English
Related papers

Related papers: Supernova deleptonization asymmetry: Impact on sel…

200 papers

We report results of the first 3-by-3 "multi-angle" simulation of the evolution of neutrino flavor in the core collapse supernova environment. In particular, we follow neutrino flavor transformation in the neutronization neutrino burst of…

High Energy Astrophysical Phenomena · Physics 2010-11-11 John F. Cherry , George M. Fuller , Joe Carlson , Huaiyu Duan , Yong-Zong Qian

We discuss the predictive power of supersymmetric models with flavor symmetries, focusing on the lepton sector of the standard model. In particular, we comment on schemes in which, after certain `flavons' acquire their vacuum expectation…

High Energy Physics - Phenomenology · Physics 2013-02-27 Mu-Chun Chen , Maximilian Fallbacher , Michael Ratz , Christian Staudt

The gauge interactions of any supersymmetric extension of the standard model involve new flavor mixing matrices. The assumptions involved in the construction of minimal supersymmetric models, both $SU(3) \times SU(2) \times U(1)$ and grand…

High Energy Physics - Phenomenology · Physics 2009-10-28 Nima Arkani-Hamed , Hsin-Chia Cheng , L. J. Hall

The Daya Bay Collaboration has recently observed neutrino oscillations in the nu_e-bar -> nu_e-bar disappearance channel, indicating that sin^2 theta_13 = 0.024 +(-) 0.005 (1 sigma) and theta_13 = 0 is already excluded at the 5.2 sigma…

High Energy Physics - Phenomenology · Physics 2012-05-04 Shun Zhou

We study the role of a very general type of flavor symmetry in controlling the strength of R-parity violation in supersymmetric models. We assume that only leptons are charged under a global symmetry whose breaking induces lepton number…

High Energy Physics - Phenomenology · Physics 2013-05-29 Gautam Bhattacharyya , Heinrich Päs , Daniel Pidt

Fast neutrino-flavor conversion (FFC) can nontrivially alter neutrino radiation field in core-collapase supernovae (CCSN) and binary neutron-star merger (BNSM) remnants. However, its interplay with global geometry remains poorly understood…

High Energy Astrophysical Phenomena · Physics 2026-04-16 Masamichi Zaizen , Hiroki Nagakura

At the present time even the most sophisticated, multi-dimensional simulations of core-collapse supernovae do not (self-consistently) include neutrino flavor transformation. This physics is missing despite the importance of neutrinos in the…

High Energy Astrophysical Phenomena · Physics 2020-10-14 Charles J. Stapleford , Carla Fröhlich , James P. Kneller

We show that interactions violating the conservation of lepton numbers in the neutrino sector could significantly alter the standard low entropy picture for the pre-supernova collapsing core of a massive star. A rapid neutrino-antineutrino…

High Energy Physics - Phenomenology · Physics 2025-06-23 Anna M. Suliga , Patrick Chi-Kit Cheong , Julien Froustey , George M. Fuller , Lukáš Gráf , Kyle Kehrer , Oliver Scholer , Shashank Shalgar

After confirmation of massiveness and mixing of neutrinos, by neutrino oscillation data, the origin of neutrino mass and the occurrence of charged-lepton-flavor non-conservation in nature have become two main objectives for the physics of…

High Energy Physics - Phenomenology · Physics 2026-02-05 Adrián González-Quiterio , Héctor Novales-Sánchez

We investigate collective flavor oscillations of supernova neutrinos at late stages of the explosion. We first show that the frequently used single-angle (averaged coupling) approximation predicts oscillations close to, or perhaps even…

High Energy Physics - Phenomenology · Physics 2011-04-21 Huaiyu Duan , Alexander Friedland

Collective flavor transformations in supernovae, caused by neutrino-neutrino interactions, are essentially a two-flavor phenomenon driven by the atmospheric mass difference and the small mixing angle theta_13. In the two-flavor…

High Energy Physics - Phenomenology · Physics 2010-04-29 Basudeb Dasgupta , Georg G. Raffelt , Irene Tamborra

We address the recent anomalies in semi-leptonic $B$-meson decays using a model of fermion masses based on the $U(2)$ flavor symmetry. The new contributions to $b \to s \ell \ell$ transitions arise due to a tree-level exchange of a…

High Energy Physics - Phenomenology · Physics 2016-01-20 Adam Falkowski , Marco Nardecchia , Robert Ziegler

Lepton flavour violation (LFV) is one of the most trending topics to probe new physics (NP). The powerful accelerators have enhanced their intensities to observe the LFV decays very precisely. In this situation, the theorists are also…

High Energy Physics - Phenomenology · Physics 2023-12-05 S. Biswas , M. Mandal , S. Mahata , S. Sahoo

We consider lepton flavor violations (LFV) mediated by photino as a result of the nondiagonal slepton mass matrices in general supersymmetric models. Using the experimental upper bounds on l \to l' + gamma and mu^- + Ti \to e^- + Ti as…

High Energy Physics - Phenomenology · Physics 2009-10-31 Yeong Gyun Kim , Pyungwon Ko , Jae Sik Lee , Kang Young Lee

The neutrino fast flavor instability dominates the evolution of neutrino flavor within the engines of core-collapse supernovae and neutron star mergers. However, theoretical models of neutrino flavor change that include many-body quantum…

High Energy Astrophysical Phenomena · Physics 2026-05-22 Zoha Laraib , Sherwood Richers

Lepton flavor violation in various sectors of the theory can bring important effects on neutrino masses and mixing through wave function renormalization. We examine general conditions for flavor structure of radiative corrections producing…

High Energy Physics - Phenomenology · Physics 2011-07-19 Eung Jin Chun

We show that in a large class of models based on anomalous U(1) symmetry which addresses the fermion mass hierarchy problem, leptonic flavor changing processes are induced that are in the experimentally interesting range. The flavor…

High Energy Physics - Phenomenology · Physics 2015-06-25 K. S. Babu , Ts. Enkhbat , I. Gogoladze

The heavy right-handed neutrinos in supersymmetric models can act as the source of lepton flavor violation (LFV). LFV processes like $ \mu \rightarrow e \gamma $, $ \tau \rightarrow \mu \gamma $, $ \tau \rightarrow e \gamma $ is an…

High Energy Physics - Phenomenology · Physics 2020-04-03 Gayatri Ghosh

A dense neutrino gas exhibiting angular crossings in the electron lepton number is unstable and develops fast flavor conversions. Instead of assuming an unstable configuration from the onset, we imagine that the system is externally driven…

High Energy Physics - Phenomenology · Physics 2024-12-11 Damiano F. G. Fiorillo , Georg Raffelt

In core-collapse supernovae, the nu_e and anti-nu_e species may experience collective flavor swaps to non-electron species nu_x, within energy intervals limited by relatively sharp boundaries ("splits"). These phenomena appear to depend…

High Energy Physics - Phenomenology · Physics 2009-12-10 Gianluigi Fogli , Eligio Lisi , Antonio Marrone , Irene Tamborra