19–23 Dec 2024
Swatantrata Bhavan, Banaras Hindu University, Varanasi
Asia/Kolkata timezone

Addressing dark matter in minimal extended seesaw framework

Not scheduled
20m
Swatantrata Bhavan, Banaras Hindu University, Varanasi

Swatantrata Bhavan, Banaras Hindu University, Varanasi

Department of Physics, I.Sc., Banaras Hindu University, 221005 Varanasi, India
Postar Neutrino Physics

Speaker

Nayana Gautam

Description

Different models have been proposed to resolve the puzzling mystery of dark matter. We study a feasible dark matter candidate in the framework of minimal extended seesaw (MES) [1]. The model is augmented with ∆(96) symmetry that leads to $TM_1$ mixing pattern. A sterile state in intermediate mass range has been added to the standard model to realize the framework [2]. The structure of the mass matrices are obtained from ∆(96) symmetry[3]. We find that sterile neutrino mass in keV range can have significant contribution to the dark matter content of the Universe [4]. The viability of the proposed model is tested considering the allowed cosmological ranges of the relic abundance, decay rates as well as its mixing with the active neutrinos.

References:
1. M. Drewes et al., A white paper on keV sterile neutrino dark matter, JCAP 01 (2017) 025.
2. Zhang H. Light Sterile Neutrino in the Minimal Extended Seesaw. Phys Lett B (2012) 714:262
3. Abada. A., Arcadi. G. and Lucente. M., Dark matter in the minimal inverse seesaw mechanism, JCAP 10 (2014) 001.
4. Gautam N. , Krishnan R., and Das M.K., “Effect of Sterile Neutrino on Low-Energy Processes in Minimal Extended Seesaw With Δ(96) Symmetry and TM1 Mixing”, Front. In Phys.0 (2021)417.

Field of contribution Phenomenology

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