scholarly journals Neutrino phenomenology and scalar Dark Matter with A 4 flavor symmetry in Inverse and type II seesaw

2016 ◽  
Vol 913 ◽  
pp. 643-663 ◽  
Author(s):  
Ananya Mukherjee ◽  
Mrinal Kumar Das
Keyword(s):  
Dark Matter ◽  
Flavor Symmetry ◽  
Type Ii

scholarly journals Exothermic dark mesons in light of electron recoil excess at XENON1T

2021 ◽  
Vol 2021 (4) ◽  
Author(s):  
Soo-Min Choi ◽  
Hyun Min Lee ◽  
Bin Zhu
Keyword(s):  
Dark Matter ◽  
Inelastic Scattering ◽  
Small Mass ◽  
Density Current ◽  
Flavor Symmetry ◽  
Color Group ◽  
Dark Sector ◽  
The Standard Model ◽  
Electron Recoil ◽  
Relic Density

Abstract We consider a novel mechanism to realize exothermic dark matter with dark mesons in the limit of approximate flavor symmetry in a dark QCD. We introduce a local dark U(1)′ symmetry to communicate between dark mesons and the Standard Model via Z′ portal by partially gauging the dark flavor symmetry with flavor-dependent charges for cancelling chiral anomalies in the dark sector. After the dark local U(1)′ is broken spontaneously by the VEV of a dark Higgs, there appear small mass splittings between dark quarks, consequently, leading to small split masses for dark mesons, required to explain the electron recoil excess in XENON1T by the inelastic scattering between dark mesons and electron. We propose a concrete benchmark model for split dark mesons based on SU(3)L× SU(3)R/SU(3)V flavor symmetry and SU(Nc) color group and show that there exists a parameter space making a better fit to the XENON1T data with two correlated peaks from exothermic processes and satisfying the correct relic density, current experimental and theoretical constraints.

scholarly journals Dark matter candidates in a type-II radiative neutrino mass model

2021 ◽  
Vol 2021 (6) ◽  
Author(s):  
Roberto A. Lineros ◽  
Mathias Pierre
Keyword(s):  
Dark Matter ◽  
Neutral Particle ◽  
Matter Density ◽  
Indirect Detection ◽  
Dark Matter Candidate ◽  
Neutrino Masses ◽  
Type Ii ◽  
Mass Model ◽  
Direct And Indirect Detection

Abstract We explore the connection between Dark Matter and neutrinos in a model inspired by radiative Type-II seessaw and scotogenic scenarios. In our model, we introduce new electroweakly charged states (scalars and a vector-like fermion) and impose a discrete ℤ2 symmetry. Neutrino masses are generated at the loop level and the lightest ℤ2-odd neutral particle is stable and it can play the role of a Dark Matter candidate. We perform a numerical analysis of the model showing that neutrino masses and flavour structure can be reproduced in addition to the correct dark matter density, with viable DM masses from 700 GeV to 30 TeV. We explore direct and indirect detection signatures and show interesting detection prospects by CTA, Darwin and KM3Net and highlight the complementarity between these observables.

scholarly journals Dark matter interactions in an S4×Z5 flavor symmetry framework

2020 ◽  
Vol 102 (11) ◽  
Author(s):  
Giorgio Arcadi ◽  
Martin B. Krauss ◽  
Davide Meloni
Keyword(s):  
Dark Matter ◽  
Flavor Symmetry

scholarly journals Type-II seesaws at colliders, lepton asymmetry and singlet scalar dark matter

2008 ◽  
Vol 2008 (04) ◽  
pp. 037 ◽  
Author(s):  
John McDonald ◽  
Narendra Sahu ◽  
Utpal Sarkar
Keyword(s):  
Dark Matter ◽  
Type Ii ◽  
Lepton Asymmetry

scholarly journals Light scalar dark matter extension of the type-II two-Higgs-doublet model

2018 ◽  
Vol 98 (3) ◽  
Author(s):  
Lei Wang ◽  
Rongle Shi ◽  
Xiao-Fang Han ◽  
Bin Zhu
Keyword(s):  
Dark Matter ◽  
Higgs Doublet ◽  
Type Ii ◽  
Light Scalar ◽  
Doublet Model ◽  
Two Higgs Doublet Model

scholarly journals Dark matter from binary tetrahedral flavor symmetry

2012 ◽  
Vol 713 (3) ◽  
pp. 249-254 ◽  
Author(s):  
David A. Eby ◽  
Paul H. Frampton
Keyword(s):  
Dark Matter ◽  
Flavor Symmetry

INVESTIGATIONS OF THE FLAVOR SYMMETRY, RADIATIVE SEESAW MODEL AND COLD DARK MATTER

2007 ◽  
Vol 16 (05) ◽  
pp. 1541-1556
Author(s):  
HIROSHI OKADA
Keyword(s):  
Dark Matter ◽  
Cold Dark Matter ◽  
Vacuum Expectation ◽  
The Other ◽  
Type Model ◽  
Flavor Symmetry ◽  
Heavy Particles ◽  
Neutrino Sector ◽  
Seesaw Model ◽  
The Masses

It is now clear that the masses of the neutrino sector are much lighter than those of the other three sectors. Canonial seesaw model would be the most famous for the above explanation. But one must introduce heavy particles that will not be able to observed with present scientific technologies. On the other hand, there are many attempts to explain the neutrino masses radiatively by means of inert Higgses, which do not have the vacuum expectation values. Then one can discuss cold dark matter candidates, because of no needing so heavy particles. The most famous work would be the Zee model17. Recently a new type model (hep-ph/0601225)4 along this line of thought was proposed by E. Ma. We adopted this idea, and then we introduced a new flavor symmetry to constrain the Yukawa sector. So our model might be more predictive, and can be investigated at LHC. I will present how we can obserb the particular signal at LHC, and what we can predict about the neutrino sector.

scholarly journals CP violation from flavor symmetry in a lepton quarticity dark matter model

2016 ◽  
Vol 761 ◽  
pp. 431-436 ◽  
Author(s):  
Salvador Centelles Chuliá ◽  
Rahul Srivastava ◽  
José W.F. Valle
Keyword(s):  
Dark Matter ◽  
Cp Violation ◽  
Flavor Symmetry ◽  
Matter Model ◽  
Dark Matter Model
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