Sterile neutrino dark matter in a U(1) extension of the standard model
@article{Iwamoto2021SterileND, title={Sterile neutrino dark matter in a U(1) extension of the standard model}, author={Sho Iwamoto and K'aroly Seller and Zolt'an Tr'ocs'anyi}, journal={Journal of Cosmology and Astroparticle Physics}, year={2021}, volume={2022} }
We explore the parameter space of a U(1) extension of the standard model — also called the super-weak model — from the point of view of explaining the observed dark matter energy density in the Universe. The new particle spectrum contains a complex scalar singlet and three right-handed neutrinos, among which the lightest one is the dark matter candidate. We explore both freeze-in and freeze-out mechanisms of dark matter production. In both cases, we find regions in the plane of the super-weak…
9 Citations
Sterile neutrino dark matter in the super-weak model
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The superweak force is a minimal, anomaly-free U(1) extension of the standard model, designed to explain the origin of (i) neutrino masses and mixing matrix elements, (ii) dark matter, (iii) cosmic…
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References
SHOWING 1-10 OF 67 REFERENCES
Scalar dark matter in the B−L model
- Physics
- 2015
The U(1)B−L extension of the Standard Model requires the existence of right-handed neutrinos and naturally realizes the seesaw mechanism of neutrino mass generation. We study the possibility of…
Constraining a general U(1)′ inverse seesaw model from vacuum stability, dark matter, and collider
- PhysicsPhysical Review D
- 2020
We consider a class of gauged $U(1)$ extensions of the Standard Model (SM), where the light neutrino masses are generated by an inverse seesaw mechanism. In addition to the three right handed…
Dark matter progenitor: Light vector boson decay into sterile neutrinos
- Physics
- 2014
We show that the existence of new, light gauge interactions coupled to Standard Model (SM) neutrinos give rise to an abundance of sterile neutrinos through the sterile neutrinos' mixing with the SM.…
Sterile neutrinos as dark matter.
- PhysicsPhysical review letters
- 1994
This model is reexamine and it is found that hot, warm, and cold dark matter are all possibilities and the number density of sterile neutrinos is proportional to [mu][sup 2]/M so that the energy density today is independent of M, which is crucial in determining the large scale structure of the Universe.
One-loop corrections to light neutrino masses in gauged U(1) extensions of the standard model
- PhysicsPhysical Review D
- 2021
We consider gauged U(1) extensions of the standard model of particle physics with three right-handed sterile neutrinos and a singlet scalar. The neutrinos obtain mass via the type I seesaw mechanism.…
Freeze-in production of sterile neutrino dark matter in U(1)B−L model
- Physics
- 2016
With the advent of new and more sensitive direct detection experiments, scope for a thermal WIMP explanation of dark matter (DM) has become extremely constricted. The non-observation of thermal WIMP…
Dark Matter Through the Neutrino Portal
- Physics
- 2009
We consider a model of dark matter whose most prominent signature is a monochromatic flux of TeV neutrinos from the galactic center. As an example of a general scenario, we consider a specific model…
Relativistic freeze-in with scalar dark matter in a gauged B − L model and electroweak symmetry breaking
- PhysicsJournal of High Energy Physics
- 2021
We explore relativistic freeze-in production of scalar dark matter in gauged B − L model, where we focus on the production of dark matter from the decay and annihilation of Standard Model (SM) and B…