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相关论文: Electroweak baryogenesis and primordial hypermagne…

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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

In models with the fundamental gravity scale in the TeV range, early cosmology is quite different from the standard picture, because the universe must have arisen at a much lower temperature and the electroweak symmetry was probably never…

高能物理 - 唯象学 · 物理学 2010-10-27 C. Bambi , A. D. Dolgov , K. Freese

We show how the temperature-dependent chiral vortical effect can generate hypermagnetic fields and matter-antimatter asymmetries, in the symmetric phase of the early Universe, in the temperature range $100\mbox{GeV} \le T\le 10\mbox{TeV}$,…

高能物理 - 唯象学 · 物理学 2025-04-11 S. Abbaslu , A. Rezaei , S. Rostam Zadeh , S. S. Gousheh

The presently observed cosmological baryon asymmetry has been finally determined at the time of the electroweak phase transition, when baryon and lepton number violating interactions fell out of thermal equilibrium. We discuss the…

高能物理 - 唯象学 · 物理学 2007-05-23 W. Buchmuller

We discuss the generation of the baryon asymmetry by a strong first order electroweak phase transition in the early universe, particularly in the context of the MSSM. This requires a thorough numerical treatment of the bubble wall profile…

高能物理 - 唯象学 · 物理学 2014-11-17 S. J. Huber , P. John , M. G. Schmidt

We show that in the presence of large scale primordial hypermagnetic fields, it is possible to generate a large amount of CP violation to explain the baryon to entropy ratio during the electroweak phase transition within the standard model.…

高能物理 - 唯象学 · 物理学 2007-05-23 Alejandro Ayala , Gabriel Pallares

Fluctuations of scalar fields produced at the stage of preheating after inflation are so large that they can break supersymmetry much stronger than inflation itself. These fluctuations may lead to symmetry restoration along flat directions…

高能物理 - 唯象学 · 物理学 2009-09-29 Greg. W. Anderson , Andrei Linde , Antonio Riotto

We compute the baryon asymmetry created in a tachyonic electroweak symmetry breaking transition, focusing on the dependence on the source of effective CP-violation. Earlier simulations of Cold Electroweak Baryogenesis have almost…

高能物理 - 唯象学 · 物理学 2018-07-04 Zong-Gang Mou , Paul M. Saffin , Anders Tranberg

It has been argued that any primordial B+L asymmetry existing at very high temperatures can be subsequently erased by anomalous electroweak effects. We argue that this is not necessarily the case in the supersymmetric standard model…

高能物理 - 唯象学 · 物理学 2010-11-01 Luis E. Ibanez , Fernando Quevedo

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

We address electroweak baryogenesis in the context of composite Higgs models, pointing out that modifications to the Higgs and top quark sectors can play an important role in generating the baryon asymmetry. Our main observation is that…

高能物理 - 唯象学 · 物理学 2015-05-30 Jose R. Espinosa , Ben Gripaios , Thomas Konstandin , Francesco Riva

The electroweak phase transition in a constant hypermagnetic field=A0 is studied in the Standard Model. The symmetry behaviour is investigated within the consistent effective potential of the scalar and magnetic fields at finite…

高能物理 - 唯象学 · 物理学 2007-05-23 Vladimir Skalozub , Vadim Demchik

We study the effect of damping on the generation of baryon asymmetry of the Universe in the standard model of the eletroweak theory with simple extensions of the Higgs sector. The propagation of quarks of masses up to about 5 GeV are…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Kundu , S. Mallik

We illustrate, via a simplified model, a scenario in which the baryon-asymmetry and, possibly the dark matter component of the Universe are simultaneously generated by the decay of a WIMP-like mother particle, in turn produced non-thermally…

高能物理 - 唯象学 · 物理学 2026-04-15 Giorgio Arcadi , Sarif Khan , Agnese Mariotti

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

In this letter we show that magnetic fields generated at the electroweak phase transition are most likely too weak to explain the void magnetic fields apparently observed today unless they have considerable helicity. We show that, in the…

宇宙学与河外天体物理 · 物理学 2016-01-15 Jacques M. Wagstaff , Robi Banerjee

We speculate that above or just below the electroweak phase transition magnetic fields are generated which have a net helicity (otherwise said, a Chern-Simons term) of order of magnitude $N_B + N_L$, where $N_{B,L}$ is the baryon or lepton…

高能物理 - 理论 · 物理学 2009-10-30 John M. Cornwall

We show that a spherical electroweak domain wall is formed around a small black hole and this is a general property of the Hawking radiation in the vacuum of the Standard Model. The wall appears not only for the first order phase transition…

高能物理 - 唯象学 · 物理学 2007-05-23 Yukinori Nagatani

Many models of baryogenesis rely on anomalous particle physics processes to give baryon number violation. By numerically evolving the electroweak equations on a lattice, we show that baryogenesis in these models creates helical cosmic…

天体物理学 · 物理学 2008-11-26 Craig J. Copi , Francesc Ferrer , Tanmay Vachaspati , Ana Achucarro

We analyze the nMSSM with CP violation in the singlet sector. We study the static and dynamical properties of the electroweak phase transition. We conclude that electroweak baryogenesis in this model is generic in the sense that if the…

高能物理 - 唯象学 · 物理学 2008-11-26 Stephan J. Huber , Thomas Konstandin , Tomislav Prokopec , Michael G. Schmidt