中文
相关论文

相关论文: Baryogenesis From Flavon Decays

200 篇论文

Distinct behavior of decaying particles in true and false vacua of the theory can lead to enhanced generation of baryon asymmetry, a scenario we call \textit{phase separation baryogenesis}. We demonstrate that for leptogenesis this…

高能物理 - 唯象学 · 物理学 2025-09-05 Jason Arakawa , Philip Lu , Volodymyr Takhistov

The presence of additional neutrino states with masses in the GeV range is allowed by electro-weak precision observables. However, these additional states can lead to lepton number violating interactions which potentially can wash out…

高能物理 - 唯象学 · 物理学 2011-10-06 Sebastian Hollenberg , Heinrich Päs , Dario Schalla

Leptogenesis is a class of scenarios in which the cosmic baryon asymmetry originates from an initial lepton asymmetry generated in the decays of heavy sterile neutrinos in the early Universe. We explain why leptogenesis is an appealing…

高能物理 - 唯象学 · 物理学 2013-01-16 Chee Sheng Fong , Enrico Nardi , Antonio Riotto

We discuss the possibility of generating the baryon asymmetry of the Universe when the temperature of the Universe is much below the electroweak scale. In our model the evaporation of primordial black holes or the decay of massive particles…

高能物理 - 唯象学 · 物理学 2011-05-23 Raghavan Rangarajan , Supratim Sengupta , Ajit M. Srivastava , ;

Among the mechanisms which successfully explain the generation of the Baryon Asymmetry of the Universe, Leptogenesis through right-handed neutrino decays is especially attractive. Unfortunately, this theory suffers from a lack of…

高能物理 - 唯象学 · 物理学 2009-05-25 G. Vertongen

It has been considered that baryogenesis models without a generation of $B$-$L$ asymmetry such as the GUT baryogenesis do not work since the asymmetry is washed out by the electroweak sphalerons. Here, we point out that helical…

高能物理 - 唯象学 · 物理学 2018-07-05 Kohei Kamada

Effects of electroweak phase transition (EWPT) in balance between baryon excess and the excess of stable quarks of new generation is studied. With the conservation of SU(2) symmetry and other quantum numbers, it makes possible sphaleron…

高能物理 - 唯象学 · 物理学 2021-10-20 Arnab Chaudhuri , Maxim Yu. Khlopov

Electroweak vacuum transition processes (sphalerons) in the early Universe provide a possible explanation of the baryon asymmetry. Anomaly theory suggests that these electroweak baryon number non-conserving processes are accompanied by the…

高能物理 - 唯象学 · 物理学 2007-05-23 Steven D. Bass

We study the transference of an initial leptonic charge contained in a complex scalar field (waterfall field) at the end of the inflation to the leptons of the standard model and then convert this leptonic charge in baryonic charge by…

高能物理 - 唯象学 · 物理学 2009-06-24 Carlos Martinez Prieto

We calculate the baryon asymmetry of the Universe which would arise during a first order electroweak phase transition due to minimal standard model processes. It agrees in sign and magnitude with the observed baryonic excess, for resonable…

高能物理 - 唯象学 · 物理学 2010-11-01 Glennys R. Farrar , M. E. Shaposhnikov

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

I give a brief overview of a novel mechanism for generating the baryon asymmetry of the universe at the electroweak scale. This scenario circumvents the need for a strongly first order electroweak phase transition by utilizing gauged…

高能物理 - 唯象学 · 物理学 2008-02-03 Mark Trodden

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

The cosmological matter-antimatter asymmetry can arise from the baryon number conserving CP asymmetry in two body decays of heavy particles, when the two final states carry equal and opposite baryon number, and one couples directly or…

高能物理 - 唯象学 · 物理学 2014-02-12 D. Aristizabal Sierra , Chee Sheng Fong , Enrico Nardi , Eduardo Peinado

Previous studies demonstrate that the inflaton, when coupled to the hypercharge Chern-Simons density, can source an explosive production of helical hypermagnetic fields. Then, in the absence of fermion production, those fields have the…

高能物理 - 唯象学 · 物理学 2023-06-21 Yann Cado , Mariano Quirós

Effect of the electroweak non-conservation of the baryon number could be a key ingredient to explain the ratio of dark and baryonic densities. If dark matter is explained by dark atoms, in which stable -2n charged particles are bound with n…

高能物理 - 唯象学 · 物理学 2024-01-15 V. A. Beylin , M. Yu. Khlopov , D. O. Sopin

Several models of baryo(lepto)-genesis that give rise to large inhomogeneities in the composition of the universe are presented. In particular, a variation of primordial abundances of light elements by the factor 2-5 at large distances is…

高能物理 - 唯象学 · 物理学 2007-05-23 A. D. Dolgov

We propose a new model for naturally light Dirac neutrinos and explain the baryon asymmetry of the universe through neutrinogenesis. We extend the standard model with a real singlet scalar, a heavy singlet Dirac fermion and a heavy doublet…

高能物理 - 唯象学 · 物理学 2008-11-26 Pei-Hong Gu , Hong-Jian He , Utpal Sarkar

The symmetry breaking of left right symmetric model around few TeV range permits the existence of massive right handed neutrinos or gauge bosons. In this work the decay of lightest right handed neutrinos in a class of minimal left right…

高能物理 - 唯象学 · 物理学 2020-10-06 Anupam Yadav , Sabeeha Naaz , Jyotsna Singh , R. B. Singh

We propose an unified model of dark matter and baryon asymmetry in a lepto-philic world above the electroweak scale. We provide an example where the inflaton decay products subsequently generate a lepton asymmetry and a dark matter…

高能物理 - 唯象学 · 物理学 2009-11-06 Kazunori Kohri , Anupam Mazumdar , Narendra Sahu , Philip Stephens