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相关论文: The Neutrino Mass Window for Baryogenesis

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Baryon asymmetry of the Universe is evaluated in the model originally proposed in Phys. Rev. Lett. 102 (2009) 051805, where Majorana masses of neutrinos are generated via three-loop diagrams composed of additional scalar bosons including…

高能物理 - 唯象学 · 物理学 2023-06-19 Mayumi Aoki , Kazuki Enomoto , Shinya Kanemura

The cosmological baryon asymmetry can be explained as remnant of heavy Majorana neutrino decays in the early universe. We study this out-of-equilibrium process by means of Kadanoff-Baym equations which are solved in a perturbative…

高能物理 - 唯象学 · 物理学 2008-11-26 Wilfried Buchmuller , Stefan Fredenhagen

In many realizations of leptogenesis, heavy right-handed neutrinos play the main role in the generation of an imbalance between matter and antimatter in the early Universe. Hence, it is relevant to address quantitatively their dynamics in a…

Recent years have seen a great improvement in the computation of $CP$-conserving and $CP$-violating equilibration rates for leptogenesis. These are relevant for the relativistic regime of the sterile Majorana fermions and the dynamics of…

高能物理 - 唯象学 · 物理学 2025-03-10 Björn Garbrecht , Edward Wang

Thermal leptogenesis explains the observed matter-antimatter asymmetry of the universe in terms of neutrino masses, consistent with neutrino oscillation experiments. We present a full quantum mechanical calculation of the generated lepton…

高能物理 - 唯象学 · 物理学 2013-11-04 A. Anisimov , W. Buchmuller , M. Drewes , S. Mendizabal

The temperature-dependent mass of the heavy neutrino can lead to the second leptogenesis occurring below the electroweak scale, potentially explaining the large discrepancy between baryon and lepton asymmetries. We investigate this scenario…

高能物理 - 唯象学 · 物理学 2025-03-19 YeolLin ChoeJo , Kazuki Enomoto , Yechan Kim , Hye-Sung Lee

The extension of the Standard Model by heavy right-handed neutrinos can simultaneously explain the observed neutrino masses via the seesaw mechanism and the baryon asymmetry of the Universe via leptogenesis. If the mass of the heavy…

高能物理 - 唯象学 · 物理学 2020-07-10 Marco Drewes , Bjorn Garbrecht , Dario Gueter , Juraj Klaric

We propose a new mechanism producing a non-vanishing lepton number asymmetry, based on decays of heavy Majorana neutrinos. If they are produced out of equilibrium, as occurs in preheating scenario, and are superpositions of mass eigenstates…

高能物理 - 唯象学 · 物理学 2014-11-17 G. Mangano , G. Miele

Low-scale baryogenesis and dark matter generation can occur via the production of neutral $B$ mesons at MeV temperatures in the early Universe, which undergo CP-violating oscillations and subsequently decay into a dark sector. In this work,…

高能物理 - 唯象学 · 物理学 2020-04-22 Gonzalo Alonso-Álvarez , Gilly Elor , Ann E. Nelson , Huangyu Xiao

The recent results of IceCube Neutrino Observatory include an excess of PeV neutrino events which appear to follow a broken power law different from the other lower energy neutrinos detected by IceCube. The possible astrophysical source of…

高能物理 - 唯象学 · 物理学 2021-05-28 Tista Mukherjee , Madhurima Pandey , Debasish Majumdar , Ashadul Halder

I review some aspects related with the connections between neutrino physics and the thermal leptogenesis mechanism for the generation of the cosmological baryon asymmetry of the Universe. A special attention is devoted to the problem of…

高能物理 - 唯象学 · 物理学 2007-05-23 F. R. Joaquim

We propose a model to explain tiny masses of neutrinos with the lepton number conservation, where neither too heavy particles beyond the TeV-scale nor tiny coupling constants are required. Assignments of conserving lepton numbers to new…

高能物理 - 唯象学 · 物理学 2017-11-29 Shinya Kanemura , Kodai Sakurai , Hiroaki Sugiyama

We propose a simple and flexible mechanism by which sterile neutrinos with masses below the electroweak scale can simultaneously account for the observed baryon asymmetry of the Universe and the dark matter abundance. Crucially, neutrinos…

高能物理 - 唯象学 · 物理学 2026-03-23 G. Arcadi , J. P. Garcés , 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 present a new mechanism of Baryogenesis and dark matter production in which both the dark matter relic abundance and the baryon asymmetry arise from neutral $B$ meson oscillations and subsequent decays. This set-up is testable at hadron…

高能物理 - 唯象学 · 物理学 2019-02-22 Gilly Elor , Miguel Escudero , Ann E. Nelson

We revisit the generation of a matter-antimatter asymmetry in the minimal extension of the Standard Model with two singlet heavy neutral leptons (HNL) that can explain neutrino masses. We derive an accurate analytical approximation to the…

高能物理 - 唯象学 · 物理学 2022-12-07 Pilar Hernandez , Jacobo Lopez-Pavon , Nuria Rius , Stefan Sandner

In theories where $B-L$ is a spontaneously broken local symmetry, the cosmological baryon asymmetry can be generated by the out-of-equilibrium decay of heavy Majorana neutrinos. We study this mechanism assuming a similar pattern of mixings…

高能物理 - 唯象学 · 物理学 2009-10-28 W. Buchmuller , M. Plumacher

We review the experimental evidence for a net baryon density in cosmology, and the theoretical mechanism for producing it, called leptogenesis, which relies on the creation of a lepton asymmetry at an intermediate step. The naturality of…

高能物理 - 唯象学 · 物理学 2007-05-23 J. Orloff

In this review we discuss how the models of neutrino masses can accommodate solutions to the problem of matter-antimatter asymmetry in the universe, dark energy or cosmological constant problem and dark matter candidates. The…

高能物理 - 唯象学 · 物理学 2009-11-13 Utpal Sarkar

Effects of the lightest neutrino mass in "flavoured" leptogenesis when the CP-violation necessary for the generation of the baryon asymmetry of the Universe is due exclusively to the Dirac and/or Majorana phases in the neutrino mixing…

高能物理 - 唯象学 · 物理学 2009-07-22 E. Molinaro , S. T. Petcov , T. Shindou , Y. Takanishi