-18 S. H. Alexander , M. Peskin , M. M. Sheikh-Jabbari

We analyze the cosmological implications of F-term hybrid inflation with a subdominant Fayet--Iliopoulos D-term whose presence explicitly breaks a D-parity in the inflaton-waterfall sector. This scenario of inflation, which is called…

High Energy Physics - Phenomenology · Physics 2009-11-11 Bjorn Garbrecht , Constantinos Pallis , Apostolos Pilaftsis

The generation of helical magnetic fields and the associated chiral asymmetry via the chiral anomaly is a generic feature in pseudoscalar inflation. In the presence of a Chern--Simons coupling between the inflaton and a U(1) gauge field,…

High Energy Physics - Phenomenology · Physics 2025-12-25 Di Wu , Yifan Hu , Kohei Kamada

We consider inflation driven by an axion-like particle coupled to an SU(2) gauge sector via a Chern-Simons term. Known as chromo-natural inflation, this scenario is in tension with CMB observations. In order to remedy this fact and preserve…

Cosmology and Nongalactic Astrophysics · Physics 2023-03-21 Ema Dimastrogiovanni , Matteo Fasiello , Martino Michelotti , Lucas Pinol

We propose a novel mechanism for significantly enhancing the amplitude of primordial electromagnetic fields during inflation. Similar to existing proposals, our idea is based on parametric resonance effects due to…

Cosmology and Nongalactic Astrophysics · Physics 2023-05-03 Misao Sasaki , Valeri Vardanyan , Vicharit Yingcharoenrat
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