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相关论文: Aidnogenesis via Leptogenesis and Dark Sphalerons

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Realization of the inverted hierarchy is studied in the radiative neutrino mass model with an additional doublet, in which neutrino masses and dark matter could be induced from a common particle. We show that the sufficient baryon number…

高能物理 - 唯象学 · 物理学 2015-06-12 Shoichi Kashiwase , Daijiro Suematsu

In the standard lore, the baryon asymmetry of the present universe is attributed to the leptogenesis from the sterile right-handed neutrino with heavy Majorana mass decaying into the Standard Model's leptons at the very early universe --…

高能物理 - 唯象学 · 物理学 2026-05-06 Juven Wang

We propose a novel mechanism to generate a suitable baryon asymmetry from dark (hidden) sector. This is a Baryogenesis through a reverse pathway of the "asymmetric dark matter" scenario. In the mechanism, the asymmetry of dark matter is…

高能物理 - 唯象学 · 物理学 2011-09-12 N. Haba , S. Matsumoto

We propose a novel scenario of generating lepton asymmetry via annihilation and coannihilation of dark sector particles including t-channel processes. In order to realistically implement this idea, we consider the scotogenic model having…

高能物理 - 唯象学 · 物理学 2020-05-19 Debasish Borah , Arnab Dasgupta , Sin Kyu Kang

We propose a novel framework where baryon asymmetry of the universe can arise due to forbidden decay of dark matter (DM) enabled by finite-temperature effects in the vicinity of a first order phase transition (FOPT). In order to implement…

高能物理 - 唯象学 · 物理学 2023-10-13 Debasish Borah , Arnab Dasgupta , Matthew Knauss , Indrajit Saha

We analyze leptogenesis in gauge extensions of the Standard Model with keV sterile neutrino dark matter. We find that both the observed dark matter abundance and the correct baryon asymmetry of the Universe can simultaneously emerge in…

高能物理 - 唯象学 · 物理学 2015-06-04 F. Bezrukov , A. Kartavtsev , M. Lindner

We propose a resonant leptogenesis scenario in a U(1)_{B-L} gauge extension of the standard model to generate large lepton asymmetries for cosmological baryon asymmetry and dark matter. After B-L number is spontaneously broken, inflaton can…

高能物理 - 唯象学 · 物理学 2010-12-09 Pei-Hong Gu

We demonstrate a common origin for high-scale leptogenesis and three-loop neutrino mass generation. Specifically we extend the standard model by two real singlet scalars, two singly charged scalars carrying different lepton numbers and two…

高能物理 - 唯象学 · 物理学 2017-05-24 Pei-Hong Gu

A scenario that relates the abundance of dark matter to the baryon asymmetry of the Universe is presented. In this scenario, based on a left-right extension of the Standard Model, dark matter is made of light, ~ 1 GeV, right-handed Majorana…

高能物理 - 唯象学 · 物理学 2007-05-23 Michel H. G. Tytgat

We propose that the observed baryon asymmetry of the Universe can naturally arise from a net asymmetry generated in the sleptonic sector at fairly low reheat temperatures. The best candidate is indeed the right-handed sneutrino. The initial…

高能物理 - 唯象学 · 物理学 2009-11-10 Rouzbeh Allahverdi , Bhaskar Dutta , Anupam mazumdar

We propose a minimal extension of the standard model with U(1)_{B-L} \times Z_{2} symmetry. In this model by assuming that the neutrinos are Dirac (i.e. $B-L$ is an exact symmetry), we found a simultaneous solution for non zero neutrino…

高能物理 - 唯象学 · 物理学 2018-10-17 Nimmala Narendra , Nirakar Sahoo , Narendra Sahu

We consider a simple extension of the Standard Model to consistently explain the observation of a peak in the galactic X-ray spectrum at 3.55 keV and the light neutrino masses along with the baryon asymmetry of the universe. The baryon…

高能物理 - 唯象学 · 物理学 2018-01-17 Sin Kyu Kang , Ayon Patra

The addition of gauge singlet fermions to the Standard Model Lagrangian renders the neutrinos massive and allows one to explain all that is experimentally known about neutrino masses and lepton mixing. At the same time, the gauge singlet…

高能物理 - 唯象学 · 物理学 2010-12-02 Wei-Chih Huang

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…

高能物理 - 唯象学 · 物理学 2022-10-19 Eleanor Hall , Robert McGehee , Hitoshi Murayama , Bethany Suter

We consider the production of asymmetric dark matter during hidden sector baryogenesis. We consider a particular supersymmetric model where the dark matter candidate has a number density approximately equal to the baryon number density,…

高能物理 - 唯象学 · 物理学 2011-10-03 Bhaskar Dutta , Jason Kumar

The existence of dark matter (DM) and the origin of the baryon asymmetry are persistent indications that the SM is incomplete. More recently, the ATLAS and CMS experiments have observed an excess of diphoton events with invariant mass of…

高能物理 - 唯象学 · 物理学 2016-06-08 Mads T. Frandsen , Ian M. Shoemaker

In the present universe visible and dark matter contribute comparable energy density although they have different properties. This coincidence can be elegantly explained if the dark matter relic density, originating from a dark matter…

高能物理 - 唯象学 · 物理学 2011-09-05 Pei-Hong Gu , Manfred Lindner , Utpal Sarkar , Xinmin Zhang

We consider the possibility that some primordial fields decay purely into the dark sector creating asymmetric dark matter. This asymmetry is subsequently transmuted into leptons and baryons. Within this paradigm we compute the amount of…

高能物理 - 唯象学 · 物理学 2013-10-07 Wan-Zhe Feng , Anupam Mazumdar , Pran Nath

In order to address the baryon asymmetry in the Universe one needs to understand the origin of baryon (B) and lepton (L) number violation. In this article, we discuss the mechanism of baryogenesis via leptogenesis to explain the…

高能物理 - 唯象学 · 物理学 2021-09-10 Pavel Fileviez Perez , Clara Murgui , Alexis D. Plascencia

We present a simple mechanism which allows the simultaneous generation of the baryon asymmetry of the Universe along with its dark matter content. To this goal, we employ the out-of-equilibrium decays of heavy bath states into a feebly…

高能物理 - 唯象学 · 物理学 2022-02-17 Andreas Goudelis , Pantelis Papachristou , Vassilis C. Spanos