Chiral gauge theories and a dirac neutrino - Dark matter connection

2016 ◽  
Author(s):  
Daniel Hernandez
Keyword(s):  
Dark Matter ◽  
Gauge Theories ◽  
Dirac Neutrino

scholarly journals Dynamical framework for KeV Dirac neutrino warm dark matter

2014 ◽  
Vol 90 (4) ◽  
Author(s):  
Dean J. Robinson ◽  
Yuhsin Tsai
Keyword(s):  
Dark Matter ◽  
Dirac Neutrino

scholarly journals Light Dirac neutrino portal dark matter with observable ΔN eff

2021 ◽  
Vol 2021 (10) ◽  
pp. 002
Author(s):  
Anirban Biswas ◽  
Debasish Borah ◽  
Dibyendu Nanda
Keyword(s):  
Dark Matter ◽  
Dirac Neutrino

scholarly journals Scotogenic cobimaximal Dirac neutrino mixing from $$\Delta (27)$$ and $$U(1)_\chi $$

2019 ◽  
Vol 79 (11) ◽  
Author(s):  
Ernest Ma
Keyword(s):  
Dark Matter ◽  
Lepton Number ◽  
Neutrino Masses ◽  
Neutrino Mixing ◽  
Dirac Neutrino

Abstract In the context of $$SU(3)_C \times SU(2)_L \times U(1)_Y \times U(1)_\chi $$SU(3)C×SU(2)L×U(1)Y×U(1)χ, where $$U(1)_\chi $$U(1)χ comes from $$SO(10) \rightarrow SU(5) \times U(1)_\chi $$SO(10)→SU(5)×U(1)χ, supplemented by the non-Abelian discrete $$\Delta (27)$$Δ(27) symmetry for three lepton families, Dirac neutrino masses and their mixing are radiatively generated through dark matter. The gauge $$U(1)_\chi $$U(1)χ symmetry is broken spontaneously. The discrete $$\Delta (27)$$Δ(27) symmetry is broken softly and spontaneously. Together, they result in two residual symmetries, a global $$U(1)_L$$U(1)L lepton number and a dark symmetry, which may be $$Z_2$$Z2, $$Z_3$$Z3, or $$U(1)_D$$U(1)D depending on what scalar breaks $$U(1)_\chi $$U(1)χ. Cobimaximal neutrino mixing, i.e. $$\theta _{13} \ne 0$$θ13≠0, $$\theta _{23} = \pi /4$$θ23=π/4, and $$\delta _{CP} = \pm \pi /2$$δCP=±π/2, may also be obtained.

scholarly journals Thermal dark matter through the Dirac neutrino portal

2018 ◽  
Vol 97 (7) ◽  
Author(s):  
Brian Batell ◽  
Tao Han ◽  
David McKeen ◽  
Barmak Shams Es Haghi
Keyword(s):  
Dark Matter ◽  
Dirac Neutrino

scholarly journals DARK MATTER CANDIDATE FROM CONFORMALITY

2007 ◽  
Vol 22 (13) ◽  
pp. 931-937 ◽  
Author(s):  
P. H. FRAMPTON
Keyword(s):  
Dark Matter ◽  
Standard Model ◽  
Cross Section ◽  
Weak Interaction ◽  
Gauge Theories ◽  
Dark Matter Candidate ◽  
Beyond The Standard Model ◽  
The Standard Model ◽  
Relic Density ◽  
Baryonic Dark Matter

Abelian quiver gauge theories provide candidates for the conformality approach to physics beyond the standard model which possess novel cancellation mechanisms for quadratic divergences. A Z2 symmetry ( R parity) can be imposed and leads naturally to a dark matter candidate which is the Lightest Conformality Particle (LCP), a neutral spin-1 / 2 state with weak interaction annihilation cross-section, mass in the 100 GeV region and relic density of non-baryonic dark matter Ωdm which can be consistent with the observed value Ωdm≃0.24.

17 keV NEUTRINO AND MAJORON MODELS

1992 ◽  
Vol 07 (09) ◽  
pp. 2021-2031 ◽  
Author(s):  
ANJAN S. JOSHIPURA
Keyword(s):  
Dark Matter ◽  
Vacuum Expectation ◽  
Vacuum Expectation Value ◽  
Expectation Value ◽  
Dirac Neutrino ◽  
Dirac Mass ◽  
Left Handed ◽  
The Invisible

A model for the 17 keV Dirac neutrino is considered in the framework of the SU(2) × U(1) theory. No right-handed neutrinos are introduced. The Dirac mass for the neutrino arises from the Le+Lτ–Lμ invariant couplings of the left-handed neutrinos to an SU(2) triplet. An SU(2) singlet field is introduced to suppress the Majoron coupling to the Z. This makes the model consistent with the LEP results on the invisible Z width. The singlet vacuum expectation value ω is constrained to be ≤O(80 MeV) from cosmological considerations. For, ω≈80 MeV, the 17 keV neutrino is shown to provide the bulk of the dark matter.

scholarly journals Dark QCD matters

2021 ◽  
Vol 2021 (12) ◽  
Author(s):  
Raghuveer Garani ◽  
Michele Redi ◽  
Andrea Tesi
Keyword(s):  
Dark Matter ◽  
Standard Model ◽  
Structure Formation ◽  
Gauge Theories ◽  
Initial Temperature ◽  
Pion Mass ◽  
Dark Sector ◽  
Abelian Gauge ◽  
The Standard Model

Abstract We investigate the nightmare scenario of dark sectors that are made of non-abelian gauge theories with fermions, gravitationally coupled to the Standard Model (SM). While testing these scenarios is experimentally challenging, they are strongly motivated by the accidental stability of dark baryons and pions, that explain the cosmological stability of dark matter (DM). We study the production of these sectors which are minimally populated through gravitational freeze-in, leading to a dark sector temperature much lower than the SM, or through inflaton decay, or renormalizable interactions producing warmer DM. Despite having only gravitational couplings with the SM these scenarios turn out to be rather predictive depending roughly on three parameters: the dark sector temperature, the confinement scale and the dark pion mass. In particular, when the initial temperature is comparable to the SM one these scenarios are very constrained by structure formation, ∆Neff and limits on DM self-interactions. Dark sectors with same temperature or warmer than SM are typically excluded.

scholarly journals Bound-state dark matter and Dirac neutrino masses

2018 ◽  
Vol 97 (11) ◽  
Author(s):  
M. Reig ◽  
D. Restrepo ◽  
J. W. F. Valle ◽  
O. Zapata
Keyword(s):  
Dark Matter ◽  
Bound State ◽  
Neutrino Masses ◽  
Dirac Neutrino
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