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We propose a new mechanism for late cosmological baryon asymmetry in models with first order electroweak phase transition. Lepton asymmetry arises through the decay of particles produced out of equilbrium in bubble collisions and is…

高能物理 - 唯象学 · 物理学 2011-07-19 Antonio Masiero , Antonio Riotto

We consider a minimal extension of the Standard Model with one singlet neutrino per generation that can realize resonant leptogenesis at the electroweak scale. In particular, the baryon asymmetry in the Universe can be created by resonant…

高能物理 - 唯象学 · 物理学 2009-11-10 Apostolos Pilaftsis

We study a new scenario for baryogenesis due to the spontaneous breaking of the $CPT$ invariance through the interaction between a baryon current and a hypermagnetic helicity. The hypermagnetic helicity (Chern-Simons number) of $U(1)_Y$…

高能物理 - 唯象学 · 物理学 2008-11-26 Kazuharu Bamba , C. Q. Geng , S. H. Ho

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

We show that a simple supersymmetric $U(1)_{B-L}$ extension of the standard model can explain simultaneously the large electron neutrino asymmetry hinted by the recent EMPRESS data as well as the observed tiny baryon number asymmetry via…

高能物理 - 唯象学 · 物理学 2025-09-17 Kyu Jung Bae , Arghyajit Datta , Rinku Maji , Wan-Il Park

We estimate the Baryon Asymmetry of the Universe (BAU) produced in an inverse seesaw model containing extra light singlets, and with lepton number conservation prior to the electroweak phase transition. An order one CP asymmetry epsilon is…

高能物理 - 唯象学 · 物理学 2015-06-11 Sacha Davidson , Martin Elmer

It is shown that late-time decay of domain walls can dilute unwanted relics such as moduli, if the universe was dominated by frustrated domain walls with tension $\sigma = (1 - 100 TeV)^3$. Since energy density of the frustrated domain…

高能物理 - 唯象学 · 物理学 2009-11-10 Masahiro Kawasaki , Fuminobu Takahashi

The observed baryon asymmetry of the Universe is suitably created in thermal leptogenesis through the out-of-equilibrium decay of $N_1$, the lightest of the three heavy singlet neutral fermions which anchor the seesaw mechanism to obtain…

高能物理 - 唯象学 · 物理学 2007-05-23 Ernest Ma , Narendra Sahu , Utpal Sarkar

We propose a new mechanism to generate baryons. Electroweak strings produced at the electroweak phase transition will introduce anomalous currents through interactions of the strings with the background electromagnetic field and through…

高能物理 - 唯象学 · 物理学 2009-12-30 M. Barriola

We propose a mechanism called axiogenesis where the cosmological excess of baryons over antibaryons is generated from the rotation of the QCD axion. The Peccei-Quinn (PQ) symmetry may be explicitly broken in the early universe, inducing the…

高能物理 - 唯象学 · 物理学 2020-04-01 Raymond T. Co , Keisuke Harigaya

Generating axion dark matter through the kinetic misalignment mechanism implies the generation of large asymmetries for Standard Model fermions in the early universe. Even if these asymmetries are washed out at later times, they can trigger…

高能物理 - 唯象学 · 物理学 2023-08-09 Raymond T. Co , Valerie Domcke , Keisuke Harigaya

We investigate the feasibility of directly detecting a generation mechanism of the cosmic baryon asymmetry, by repeating the same particle physics process inside the LHC. We propose a framework with R-parity and CP violating squark decays…

高能物理 - 唯象学 · 物理学 2013-10-25 Haipeng An , Yue Zhang

A cosmological pseudoscalar field coupled to hypercharge topological number density can exponentially amplify hyperelectric and hypermagnetic fields while coherently rolling or oscillating, leading to the formation of a time-dependent…

高能物理 - 唯象学 · 物理学 2009-10-31 Ram Brustein , David H. Oaknin

We study domain walls (DWs) arising in field theories where $Z_2$-symmetry is spontaneously broken by a scalar expectation value decreasing proportionally to the Universe temperature. The energy density of such melting DWs redshifts…

高能物理 - 唯象学 · 物理学 2025-02-27 I. Dankovsky , S. Ramazanov , E. Babichev , D. Gorbunov , A. Vikman

We examine two semi-analytical methods for estimating the baryon asymmetry of the universe (BAU) generated in scenarios of ``local'' electroweak baryogenesis (in which the requisite baryon number violation and CP violation occur together in…

高能物理 - 唯象学 · 物理学 2016-08-24 Arthur Lue , Krishna Rajagopal , Mark Trodden

We consider the scenario of electroweak baryogenesis mediated by cosmological defects in a model of extra dimension. We consider the domain wall on the brane in higher-dimensional theories.The electroweak breaking scale is suppressed and…

高能物理 - 唯象学 · 物理学 2007-05-23 Tomohiro Matsuda

CP violation and the violation of baryon-minus-lepton number B-L do not necessarily have to occur simultaneously in order to accomplish successful leptogenesis. Instead, it suffices if new CP-violating interactions at high energies result…

高能物理 - 唯象学 · 物理学 2023-02-07 Valerie Domcke , Kohei Kamada , Kyohei Mukaida , Kai Schmitz , Masaki Yamada

We explore the spontaneous breaking of global baryon number for baryogenesis. We introduce a model with three majorana fermions and a complex scalar carrying baryon number charge. After symmetry breaking, the baryon asymmetry is generated…

高能物理 - 唯象学 · 物理学 2025-04-21 Pedro Bittar , Gustavo Burdman , Gabriel M. Salla

We show that an axionlike particle (ALP) naturally implements spontaneous electroweak baryogenesis through a cosmic evolution strongly tied to the electroweak phase transition (EWPT) if it feebly couples to the Higgs field while giving a…

高能物理 - 唯象学 · 物理学 2022-03-14 Sang Hui Im , Kwang Sik Jeong , Yeseong Lee

The energy levels of the left and the right handed neutrinos is split in the background of gravitational waves generated during inflation which in presence of lepton number violating interactions gives rise to a net lepton asymmetry at…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Subhendra Mohanty , A. R. Prasanna , G. Lambiase