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相关论文: Lepton Asymmetric Universe

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We propose a scenario which can explain large lepton asymmetry and small baryon asymmetry simultaneously. Large lepton asymmetry is generated through Affleck-Dine (AD) mechanism and almost all the produced lepton numbers are absorbed into…

高能物理 - 唯象学 · 物理学 2009-11-07 M. Kawasaki , Fuminobu Takahashi , Masahide Yamaguchi

We propose a scenario to produce large primordial lepton flavor asymmetries with vanishing total lepton asymmetry, based on the Affleck-Dine mechanism with Q-ball formation. This scenario can produce large lepton flavor asymmetries while…

高能物理 - 唯象学 · 物理学 2026-02-17 Kensuke Akita , Koichi Hamaguchi , Maksym Ovchynnikov

We propose a mechanism for cogenesis of baryon and dark matter (DM) in the universe via the Affleck-Dine (AD) route. An AD field which breaks the lepton number symmetry, leads to the generation of lepton asymmetry by virtue of its cosmic…

高能物理 - 唯象学 · 物理学 2023-05-24 Debasish Borah , Suruj Jyoti Das , Nobuchika Okada

A large lepton number asymmetry of $\mathcal{O}(0.1-1)$ at present universe might not only be allowed but also necessary for consistency among cosmological data. We show that, if a sizeable lepton number asymmetry were produced before the…

高能物理 - 唯象学 · 物理学 2017-05-10 Gabriela Barenboim , Wan-Il Park

We present here a realistic model to produce a very large lepton asymmetry L of 0.1 to 1, without producing a large baryon asymmetry. The model is based on the Affleck and Dine scenario, in which the field acquiring a large vacuum…

高能物理 - 唯象学 · 物理学 2009-10-30 J. A. Casas , Wai Yan Cheng , G. B. Gelmini

We investigate whether the baryon asymmetry of the universe is explained in the framework of the supersymmetric extension of the Standard Model with R-parity violating interactions. It is shown that the Affleck-Dine mechanism naturally…

高能物理 - 唯象学 · 物理学 2014-08-05 Tetsutaro Higaki , Kazunori Nakayama , Ken'ichi Saikawa , Tomo Takahashi , Masahide Yamaguchi

We show that the monopole problem in Grand Unified Theories as well as the domain wall problem may be easily solved if the lepton number asymmetry in the Universe is large enough.

高能物理 - 唯象学 · 物理学 2009-10-30 Borut Bajc , Antonio Riotto , Goran Senjanovic'

We propose a new mechanism of lepton (L) number asymmetry generation, hence offer an explanation of matter-antimatter imbalance when a significant amount of baryon number is later transformed from this L-number by known electroweak…

高能物理 - 唯象学 · 物理学 2022-09-07 M. Yoshimura

In this article, we discuss the mechanism for generating the lepton/baryon number and its subsequent conservation based on extradimensional evolution. The internal angular momentum of extra space is related to the lepton/baryon charge.…

高能物理 - 唯象学 · 物理学 2021-09-14 Valery V. Nikulin , Sergey G. Rubin

Baryogenesis appears to require lepton number violation. This is naturally realized in extensions of the standard model containing right-handed neutrinos. We discuss the generation of a baryon asymmetry by the out-of-equilibrium decay of…

高能物理 - 唯象学 · 物理学 2007-05-23 W. Buchmuller , M. Plumacher

Sterile neutrino is a fascinating candidate for dark matter. In this paper, we examine the Affleck-Dine (AD) leptogenesis scenario generating a large lepton asymmetry, which can induce the resonant production of sterile neutrino dark matter…

高能物理 - 唯象学 · 物理学 2024-08-09 Kentaro Kasai , Masahiro Kawasaki , Kai Murai

Leptogenesis is a class of scenarios where the baryon asymmetry of the Universe is produced from a lepton asymmetry generated in the decays of a heavy sterile neutrino. We explain the motivation for leptogenesis. We review the basic…

高能物理 - 唯象学 · 物理学 2008-11-26 Sacha Davidson , Enrico Nardi , Yosef Nir

Radiative neutrino mass models have interesting features, which make it possible to relate neutrino masses to the existence of dark matter. However, the explanation of the baryon number asymmetry in the universe seems to be generally…

高能物理 - 唯象学 · 物理学 2015-03-17 H. Higashi , T. Ishima , D. Suematsu

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

The lepton sector masses and mixing angles can be explained in models based on $A_4$ symmetry. $A_4$ is a non-Abelian discrete group. Therefore, one issue in constructing models based on it is explaining the origin of $A_4$. A plausible…

高能物理 - 唯象学 · 物理学 2010-02-23 Joshua Berger , Yuval Grossman

We consider a baryogenesis scenario, where the difference of baryon (B) and lepton (L) number is conserved in such a way that the B-L asymmetry in the standard model sector is compensated by an asymmetry of opposite sign stored in the dark…

高能物理 - 唯象学 · 物理学 2010-11-26 Florian Bauer , Marc-Thomas Eisele , Mathias Garny

The observed baryon asymmetry of the Universe is suitably created in thermal leptogenesis through the out-of-equilibrium decay of $N_1$, the lightest of the three heavy singlet neutral fermions which anchor the seesaw mechanism to obtain…

高能物理 - 唯象学 · 物理学 2007-05-23 Ernest Ma , Narendra Sahu , Utpal Sarkar

Affleck-Dine (AD) mechanism for leptogenesis involves the cosmological evolution of a complex scalar field (AD field) that carries non-zero lepton number. We show how explicit lepton number breaking terms, which involve the AD field needed…

高能物理 - 唯象学 · 物理学 2022-03-30 Rabindra N. Mohapatra , Nobuchika Okada

We describe a "neutrinogenesis" mechanism whereby, in the presence of right-handed neutrinos with sufficiently small pure Dirac masses, (B+L)-violating sphaleron processes create the baryon asymmetry of the Universe, even when B=L=0…

高能物理 - 唯象学 · 物理学 2009-09-25 Karin Dick , Manfred Lindner , Michael Ratz , David Wright

Oscillations of active to sterile neutrinos with a small mixing angle sin 2 \theta < 10^{-2} could generate a large lepton asymmetry in the Early Universe. The final order of magnitude of the lepton asymmetry \eta is mainly determined by…

高能物理 - 唯象学 · 物理学 2011-05-23 R. Buras , D. V. Semikoz
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