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Related papers: TeV Scale Leptogenesis in B-L Model with Alternati…

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Up until now the works regarding leptogenesis have discussed different mechanisms to explain the observed baryon asymmetry of the universe (BAU). The type-$II$ seesaw mechanism employing triplet scalars has been well studied in this context…

High Energy Physics - Phenomenology · Physics 2025-04-22 Rituparna Ghosh , Biswarup Mukhopadhyaya , Utpal Sarkar

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 presence of additional neutrino states with masses in the GeV range is allowed by electro-weak precision observables. However, these additional states can lead to lepton number violating interactions which potentially can wash out…

High Energy Physics - Phenomenology · Physics 2011-10-06 Sebastian Hollenberg , Heinrich Päs , Dario Schalla

The minimal Type I see-saw model cannot explain the observed neutrino masses and the baryon asymmetry of the Universe via hierarchical thermal leptogenesis without ceding naturalness. We show that this conclusion can be avoided by adding a…

High Energy Physics - Phenomenology · Physics 2015-08-26 Jackson D. Clarke , Robert Foot , Raymond R. Volkas

In the presence of anomaly induced sphaleron process, only a B-L asymmetry can be partially converted to the baryon asymmetry while any B+L asymmetry would be completely erased. Thus in any successful baryogenesis theories, B-L is usually…

High Energy Physics - Phenomenology · Physics 2008-11-26 Pei-Hong Gu , Utpal Sarkar

We study the possibility of generating non-zero reactor mixing angle $\theta_{13}$ and baryon asymmetry of the Universe within the framework of an $A_4$ flavour symmetric model. Using the conventional type I seesaw mechanism we construct…

High Energy Physics - Phenomenology · Physics 2018-06-13 Debasish Borah , Mrinal Kumar Das , Ananya Mukherjee

A typical problem of the leptogenesis scenario is the mismatch between the maximum reheat temperature implied by gravitino overproduction bound and the minimum temperature required to create thermally the lightest right-handed neutrino. We…

High Energy Physics - Phenomenology · Physics 2007-05-23 Lotfi Boubekeur

We study the consequence of a non-standard cosmological epoch in the early universe on the generation of baryon asymmetry through leptogenesis as well as dark matter abundance. We consider two different non-standard epochs: one where a…

High Energy Physics - Phenomenology · Physics 2020-04-29 Devabrat Mahanta , Debasish Borah

Realization of the inverted hierarchy is studied in the radiative neutrino mass model with an additional doublet, in which neutrino masses and dark matter could be induced from a common particle. We show that the sufficient baryon number…

High Energy Physics - Phenomenology · Physics 2015-06-12 Shoichi Kashiwase , Daijiro Suematsu

The minimal gauged U(1)$_{L_\mu-L_\tau}$ model is a simple extension of the Standard Model and has a strong predictive power for the neutrino sector. In particular, the mass spectrum and couplings of heavy right-handed neutrinos are…

High Energy Physics - Phenomenology · Physics 2020-11-25 Kento Asai , Koichi Hamaguchi , Natsumi Nagata , Shih-Yen Tseng

Thermal leptogenesis, in the framework of the standard model with three additional heavy Majorana neutrinos, provides an attractive scenario to explain the observed baryon asymmetry in the universe. It is based on the out-of-equilibrium…

High Energy Physics - Phenomenology · Physics 2020-09-30 Paul Frederik Depta , Andreas Halsch , Janine Hütig , Sebastian Mendizabal , Owe Philipsen

The observed baryon asymmetry of the Universe can be due to the $B-L$ violating decay of heavy right handed (s)neutrinos. The amount of the asymmetry depends crucially on their number density. If the (s)neutrinos are generated thermally, in…

High Energy Physics - Phenomenology · Physics 2009-11-07 Lotfi Boubekeur , Sacha Davidson , Marco Peloso , Lorenzo Sorbo

Cosmological relaxation of the electroweak scale is improved by using particle production to trap the relaxion. We combine leptogenesis with such a relaxion model that has no extremely small parameters or large e-foldings. Scanning happens…

High Energy Physics - Phenomenology · Physics 2019-05-22 Minho Son , Fang Ye , Tevong You

Our present work explores the possibility of neutrino mass generation through {\em Type-I see-saw} mechanism and provides an explanation of the baryon asymmetry of the Universe via thermal leptogenesis in the framework of $Z_3$-symmetric…

High Energy Physics - Phenomenology · Physics 2020-09-08 Indrani Chakraborty , Himadri Roy

Standard thermal leptogenesis in the type-I seesaw model requires very heavy right-handed neutrinos (RHNs). This makes it hard to probe this scenario experimentally and results in large radiative corrections to the Higgs boson mass. In this…

High Energy Physics - Phenomenology · Physics 2019-04-24 Tommi Alanne , Thomas Hugle , Moritz Platscher , Kai Schmitz

We study the model with three right-handed neutrinos which masses are smaller than the weak scale ${\cal O}(10^2)$ GeV (called as the $\nu$MSM). The model can explain the origin of neutrino masses by the seesaw mechanism, offer a candidate…

High Energy Physics - Phenomenology · Physics 2015-06-02 Takehiko Asaka , Shintaro Eijima , Kazuhiro Takeda

We study baryon asymmetry generation originated from the leptogenesis in the presence of hypermagnetic fields in the early Universe plasma before the electroweak phase transition (EWPT). For the simplest Chern-Simons (CS) wave configuration…

High Energy Physics - Phenomenology · Physics 2012-08-17 Maxim Dvornikov , Victor B. Semikoz

The conventional seesaw-leptogenesis can simultaneously explain the suppression of neutrino masses and the generation of cosmic baryon asymmetry, but usually cannot predict an unambiguous relation between these two sectors. In this work we…

High Energy Physics - Phenomenology · Physics 2016-10-12 Pei-Hong Gu , Xiao-Gang He

In this work, we classify all the effective $U(1)$ symmetries and their associated Noether charges in the Standard Model (SM) and its minimal supersymmetric extension (MSSM) from the highest scale after inflation down to the weak scale. We…

High Energy Physics - Phenomenology · Physics 2021-08-26 Chee Sheng Fong

With the consideration of a fast expanding Universe in effect due to an additional scalar field, we present a study of leptogenesis in non-standard cosmology. The Hubble expansion rate is modified by the new added scalar field $\varphi$,…

High Energy Physics - Phenomenology · Physics 2020-03-18 Shao-Long Chen , Amit Dutta Banik , Ze-Kun Liu
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