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Related papers: Asymmetric matter from $B-L$ symmetry breaking

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It has been pointed out in ref.[1] that in the nuMSM (Standard Model extended by three right-handed neutrinos with masses smaller than the electroweak scale), there is a corner in the parameter space where CP-violating resonant oscillations…

High Energy Physics - Phenomenology · Physics 2009-01-06 M. Laine , M. Shaposhnikov

We show that in supersymmetric models with gauged B-L symmetry, there is a new source for cosmological lepton asymmetry. The Higgs bosons responsible for B-L gauge symmetry breaking decay dominantly into right-handed sneutrinos \tilde{N}…

High Energy Physics - Phenomenology · Physics 2010-01-05 K. S. Babu , Yanzhi Meng , Zurab Tavartkiladze

Symmetries in the Physical Laws of Nature lead to observable effects. Beyond regularities and conserved magnitudes, the last decades in Particle Physics have seen the identification of symmetries, and their well defined breaking, as the…

High Energy Physics - Phenomenology · Physics 2020-06-26 Jose Bernabeu

In a baryon-symmetric universe, the baryon asymmetry observed for visible matter is matched by an equal and opposite asymmetry for dark matter, thereby closely connecting the number densities of both types of matter. This is a necessary…

High Energy Physics - Phenomenology · Physics 2015-06-12 Raymond R. Volkas

We investigate scenarios in which dark matter is stabilized by an abelian Z_N discrete gauge symmetry. Models are surveyed according to symmetries and matter content. Multi-component dark matter arises when N is not prime and Z_N contains…

High Energy Physics - Phenomenology · Physics 2011-02-18 Brian Batell

We provide a minimal alternative gauged U(1)$_{\rm B-L}$ model in which three right-handed neutrinos with charges of (5,-4,-4) and only one B-L Higgs field with charge 1 are introduced. Consistent active neutrino masses and mixings can be…

High Energy Physics - Phenomenology · Physics 2021-02-03 Kento Asai , Kazunori Nakayama , Shih-Yen Tseng

We propose a scenario of the right-handed neutrino dark matter in the context of the minimal gauged $U(1)_{B-L}$ model by introducing an additional parity which ensures the stability of dark matter particle. The annihilation of this…

High Energy Physics - Phenomenology · Physics 2014-11-20 Nobuchika Okada , Osamu Seto

Sterile neutrino dark matter of mass O(1-10) keV decays into an active neutrino and an X-ray photon, and the non-observation of the corresponding X-ray line requires the sterile neutrino to be more long-lived than estimated based on the…

High Energy Physics - Phenomenology · Physics 2014-03-14 Hiroyuki Ishida , Kwang Sik Jeong , Fuminobu Takahashi

An exact spacetime parity replicates the $SU(2) \times U(1)$ electroweak interaction, the Higgs boson $H$, and the matter of the Standard Model. This "Higgs Parity" and the mirror electroweak symmetry are spontaneously broken at scale $v' =…

High Energy Physics - Phenomenology · Physics 2019-07-12 David Dunsky , Lawrence J. Hall , Keisuke Harigaya

I suggest a new extension of the standard model of particle physics, which introduces a dark sector with the $SU(2)_{D}\otimes U(1)_{D'}$ symmetry besides the SM sector. The new particles of the model all inhabit in the dark sector. The…

High Energy Physics - Phenomenology · Physics 2019-06-26 Wei-Min Yang

We propose a new mechanism which simultaneously explains tiny neutrino masses, stability of dark matter and baryon asymmetry of the Universe via leptogenesis due to the common origin: a spontaneous breaking of a $U(1)_X$ gauge symmetry at…

High Energy Physics - Phenomenology · Physics 2023-08-02 Toshinori Matsui , Takaaki Nomura , Kei Yagyu

We construct a model explaining dark matter, baryon asymmetry and reheating in quintessential inflation model. Three generations of right-handed neutrinos having hierarchical masses, and the light scalar field leading to self-interaction of…

High Energy Physics - Phenomenology · Physics 2023-04-05 Kohei Fujikura , Soichiro Hashiba , Jun'ichi Yokoyama

In the absence of low-energy supersymmetry, a multiplicity of weak-scale Higgs doublets would require additional fine-tunings unless they formed an irreducible multiplet of a non-abelian symmetry. Remnants of such symmetry typically render…

High Energy Physics - Phenomenology · Physics 2013-05-29 S. M. Barr

The Inverse Seesaw naturally explains the smallness of neutrino masses via an approximate $B-L$ symmetry broken only by a correspondingly small parameter. In this work the possible dynamical generation of the Inverse Seesaw neutrino mass…

High Energy Physics - Phenomenology · Physics 2017-12-06 Valentina De Romeri , Enrique Fernandez-Martinez , Julia Gehrlein , Pedro A. N. Machado , Viviana Niro

Reframing certain well-known particle models in terms of normed division algebras leads to two new results for BSM physics. (1) We identify a sequence of complex structures which induces a cascade of breaking symmetries: Spin(10) $\mapsto$…

High Energy Physics - Phenomenology · Physics 2022-10-20 N. Furey , M. J. Hughes

We propose a new model where the Dirac mass term for neutrinos, the Majorana mass term for right-handed neutrinos, and the other new fermion masses arise via the spontaneous breakdown of the $U(1)_{B-L}$ gauge symmetry. The anomaly-free…

High Energy Physics - Phenomenology · Physics 2014-07-10 Shinya Kanemura , Toshinori Matsui , Hiroaki Sugiyama

It is often said that asymmetric dark matter is light compared to typical weakly interacting massive particles. Here we point out a simple scheme with a neutrino portal and $\mathcal{O}(60 \text{ GeV})$ asymmetric dark matter which may be…

High Energy Physics - Phenomenology · Physics 2022-10-19 Eleanor Hall , Robert McGehee , Hitoshi Murayama , Bethany Suter

A gauged U(1)_B-L symmetry predicts three right handed handed neutrinos and its spontaneous breaking automatically yields the seesaw mechanism. In a supersymmetric setting this breaking can be nicely linked with inflation to yield deltaT/ T…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. N. Senoguz , Q. Shafi

The radiative seesaw model with gauged $\mathrm{U(1)}_{B-L}\times\mathbb{Z}_2$ extension is a well-motivated scenario which gives consistent predictions of active neutrino masses and the abundance of dark matter. Majorana masses of…

High Energy Physics - Phenomenology · Physics 2024-10-31 Shinya Kanemura , Yushi Mura , Guohao Ying

Interactions of heavy Majorana neutrinos in the thermal phase of the early universe may be the origin of the cosmological matter-antimatter asymmetry. Successful baryogenesis, independent of initial conditions, is possible for neutrino…

High Energy Physics - Phenomenology · Physics 2016-09-06 Wilfried Buchmüller
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