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We study the impact of flavour in thermal leptogenesis, including the quantum oscillations of the asymmetries in lepton flavour space. In the Boltzmann equations we find different numerical factors and additional terms which can affect the…

高能物理 - 唯象学 · 物理学 2009-11-11 A. Abada , S. Davidson , F-X. J. Michaux , M. Losada , A. Riotto

A large primordial lepton asymmetry can lead to successful baryogenesis by preventing the restoration of electroweak symmetry at high temperatures, thereby suppressing the sphaleron rate. This asymmetry can also lead to a first-order cosmic…

高能物理 - 唯象学 · 物理学 2025-08-29 Fei Gao , Julia Harz , Chandan Hati , Yi Lu , Isabel M. Oldengott , Graham White

The lepton asymmetry of order one is not excluded experimentally and, if present, can lead to interesting phenomena in the early Universe. It is shown that, when the temperature is above the quark-hadron transition, the lepton asymmetry…

高能物理 - 唯象学 · 物理学 2009-10-31 K. Zarembo

The relic cosmic background neutrinos accompanying the cosmic microwave background (CMB) photons may hide a universal lepton asymmetry orders of magnitude larger than the universal baryon asymmetry. At present, the only direct way to probe…

高能物理 - 唯象学 · 物理学 2008-11-26 Vimal Simha , Gary Steigman

The concept of lepton flavour universality (LFU), according to which the three lepton families are equivalent except for their masses, is a cornerstone prediction of the Standard Model (SM). LFU can be violated in models beyond the SM by…

高能物理 - 实验 · 物理学 2019-05-22 Elena Graverini

A large lepton number asymmetry of $\mathcal{O}(0.1-1)$ at present universe might not only be allowed but also necessary for consistency among cosmological data. We show that, if a sizeable lepton number asymmetry were produced before the…

高能物理 - 唯象学 · 物理学 2017-05-10 Gabriela Barenboim , Wan-Il Park

Cosmological baryon asymmetry B is studied in supersymmetric standard models, assuming the electroweak reprocessing of B and L. Only when the soft supersymmetry breaking is taken into account, B is proportional to the primordial B-L in the…

高能物理 - 唯象学 · 物理学 2009-10-22 T. Inui , T. Ichihara , Y. Mimura , N. Sakai

We study the impact of large lepton flavour asymmetries on the cosmic QCD transition. Scenarios of unequal lepton flavour asymmetries are observationally almost unconstrained and therefore open up a whole new parameter space for the cosmic…

高能物理 - 唯象学 · 物理学 2022-06-28 Mandy M. Middeldorf-Wygas , Isabel M. Oldengott , Dietrich Bödeker , Dominik J. Schwarz

The flavour lepton symmetry is gauged for both the Standard Model flavor group and its extension with three degenerate right-handed neutrinos. As a consequence of anomaly cancellation, exotic leptons are introduced which induce a see-saw…

高能物理 - 唯象学 · 物理学 2017-05-18 P. Quilez

A predictive Leptogenesis scenario is presented based on the Minimal Lepton Flavour Violation symmetry. In the realisation with three right-handed neutrinos transforming under the same flavour symmetry of the lepton electroweak doublets,…

高能物理 - 唯象学 · 物理学 2018-08-01 L. Merlo , S. Rosauro-Alcaraz

Recent observations of the cosmic microwave background (CMB) at smallest angular scales and updated abundances of primordial elements, indicate an increase of the energy density and the helium-4 abundance with respect to standard big bang…

宇宙学与河外天体物理 · 物理学 2013-03-19 Dominik J. Schwarz , Maik Stuke

We construct an extension of the Standard Model with a scalar leptoquark $\phi \sim (3,1,-\tfrac13)$ and the discrete flavour symmetry $G_f=D_{17}\times Z_{17}$ to explain anomalies observed in charged-current semi-leptonic $B$ meson decays…

高能物理 - 唯象学 · 物理学 2023-10-23 Innes Bigaran , Tobias Felkl , Claudia Hagedorn , Michael A. Schmidt

We show that the non-integer effective number of neutrinos $N^{\mathrm{eff}}_\nu$ can be understood as an effect of lepton $L$ asymmetry in the early Universe carried by the Dirac neutrino cosmic background. We show that…

高能物理 - 唯象学 · 物理学 2019-01-17 Cheng Tao Yang , Jeremiah Birrell , Johann Rafelski

We discuss charged lepton flavour violating processes such as mu -> e gamma in supersymmetric extensions of the Standard Model and in models with gauge-Higgs unification and a warped extra dimension. In both classes of models the processes…

高能物理 - 唯象学 · 物理学 2015-06-17 C. Hagedorn

It is shown that the mixing of lepton doublets of the Standard Model can yield sizeable contributions to the lepton asymmetry, that is generated through the decays of right-handed neutrinos at finite temperature in the early Universe. When…

高能物理 - 唯象学 · 物理学 2015-06-11 Bjorn Garbrecht

We discuss the bounds on the cosmological lepton number from Big Bang Nucleosynthesis (BBN), in light of recent evidences for a large value of the neutrino mixing angle theta13. The largest asymmetries for electron and muon or tau neutrinos…

高能物理 - 唯象学 · 物理学 2012-02-01 Gianpiero Mangano , Gennaro Miele , Sergio Pastor , Ofelia Pisanti , Srdjan Sarikas

A large primordial lepton asymmetry is capable of explaining the baryon asymmetry of the Universe (BAU) through suppression of the electroweak sphaleron rates (``sphaleron freeze-in") which can lead to a first-order cosmic QCD transition…

高能物理 - 唯象学 · 物理学 2023-09-06 Fei Gao , Julia Harz , Chandan Hati , Yi Lu , Isabel M. Oldengott , Graham White

Using a new sample of extremely metal poor systems, the EMPRESS survey has recently reported a primordial helium abundance that is $3\sigma$ smaller than the prediction from the standard big bang nucleosynthesis (BBN) scenario. This…

高能物理 - 唯象学 · 物理学 2023-03-08 Miguel Escudero , Alejandro Ibarra , Victor Maura

We argue that \Delta L=2 neutrino spin flavor precession, induced by the primordial magnetic fields, could have a significant impact on the leptogenesis process that accounts for the baryon asymmetry of the universe. Although the extra…

高能物理 - 唯象学 · 物理学 2015-06-05 Juan Barranco , Roberto Cota , David Delepine , Shaaban Khalil

We explore the possibility that the observed baryon asymmetry of the universe is the result of an earlier phase transition in which an extended gauge sector breaks down into the $SU(3)_C \times SU(2)_L \times U(1)_Y$ of the Standard Model.…

高能物理 - 唯象学 · 物理学 2008-11-26 Jing Shu , Tim M. P. Tait , Carlos E. M. Wagner