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相关论文: The Effects of Electro-weak Phase Transition Dynam…

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It is known that baryon number inhomogeneities may arise as a consequence of electroweak baryogenesis. Their geometry, size, and amplitude depend on the parameters that characterize the baryogenesis mechanism, as well as on those that…

高能物理 - 唯象学 · 物理学 2009-11-10 Ariel Megevand , Francisco Astorga

The latent heat released during the expansion of bubbles in the electroweak phase transition reheats the plasma and causes the bubble growth to slow down. This decrease of the bubble wall velocity affects the result of electroweak…

高能物理 - 唯象学 · 物理学 2009-10-31 Ariel Megevand

The baryogenesis is reanalyzed based on the model by A.G.Cohen et al., in which the lepton number, generated by the neutrinos' scattering from the bubble walls appearing in the development of the electroweak phase transition, is converted…

高能物理 - 唯象学 · 物理学 2019-08-15 Azusa Yamaguchi , Akio Sugamoto

The standard picture of electroweak baryogenesis requires slowly expanding bubbles. This can be difficult to achieve if the vacuum expectation value of a gauge singlet scalar field changes appreciably during the electroweak phase…

高能物理 - 唯象学 · 物理学 2015-11-13 Jonathan Kozaczuk

We investigate the evolution of the electroweak phase transition, using a one-Higgs effective potential that can be regarded as an approximation for the Minimal Supersymmetric Standard Model. The phase transition occurs in a small interval…

高能物理 - 唯象学 · 物理学 2009-10-31 Ariel Megevand

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 the defect-mediated electroweak baryogenesis scenario, baryons are produced in well separated regions of space. It is shown that between the electroweak phase transition at a temperature of $T \sim 100 {\rm GeV}$ and the end of…

天体物理学 · 物理学 2010-11-01 Robert Brandenberger , Anne-Christine Davis , Martin J. Rees

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

It is widely believed that electroweak baryogenesis should be suppressed in strong phase transitions with fast-moving bubble walls, but this effect has never been quantitatively studied. We rederive fluid equations describing transport of…

高能物理 - 唯象学 · 物理学 2020-03-25 James M. Cline , Kimmo Kainulainen

One mechanism for generating a baryon asymmetry at the electroweak phase transition involves propagation of particle asymmetries generated by reflection from the bubble walls into the unbroken phase. Hitherto attention has focussed on top…

高能物理 - 唯象学 · 物理学 2010-11-01 Michael Joyce , Tomislav Prokopec , Neil Turok

A precise determination of the bubble wall velocity $v_w$ is crucial for making accurate predictions of the baryon asymmetry and gravitational wave (GW) signals in models of electroweak baryogenesis (EWBG). Working in the local thermal…

高能物理 - 唯象学 · 物理学 2025-08-19 Marcela Carena , Aurora Ireland , Tong Ou , Isaac R. Wang

I describe work done in collaboration with M. Joyce and K. Kainulainen on (1) the strength of the electroweak phase transition in the MSSM and (2) the mechanism for producing the baryon asymmetry during the phase transition. In the former…

高能物理 - 唯象学 · 物理学 2007-05-23 J. M. Cline

It now seems plausible that the observed baryon asymmetry may have been produced at the electroweak phase transition. We review the considerations which lead to this conclusion, focusing on the obstacles to making reliable estimates. These…

高能物理 - 唯象学 · 物理学 2008-02-03 Michael Dine

The dynamics of the electroweak phase transition in the early universe has profound implications for cosmology and particle physics. We systematically study the steady-state dynamics of bubble walls in scenarios where the transition is…

高能物理 - 唯象学 · 物理学 2025-08-07 Carlo Branchina , Angela Conaci , Stefania De Curtis , Luigi Delle Rose

The baryon density which may be produced during the electroweak phase transition in supersymmetric models is computed, taking into account the previously neglected effects of transport, strong and weak anomalous fermion number violation,…

高能物理 - 唯象学 · 物理学 2009-10-28 Patrick Huet , Ann E. Nelson

I describe work done in collaboration with M. Joyce and K. Kainulainen on (1) the strength of the electroweak phase transition in the MSSM and (2) the mechanism for producing the baryon asymmetry during the phase transition. In the former…

高能物理 - 唯象学 · 物理学 2016-10-26 J. M. Cline

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

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

The electroweak baryogenesis is studied in the charge transport mechanism with the vector-like quark model. Introducing an extra vector-like up-type quark and a singlet Higgs scalar with the mass of the order of a few hundred GeV, the…

高能物理 - 唯象学 · 物理学 2009-10-28 Tomoko Uesugi , Akio Sugamoto , Azusa Yamaguchi

Computing the properties of the bubble wall of a cosmological first order phase transition at electroweak scale is of paramount importance for the correct prediction of the baryon asymmetry of the universe and the spectrum of gravitational…

宇宙学与河外天体物理 · 物理学 2022-02-23 Marek Lewicki , Marco Merchand , Mateusz Zych
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