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Related papers: A Single Scale Theory for Cold and Hot Dark Matter

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We consider an extension of the nuMSM in which sterile neutrino masses originate from the VEV of a Higgs singlet phi and dark matter is produced through the decays of phi rather than through active-sterile neutrino mixing. This model, which…

High Energy Physics - Phenomenology · Physics 2013-05-10 Kyle Allison

We propose a gauged $U(1)_{B-L}$ extension of the standard model (SM) to explain simultaneously the light neutrino masses and dark matter (DM). The generation of neutrino masses occurs through a variant of type-II seesaw mechanism in which…

High Energy Physics - Phenomenology · Physics 2020-02-18 Satyabrata Mahapatra , Nimmala Narendra , Narendra Sahu

We study an extension of the MSSM with a singlet S with coupling SH1H2 in order to solve the mu problem as in the NMSSM, and right-handed neutrinos N with couplings SNN in order to generate dynamically electroweak-scale Majorana masses. We…

High Energy Physics - Phenomenology · Physics 2009-01-21 D. G. Cerdeno , C. Munoz , O. Seto

We study sterile neutrino dark matter (DM) in a classically conformal U(1)' extension of the Standard Model with three right-handed neutrinos and a Majoron-like singlet scalar that generate the observed pattern of active neutrino masses and…

High Energy Physics - Phenomenology · Physics 2026-02-13 João Gonçalves , Danny Marfatia , António P. Morais , Vinícius Oliveira , Roman Pasechnik

The asymmetric dark matter scenario is known to give an interesting solution for the cosmic coincidence problem between baryon and dark matter densities. In the scenario, the dark matter asymmetry, which is translated to the dark matter…

High Energy Physics - Phenomenology · Physics 2015-05-27 Naoyuki Haba , Shigeki Matsumoto , Ryosuke Sato

There appear to be three challenges that any theory of dark matter must face: (i) why is $\Omega_{DM}$ of the same order as $\Omega_{Baryons}$ ? (ii) what are the near solar mass objects ($\sim 0.5 M_{\odot}$) observed by the MACHO…

Astrophysics · Physics 2016-11-03 R. N. Mohapatra , V. L. Teplitz

We extend the concept of matter parity $P_M=(-1)^{3(B-L)}$ to non-supersymmetric theories and argue that $P_M$ is the natural explanation to the existence of Dark Matter of the Universe. We show that the non-supersymmetric Dark Matter must…

High Energy Physics - Phenomenology · Physics 2010-01-27 Mario Kadastik , Kristjan Kannike , Martti Raidal

In prior article of the author, the unimodular bimode gravity/systo-gravity, with the scalar-graviton/systolon dark matter, was worked out. To compile with the anomalous rotation curves of galaxies the scale of the local scale violation in…

General Relativity and Quantum Cosmology · Physics 2012-11-02 Yu. F. Pirogov

We review the prospects for dark matter (DM) in two classes of supersymmetric (SUSY) models which are characterized by the different mechanism of SUSY breaking, namely the more common supergravity models with very large scale of SUSY…

High Energy Physics - Phenomenology · Physics 2007-05-23 Stefano Borgani , Antonio Masiero

We consider a model for cold dark matter, which combines a real scalar singlet and a real scalar $SU(2)_L$ triplet field, both of which are residing in the odd representation of a global $Z_2$ symmetry. The parameter space of the model is…

High Energy Physics - Phenomenology · Physics 2014-05-08 Oliver Fischer , Jochum J. van der Bij

We argue that the striking similarity between the cosmic abundances of baryons and dark matter, despite their very different astrophysical behavior, strongly motivates the scenario in which dark matter resides within a rich dark sector…

High Energy Physics - Phenomenology · Physics 2024-06-13 Arushi Bodas , Manuel A. Buen-Abad , Anson Hook , Raman Sundrum

We discuss the possibility of light dark matter in a general singlet extension of the MSSM. Singlino LSPs with masses of a few GeV can explain the signals reported by the CRESST, CoGeNT and possibly also DAMA experiments. The interactions…

High Energy Physics - Phenomenology · Physics 2015-03-17 Rolf Kappl , Michael Ratz , Martin Wolfgang Winkler

I suggest a practical particle model as an extension to the standard model. The model has a TeV scale $U(1)_{B-L}$ symmetry and it contains the fourth generation fermions with the TeV scale masses, in which including a cold dark matter…

High Energy Physics - Phenomenology · Physics 2013-05-15 Wei-Min Yang

The generation of neutrino masses by inverse seesaw mechanisms has advantages over other seesaw models since the potential new physics can be produced at the TeV scale. We propose a model that generates the inverse seesaw mechanism via…

High Energy Physics - Phenomenology · Physics 2020-06-29 N. Rojas , R. A. Lineros , F. Gonzalez-Canales

It has been proposed that two resonances could coincide in the early universe at temperatures $T \sim 0.2 ... 0.5$ GeV: one between two nearly degenerate GeV-scale sterile neutrinos, producing a large lepton asymmetry through freeze-out and…

High Energy Physics - Phenomenology · Physics 2020-07-08 J. Ghiglieri , M. Laine

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. Specifically, in the mass range of…

High Energy Physics - Phenomenology · Physics 2014-06-18 Brian Shuve , Itay Yavin

In this work we study a classically scale invariant extension of the Standard Model that can explain simultaneously dark matter and the baryon asymmetry in the universe. In our set-up we introduce a dark sector, namely a non-Abelian SU(2)…

High Energy Physics - Phenomenology · Physics 2016-11-23 Valentin V. Khoze , Alexis D. Plascencia

In this work, we explain three beyond standard model (BSM) phenomena, namely neutrino masses, the baryon asymmetry of the Universe and Dark Matter, within a single model and in each explanation the right handed (RH) neutrinos play the prime…

High Energy Physics - Phenomenology · Physics 2019-06-26 Anirban Biswas , Sandhya Choubey , Laura Covi , Sarif Khan

Despite direct observations favoring a low mass density, a critical density universe with a neutrino component of dark matter provides the best existing model to explain the observed structure of the universe over more than three orders of…

Astrophysics · Physics 2009-10-31 David O. Caldwell

We investigate the possibility of keV scale thermal dark matter (DM) in a gauged $B - L$ extension of the standard model with three right-handed neutrinos (RHN) and one vector like fermion in the context of cosmic inflation. The complex…

High Energy Physics - Phenomenology · Physics 2022-09-21 Debasish Borah , Suruj Jyoti Das , Abhijit Kumar Saha