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相关论文: Baryon Asymmetry of Universe: View from Superfluid…

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The gapless fermionic excitations in superfluid 3He-A have a "relativistic" spectrum close to the gap nodes. They are the counterpart of the chiral particles (left-handed and right-handed) in high energy physics above the electroweak…

凝聚态物理 · 物理学 2009-10-31 G. E. Volovik

Superfluid 3He-A and high-temperature superconductors both have gapless fermionic quasiparticles with the "relativistic" spectrum close to the gap nodes. The interaction of these "relaitivistic" fermions with bosonic collective modes of the…

凝聚态物理 · 物理学 2007-05-23 G. E. Volovik

It is now well-recognized that the Universe may behave like a condensed matter system in which several phase transitions have taken place. Superconductors and the superfluid phases of 3He are condensed matter systems with useful…

凝聚态物理 · 物理学 2007-05-23 M. Krusius , T. Vachaspati , G. E. Volovik

Many direct parallels connect superfluid 3He with the field theories describing the physical vacuum, gauge fields and elementary fermions. Superfluid $^3$He exhibits a variety of topological defects which can be detected with single-defect…

凝聚态物理 · 物理学 2009-09-25 G. E. Volovik

We discuss the possibility of generating the baryon asymmetry of the Universe when the temperature of the Universe is much below the electroweak scale. In our model the evaporation of primordial black holes or the decay of massive particles…

高能物理 - 唯象学 · 物理学 2011-05-23 Raghavan Rangarajan , Supratim Sengupta , Ajit M. Srivastava , ;

As a result of the Standard Model chiral anomalies, baryon number is violated in the early universe in the presence of a hypermagnetic field with varying helicity. We investigate whether the matter / anti-matter asymmetry of the universe…

宇宙学与河外天体物理 · 物理学 2016-09-14 Kohei Kamada , Andrew J. Long

Superfluid phases of 3He are quantuim liquids with the interacting fermionic and bosonic fields. In many respects they can simulate the interacting quantum fields in the phyiscal vacuum. One can observe analogs of such phenomena as axial…

凝聚态物理 · 物理学 2011-04-20 G. E. Volovik

Although the origin of matter-antimatter asymmetry remains unknown, continuing advances in theory and improved experimental limits have ruled out some scenarios for baryogenesis, for example the sphaleron baryogenesis at the electroweak…

高能物理 - 唯象学 · 物理学 2008-11-26 Michael Dine , Alexander Kusenko

We present a new scenario for baryogenesis in the context of heterotic brane-world models. The baryon asymmetry of the universe is generated at a small-instanton phase transition which is initiated by a moving brane colliding with the…

高能物理 - 理论 · 物理学 2009-11-07 Mar Bastero-Gil , Edmund J. Copeland , James Gray , Andre Lukas , Michael Plumacher

The origin of the universal asymmetry between matter and antimatter remains a mystery. Electroweak baryogenesis is a well-motivated mechanism for generating the asymmetry dynamically, using interesting features of the Standard Model. In…

高能物理 - 唯象学 · 物理学 2025-08-14 Jorinde van de Vis , Jordy de Vries , Marieke Postma

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

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

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 describe a new effect which produces baryons at a first order electroweak phase transition. It operates when there is a CP-violating field present on propagating bubble walls. The novel aspect is that it involves a purely classical…

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

We calculate the baryon asymmetry of the Universe which would arise during a first order electroweak phase transition due to minimal standard model processes. It agrees in sign and magnitude with the observed baryonic excess, for resonable…

高能物理 - 唯象学 · 物理学 2010-11-01 Glennys R. Farrar , M. E. Shaposhnikov

We propose a scenario that generates the observed baryon asymmetry of the Universe through a multi--step phase transition in which SU(3) color symmetry is first broken and then restored. A spontaneous violation of $B-L$ conservation leads…

高能物理 - 唯象学 · 物理学 2018-07-26 Michael J. Ramsey-Musolf , Peter Winslow , Graham White

The origin of the matter-antimatter asymmetry of the universe is one of the major unsolved problems in cosmology and particle physics. In this paper, we investigate the recently proposed possibility that split fermion models -- extra…

高能物理 - 唯象学 · 物理学 2009-11-11 Andrew Coulthurst

One of the most experimentally testable explanations for the origin of the baryon asymmetry of the universe is that it was created during the electroweak phase transition, in the minimal supersymmetric standard model. Previous efforts have…

高能物理 - 唯象学 · 物理学 2008-11-26 James M. Cline , Kimmo Kainulainen

Baryon asymmetry of the universe is generated in the supersymmetric standard model (SSM) through the charge transport mechanism mediated by top squarks. Necessary CP violation originates from a complex phase contained in mass-squared…

高能物理 - 唯象学 · 物理学 2007-05-23 Mayumi Aoki , Noriyuki Oshimo

In principle, the baryon asymmetry of the Universe can be generated at the electroweak phase transition but the experimental lower limit on the Higgs mass seems to rule out a Standard Model scenario. However, it has been shown recently that…

高能物理 - 唯象学 · 物理学 2009-02-16 D. Delepine
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