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Related papers: Sneutrino Inflation

200 papers

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…

High Energy Physics - Phenomenology · Physics 2012-09-21 Charanjit S. Aulakh , Ila Garg

We present the possibility that the seesaw mechanism with thermal leptogenesis can be tested using the stochastic gravitational background. Achieving neutrino masses consistent with atmospheric and solar neutrino data, while avoiding…

High Energy Physics - Phenomenology · Physics 2020-03-11 Jeff A. Dror , Takashi Hiramatsu , Kazunori Kohri , Hitoshi Murayama , Graham White

The nature of dark matter (DM) particles and the mechanism that provides their measured relic abundance are currently unknown. Likewise, the nature of the inflaton is unknown as well. We investigate the triplet seesaw model in an unified…

High Energy Physics - Phenomenology · Physics 2012-09-07 Chiara Arina

We have discussed in detail how neutrinos produced from inflaton solely through gravitational interaction can successfully reheat the universe. For this, we have introduced the well-known Type-I seesaw neutrino model. Depending on seesaw…

High Energy Physics - Phenomenology · Physics 2025-04-01 Md Riajul Haque , Debaprasad Maity , Rajesh Mondal

We consider supersymmetric models in which the right-handed sneutrino is a viable WIMP dark matter candidate. These are either simple extensions of the Minimal Supersymmetric Standard Model or models with the addition of an extra U(1)…

High Energy Physics - Phenomenology · Physics 2012-09-10 Valentina De Romeri

We present a complete particle physics model that explains three major problems of modern cosmology: inflation, dark matter and dark energy, and also gives a mechanism for leptogenesis. The model has a new gauge group $SU(2)_Z$ that grows…

Astrophysics · Physics 2008-11-26 P. Q. Hung , Eduard Masso , Gabriel Zsembinszki

In this work, we interpret the 3-3-1-1 model when the B-L and 3-3-1 breaking scales behave simultaneously as the inflation scale. This setup not only realizes the previously-achieved consequences of inflation and leptogenesis, but also…

High Energy Physics - Phenomenology · Physics 2017-04-04 D. T. Huong , P. V. Dong

The lepton flavour violating charged lepton decays mu to e + gamma and thermal leptogenesis are analysed in the minimal supersymmetric standard model with see-saw mechanism of neutrino mass generation and soft supersymmetry breaking terms…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. T. Petcov , T. Shindou

An epoch of accelerated expansion, or inflation, in the early universe solves several cosmological problems. While there are many models of inflation only recently has it become possible to discriminate between some of the models using…

High Energy Physics - Phenomenology · Physics 2007-06-29 Raghavan Rangarajan

We propose that the observed baryon asymmetry of the Universe can naturally arise from a net asymmetry generated in the sleptonic sector at fairly low reheat temperatures. The best candidate is indeed the right-handed sneutrino. The initial…

High Energy Physics - Phenomenology · Physics 2009-11-10 Rouzbeh Allahverdi , Bhaskar Dutta , Anupam mazumdar

The historical discovery of neutrino oscillations using solar and atmospheric neutrinos, and subsequent accelerator and reactor studies, has brought neutrino physics to the precision era. We note that CP effects in oscillation phenomena…

High Energy Physics - Phenomenology · Physics 2016-06-22 O. G. Miranda , J. W. F. Valle

Models with low-scale breaking of global symmetries in the neutrino sector provide an alternative to the seesaw mechanism for understanding why neutrinos are light. Such models can easily incorporate light sterile neutrinos required by the…

High Energy Physics - Phenomenology · Physics 2010-12-09 Z. Chacko , Lawrence J. Hall , Steven J. Oliver , Maxim Perelstein

We show that three open questions in particle physics and cosmology: the origin of neutrino mass, the identity of dark matter, and the origin of the baryon asymmetry of the universe can be explained simultaneously in the three-loop seesaw…

High Energy Physics - Phenomenology · Physics 2023-09-08 Osamu Seto , Tetsuo Shindou , Takanao Tsuyuki

A model of nonlinear electrodynamics with a dimensional parameter $\beta$ is considered. Electromagnetic fields are the source of the gravitation field and inflation of the universe. We imply that the universe is filled by stochastic…

General Relativity and Quantum Cosmology · Physics 2017-05-08 S. I. Kruglov

After a brief discussion of baryon and lepton number nonconservation, we review the status of thermal leptogenesis with GUT scale neutrino masses, as well as low scale alternatives with keV neutrinos as dark matter and heavy neutrino masses…

High Energy Physics - Phenomenology · Physics 2015-06-11 Wilfried Buchmuller

By combining the simplest (3,1) version of the seesaw mechanism containing a single heavy "right-handed" neutrino with the minimal scotogenic approach to dark matter, we propose a theory for neutrino oscillations. The "atmospheric" mass…

High Energy Physics - Phenomenology · Physics 2018-12-19 Nicolás Rojas , Rahul Srivastava , José W. F. Valle

We present a successful realization of sneutrino tribrid inflation model based on a gauged $U(1)_{B-L}$ extension of Minimal Supersymmetric Standard Model (MSSM). A single interaction term involving the $B-L$ Higgs field and the…

High Energy Physics - Phenomenology · Physics 2021-11-18 Muhammad Atif Masoud , Mansoor Ur Rehman , Qaisar Shafi

We discuss sneutrino inflation in the brane-world scenario. We work in the Randall-Sundrum type II brane-world, generalized with the introduction of the Gauss-Bonnet term, a correction to the effective action in string theories. We find…

High Energy Physics - Phenomenology · Physics 2009-11-11 G. Panotopoulos

A rapid phase of accelerated expansion in the early universe, known as inflation, dilutes all matter except the vacuum induced quantum fluctuations. These are responsible for seeding the initial perturbations in the baryonic matter, the…

High Energy Physics - Phenomenology · Physics 2011-06-28 Anupam Mazumdar

We use modular symmetry as an organizing principle that attempts to simultaneously address the lepton flavor puzzle, inflation, and post-inflationary reheating. We demonstrate this approach using the finite modular group $A_4$ in the lepton…

High Energy Physics - Phenomenology · Physics 2025-11-05 Gui-Jun Ding , Si-Yi Jiang , Yong Xu , Wenbin Zhao