中文
相关论文

相关论文: Activated Sphalerons and Large Extra Dimensions

200 篇论文

We present a testable mechanism of low-scale baryogenesis and dark matter production in which neither baryon nor lepton number are violated. Charged $D$ mesons are produced out-of-equilibrium at tens of MeV temperatures. The $D$ mesons…

高能物理 - 唯象学 · 物理学 2021-02-12 Gilly Elor , Robert McGehee

We investigate the viability of electroweak baryogenesis in a model with a first order electroweak phase transition induced by the addition of two gauge singlet scalars. A vector-like lepton doublet is introduced in order to provide CP…

高能物理 - 唯象学 · 物理学 2019-10-08 Nicole F. Bell , Matthew J. Dolan , Leon S. Friedrich , Michael J. Ramsey-Musolf , Raymond R. Volkas

We show that a phase transition may take place in the early Universe at a temperature $T_*$ via a Standard Model singlet scalar field which happens to couple to right handed neutrinos (RHN) resulting a temperature dependent mass for them…

高能物理 - 唯象学 · 物理学 2024-11-14 Dipendu Bhandari , Arghyajit Datta , Arunansu Sil

A possible solution to the observed baryon asymmetry in the universe is described, based on the physics of the standard model of electroweak interactions. At temperatures high enough electroweak physics provides violation of baryon number,…

高能物理 - 唯象学 · 物理学 2007-05-23 Nicholas Petropoulos

In an external magnetic field, the energy of the electroweak sphaleron---representing the energy barrier to baryon and lepton number violation---decreases but remains nonzero until the upper Ambjorn-Olesen critical field strength set by the…

高能物理 - 理论 · 物理学 2020-09-16 David L. -J. Ho , Arttu Rajantie

Lepton flavour asymmetries generated at the onset of the oscillations of sterile neutrinos with masses above the electroweak scale can be large enough to partly survive washout and to explain the baryon asymmetry of the Universe. This opens…

高能物理 - 唯象学 · 物理学 2014-10-01 Bjorn Garbrecht

We suppose that the baryon asymmetry is produced by thermal leptogenesis (with flavour effects), at temperatures $\sim 10^{9} - 10^{10}$ GeV, in the supersymmetric seesaw with universal and real soft terms. The parameter space is restricted…

高能物理 - 唯象学 · 物理学 2009-01-06 Sacha Davidson , Julia Garayoa , Federica Palorini , Nuria Rius

We consider the presence of cosmic string induced density fluctuations in the universe at temperatures below the electroweak phase transition temperature. Resulting temperature fluctuations can restore the electroweak symmetry locally,…

高能物理 - 唯象学 · 物理学 2009-11-07 Biswanath Layek , Soma Sanyal , Ajit M. Srivastava

For successful electroweak baryogenesis to take place through the sphaleron process the universe needs to undergo a strong first order cosmological phase transition. While it does not occur in the Standard Model it becomes possible in the…

高能物理 - 唯象学 · 物理学 2016-01-19 Anish Ghoshal

I propose a new mechanism for baryogenesis, in which the out-of-equilibrium condition is not neccessary. When the electroweak symmetry is broken spontaneously, left-handed neutrinos may get Majorana masses containing $CP-$violating phases.…

高能物理 - 唯象学 · 物理学 2007-05-23 Utpal Sarkar

We consider a model in which baryogenesis occurs at low scale, at a temperature below the electroweak phase transition. This model involves new diquark-type scalars which carry baryon number. Baryon number violation is introduced in the…

高能物理 - 唯象学 · 物理学 2019-01-30 Nicole F. Bell , Tyler Corbett , Michael Nee , Michael J. Ramsey-Musolf

We study the evolution of a cosmological baryon asymmetry in leptogenesis when the right-handed neutrinos are produced in inflaton decays. By performing a detailed numerical study over a broad range of inflaton-neutrino couplings we show…

高能物理 - 唯象学 · 物理学 2008-11-26 F. Hahn-Woernle , M. Plumacher

We discuss one-loop radiative corrections to the sphaleron-induced baryon number-violating transition rate near the electroweak phase transition in the standard model. We emphasize that in the case of a first-order transition a…

高能物理 - 唯象学 · 物理学 2011-07-19 Meik Hellmund , Jochen Kripfganz , Michael G. Schmidt

The origin of the matter-antimatter asymmetry remains one of the most fundamental problems of cosmology. In this talk I present a novel scenario for baryogenesis at the electroweak scale, without the need for a first order phase transition.…

高能物理 - 唯象学 · 物理学 2016-11-03 Juan Garcia-Bellido

We consider leptogenesis in scenarios with many neutrino singlets. We find that the lower bound for the reheating temperature can be significantly relaxed with respect to the hierarchical three neutrino case. We further argue that the upper…

高能物理 - 唯象学 · 物理学 2008-11-26 Marc-Thomas Eisele

We explore viable scenarios for parametric resonant amplification of electroweak (EW) gauge fields and Chern-Simons number during preheating, leading to baryogenesis at the electroweak (EW) scale. In this class of scenarios time-dependent…

高能物理 - 唯象学 · 物理学 2014-11-17 J. M. Cornwall , D. Grigoriev , A. Kusenko

Dirac neutrinos with lepton-number-violating interactions can give rise to a new leptogenesis mechanism. In its simplest renormalizable realization, based on a gauged B-L symmetry spontaneously broken by four units, the decay of a new…

高能物理 - 唯象学 · 物理学 2013-10-10 Julian Heeck

We report results obtained with the first complete event generator for electroweak baryon and lepton number violating interactions at supercolliders. We find that baryon number violation would be very difficult to establish, but lepton…

高能物理 - 唯象学 · 物理学 2009-10-28 M. J. Gibbs , A. Ringwald , B. R. Webber , J. T Zadrozny

We consider the scenario of electroweak baryogenesis mediated by cosmological defects in a model of extra dimension. We consider the domain wall on the brane in higher-dimensional theories.The electroweak breaking scale is suppressed and…

高能物理 - 唯象学 · 物理学 2007-05-23 Tomohiro Matsuda

Electroweak Baryogenesis is a particularly attractive theoretical scenario, since it relies on physics which can be tested at present high energy collider facilities. Within the Standard Model, it has been shown that the requirement of…

高能物理 - 唯象学 · 物理学 2016-11-03 M. Carena , C. E. M. Wagner