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相关论文: On Constraining Electroweak-Baryogenesis with Inho…

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Electroweak baryogenesis is an attractive mechanism to generate the baryon asymmetry of the Universe via a strong first order electroweak phase transition. We compare the phase transition patterns suggested by the vacuum structure at the…

高能物理 - 唯象学 · 物理学 2021-03-12 Sebastian Baum , Marcela Carena , Nausheen R. Shah , Carlos E. M. Wagner , Yikun Wang

We calculate the baryon asymmetry generated at the electroweak phase transition in the minimal supersymmetric standard model, treating the particles in a WKB approximation in the bubble wall background. A set of diffusion equations for the…

高能物理 - 唯象学 · 物理学 2009-10-30 J. Cline , M. Joyce , K. Kainulainen

We show that primordial nucleosynthesis in baryon inhomogeneous big-bang models can lead to significant heavy-element production while still satisfying all the light-element abundance constraints including the low lithium abundance observed…

天体物理学 · 物理学 2009-10-22 K. Jedamzik , G. M. Fuller , G. J. Mathews , T. Kajino

The possibility of baryogenesis at the electroweak phase transition is considered within the context of a minimal supersymmetric standard model with spontaneous R-parity violation. Provided that at least one of the sneutrino fields acquires…

高能物理 - 唯象学 · 物理学 2009-10-31 Tuomas Multamaki , Iiro Vilja

If stable electroweak strings are copiously produced during the electroweak phase transition, they may contribute significantly to the presently observed baryon to entropy ratio of the universe. This analysis establishes the feasibility of…

高能物理 - 唯象学 · 物理学 2007-05-23 Robert H. Brandenberger , Anne-Christine Davis

We investigate the possibility that inhomogeneous nucleosynthesis may eventually be used to explain the abundances of \li6, \be9 and B in population II stars. The present work differs from previous studies in that we have used a more…

Standard electroweak baryogenesis in the context of a first order phase transition is effective in generating the baryon asymmetry of the universe if the broken phase bubbles expand at subsonic speed, so that CP asymmetric currents can…

高能物理 - 唯象学 · 物理学 2015-06-03 Chiara Caprini , Jose M. No

In light of the Higgs boson discovery we reconsider generation of the baryon asymmetry in the non-minimal split Supersymmetry model with an additional singlet superfield in the Higgs sector. We find that successful baryogenesis during the…

高能物理 - 唯象学 · 物理学 2016-12-21 S. V. Demidov , D. S. Gorbunov , D. V. Kirpichnikov

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

The standard requirement for the production of baryons at the electroweak phase transition, that the phase transition be first order and the sphaleron bound be satisfied, is predicated on the assumption of a radiation dominated universe at…

高能物理 - 唯象学 · 物理学 2016-09-06 Michael Joyce

The possibility of creating baryon asymmetry at the electroweak phase transition in the minimal supersymmetric standard model is considered for the case when right-handed squarks are much lighter than left-handed ones. It is shown that the…

高能物理 - 唯象学 · 物理学 2009-10-28 D. Delepine , J. -M. Gerard , R. Gonzalez Felipe , J. Weyers

Based on a scenario of the inhomogeneous big-bang nucleosynthesis (IBBN), we investigate the detailed nucleosynthesis that includes the production of heavy elements beyond Li-7. From the observational constraints on light elements of He4…

宇宙学与河外天体物理 · 物理学 2013-07-08 Riou Nakamura , Masa-aki Hashimoto , Shin-ichiro Fujimoto , Nobuya Nishimura , Katsuhiko Sato

We study the impact of possible high density baryonic bubbles on the early formed QSO, IGM, and metal poor stars. Such bubbles could be created, under certain conditions, in Affleck-Dine model of baryogenesis and may occupy a relatively…

天体物理学 · 物理学 2009-11-10 Shunji Matsuura , Alexander. D. Dolgov , Shigehiro Nagataki , Katsuhiko Sato

We propose a mechanism for baryogenesis in which the baryon asymmetry is generated as an equilibrium response of weak sphalerons in a region where electroweak sphaleron transitions remain unsuppressed, $h/T\lesssim 1$. A nonzero equilibrium…

高能物理 - 唯象学 · 物理学 2026-05-18 Jacopo Azzola , Oleksii Matsedonskyi , Andreas Weiler

This article presents an original code for Big Bang Nucleosynthesis in a baryon inhomogeneous model of the universe. In this code neutron diffusion between high and low baryon density regions is calculated simultaneously with the nuclear…

天体物理学 · 物理学 2009-11-11 Juan F. Lara

Electroweak baryogenesis can occur in the ``adiabatic limit,'' in which expanding bubbles of true vacuum are assumed to have rather thick walls and be slowly moving. Here the problem of calculating the baryon asymmetry in this limit is…

高能物理 - 唯象学 · 物理学 2009-10-28 Michael Dine , Scott Thomas

A phenomenological consequence of electroweak baryogenesis is studied in connection with the Higgs physics. In a two Higgs double model, the first order phase transition can be strong enough to allow the electroweak baryogenesis due to the…

高能物理 - 唯象学 · 物理学 2009-11-10 Shinya Kanemura , Yasuhiro Okada , Eibun Senaha

We consider inhomogeneous big bang nucleosynthesis in light of the present observational situation. Different observations of He-4 and D disagree with each other, and depending on which set of observations one uses, the estimated primordial…

天体物理学 · 物理学 2009-10-30 K. Kainulainen , H. Kurki-Suonio , E. Sihvola

The generation of the baryon asymmetry of the universe is considered in the standard model of the electroweak theory with simple extensions of the Higgs sector. The propagation of quarks of masses up to about 5 GeV are considered, taking…

高能物理 - 唯象学 · 物理学 2010-11-01 A. Kundu , S. Mallik

Big Bang nucleosynthesis in the presence of decaying relic neutral particles is examined in detail. All non-thermal processes important for the determination of light-element abundance yields of 2H, 3H, 3He, 4He, 6Li, and 7Li are coupled to…

高能物理 - 唯象学 · 物理学 2009-11-11 Karsten Jedamzik