from 29 November 2022 to 2 December 2022
Hotel Intourist Kolomenskoye 4*
Europe/Moscow timezone
The conference is over! Thank you for participation!

Flavoured leptogenesis in a minimal type-I+II seesaw mechanism

2 Dec 2022, 19:20
15m
Petrovskiy 2 (Hotel Intourist Kolomenskoye 4*)

Petrovskiy 2

Hotel Intourist Kolomenskoye 4*

Oral talk Neutrino physics Neutrino Physics

Speaker

Ms. Sreerupa Chongdar (PhD Scholar, Department of Physics and Astronomy, National Institute of Technology Rourkela)

Description

The seesaw mechanism is a popular approach to give a viable explanation for the source of non-zero neutrino mass and for the cause of matter dominance of the Universe - two of the most important open problems that could not be answered in the Standard Model (SM) of Particle Physics. A minimal extension of the SM is studied, incorporating a type-I+II seesaw mechanism with only one right-handed neutrino and one Higgs triplet scalar. These heavy particles contribute to the generation of tiny neutrino mass, which is inversely proportional to the corresponding heavy particle masses. Considering that leptogenesis is achieved by the decay of the right-handed neutrino, the new source of CP asymmetry comes solely from the decay of the right-handed neutrino by one-loop vertex correction involving the Higgs triplet scalar. The model's predictability enhances by introducing Fritzsch type 2-zero and 3-zero textures for the neutrino mass matrix and the non-diagonal charged lepton mass matrix, respectively. We execute the parameter space study following the latest neutrino oscillation parameter data, and the phenomenological importance of this hybrid texture is analyzed. We study leptogenesis in the two-flavoured and three-flavoured regimes, and we observe that the leptogenesis in different flavoured regimes, within the temperature range $T\subset[10^{10},10^{11}]$ GeV, can efficiently predict baryon asymmetry of the Universe within experimentally obtained range.

Primary authors

Ms. Sreerupa Chongdar (PhD Scholar, Department of Physics and Astronomy, National Institute of Technology Rourkela) Dr. Sasmita Mishra (Assistant Professor Grade-I, Department of Physics and Astronomy, National Institute of Technology Rourkela)

Presentation Materials

There are no materials yet.
Your browser is out of date!

Update your browser to view this website correctly. Update my browser now

×