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相关论文: Baryogenesis from Long Cosmic Strings

200 篇论文

${\rm B - L}$ cosmic strings form in a wide class of theories beyond the Standard Model which contain a ${\rm U}(1)_{{\rm B - L}}$ gauge symmetry. They can form at the end of hybrid inflation and explain, together with inflation, the Cosmic…

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

Generic axion models give rise to axion domain walls in the early Universe and they have to disappear not to overclose the universe, thus limiting the nature of discrete symmetry allowed in these type of models. Through QCD sphalerons, net…

高能物理 - 唯象学 · 物理学 2007-05-23 S. N. Nayak , U. A. Yajnik

In a previous work, a mechanism was presented by which baryon asymmetry can be generated during inflation from elliptically polarized gravitons. Nonetheless, the mechanism only generated a realistic baryon asymmetry under special…

高能物理 - 理论 · 物理学 2009-11-10 Stephon H. S. Alexander , S. James Gates

A generic prediction of models where supersymmetry is broken at scales within a few orders of magnitude of the weak scale and is fed down to the observable sector by gauge interactions is the existence of superconducting cosmic strings…

高能物理 - 唯象学 · 物理学 2009-10-31 R. Brandenberger , A. Riotto

We propose a robust, unified framework, in which the similar baryon and dark matter cosmic abundances both arise from the physics of weakly interacting massive particles (WIMPs), with the rough quantitative success of the so-called "WIMP…

高能物理 - 唯象学 · 物理学 2015-06-12 Yanou Cui , Raman Sundrum

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 baryon-antibaryon asymmetry (excess of matter over antimatter in our Universe), indicated by observational data from the Cosmic Microwave Background anisotropies, predictions of primordial Nucleosynthesis, and the absence of intense…

广义相对论与量子宇宙学 · 物理学 2020-10-13 P. C. M. Delgado , M. B. Jesus , N. Pinto-Neto , T. Mourão , G. S. Vicente

We have studied numerically the evolution and decay of axion strings. These global defects decay mainly by axion emission and thus contribute to the cosmological axion density. The relative importance of this source relative to misalignment…

高能物理 - 唯象学 · 物理学 2009-10-31 C. Hagmann , S. Chang , P. Sikivie

In generic models for grand unified theories(GUT), various types of baryon number violating processes are expected when quarks and leptons propagate in the background of GUT strings. On the other hand, in models with large extra dimensions,…

高能物理 - 唯象学 · 物理学 2009-11-07 Tomohiro Matsuda

Unified theories containing a $U(1)_{B-L}$ gauge symmetry predict heavy Majorana right-handed neutrinos. In such theories, cosmic strings may form at the $B-L$ breaking scale. If the Higgs field forming the strings is also the Higgs field…

高能物理 - 唯象学 · 物理学 2009-10-28 R. Jeannerot

We examine the generation of baryon asymmetry at the weak scale from a primordial lepton asymmetry. If the electroweak phase transition is first order, partial reflection of tau leptons off the bubble walls and the resulting hypercharge…

高能物理 - 唯象学 · 物理学 2009-10-28 S. A. Abel , K. E. C. Benson

Baryogenesis scenarios at the string scale are considered. The observed baryon to entropy ratio, $n_B /s \sim 10^{-10}$, can be explained in these scenarios.

高能物理 - 唯象学 · 物理学 2009-10-30 H. Aoki , H. Kawai

Cosmic strings can be created in the early universe during symmetry-breaking phase transitions, such as might arise if the gauge structure of the standard model is extended by additional U(1) factors at high energies. Cosmic strings present…

高能物理 - 唯象学 · 物理学 2009-10-29 Yanou Cui , David E. Morrissey

A mechanism is presented, in which the mixing of right handed heavy Majorana neutrinos creates a $CP-$asymmetric universe. When these Majorana neutrinos subsequently decay more leptons than anti-leptons are produced. The lepton asymmetry…

高能物理 - 唯象学 · 物理学 2009-10-28 Marion Flanz , Emmanuel A. Paschos , Utpal Sarkar , Jan Weiss

We propose that the baryon asymmetry of the Universe may originate from the amplification of quantum fluctuations of a light complex scalar field during inflation. CP-violation is sourced by complex mass terms, which are smaller than the…

天体物理学 · 物理学 2008-12-18 Bjorn Garbrecht , Tomislav Prokopec

The cosmological baryon asymmetry can be explained by the nonperturbative electroweak reprocessing of a lepton asymmetry generated in the out-of-equilibrium decay of heavy right-handed Majorana neutrinos. We analyze this mechanism in detail…

高能物理 - 唯象学 · 物理学 2007-05-23 Michael Pluemacher

The possible role of supersymmetry in our understanding of big bang baryogenesis and cosmological dark matter is explored. The discussion will be limited to the out-of equilibrium decay scenario in SUSY GUTs, the decay of scalar…

高能物理 - 唯象学 · 物理学 2016-09-01 Keith A. Olive

We study the structure of cosmic strings produced at the breaking of an anomalous U(1) gauge symmetry present in many superstring compactification models. We show that their coupling with the axion necessary in order to cancel the anomalies…

高能物理 - 唯象学 · 物理学 2009-10-07 P. Binetruy , C. Deffayet , P. Peter

In the following work we consider the possibility of explaining the observed baryon number asymmetry in the universe from simple baryon number violating modifications, involving massive scalar bosons, to the Standard Model. In these cases…

高能物理 - 唯象学 · 物理学 2009-10-30 J. P. Bowes , R. R. Volkas

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