Narendra, Nimmala and Sahu, Narendra and Shilb, Sujay
(2019)
Asymmetric Dark Matter From Triplet Scalar Leptogenesis.
arXiv.org.
Full text not available from this repository.
Abstract
In this article we extend the standard model with a SU(2) singlet leptonic
Dirac fermion χ, which represents the candidate of dark matter, and a triplet scalar ∆. In
the early Universe, the CP violating out of equilibrium decay of ∆ generates a net B − L
asymmetry in the SM sector, where B and L represents the total baryon and lepton number
respectively. A part of this asymmetry gets transferred to the dark sector through a higher
dimensional operator which conserve B − L, while the B + L violating sphalerons keeps
converting B − L asymmetry to the observed B asymmetry. In addition, we introduce
a singlet scalar field φ which mixes with the SM-Higgs to give a resonance channel to
annihilate the symmetric component of DM and also gives direct detection signal. In our
model, the active neutrinos get small masses by the induced vacuum expectation value
(vev) of the triplet scalar ∆. In the later part of the paper we discuss all the constraints
coming from invisible Higgs decay, Higgs signal strength, DM direct detection and relic
density of DM.
[error in script]
IITH Creators: |
IITH Creators | ORCiD |
---|
Sahu, Narendra | UNSPECIFIED |
|
Item Type: |
Article
|
Uncontrolled Keywords: |
Seesaw Models, Leptogenesis, Asymmetric dark matter, Beyond Standard, Model Physics |
Subjects: |
Physics |
Divisions: |
Department of Physics |
Depositing User: |
Team Library
|
Date Deposited: |
11 Nov 2019 04:59 |
Last Modified: |
11 Nov 2019 04:59 |
URI: |
http://raiithold.iith.ac.in/id/eprint/6937 |
Publisher URL: |
|
Related URLs: |
|
Actions (login required)
|
View Item |