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We examine simulations of core-collapse supernovae in spherical symmetry. Our model is based on general relativistic radiation hydrodynamics with three-flavor Boltzmann neutrino transport. We discuss the different supernova phases,…

高能天体物理现象 · 物理学 2012-01-04 T. Fischer , M. Liebendörfer , F. -K. Thielemann , G. Martínez-Pinedo , B. Ziebarth , K. Langanke

In supersymmetric (SUSY) models the misalignment between fermion and sfermion families introduces unsuppressed flavor-changing processes. Even if the mass parameters are chosen to give no flavor violation, family dependent radiative…

高能物理 - 唯象学 · 物理学 2007-05-23 J. I. Illana , M. Masip

We investigate the collective neutrino oscillations under the three flavor multi-angle approximation in a spherically symmetric simulation of failed supernovae. A failed supernova emits high neutrino fluxes in a short time, while intense…

高能天体物理现象 · 物理学 2018-12-19 Masamichi Zaizen , Takashi Yoshida , Kohsuke Sumiyoshi , Hideyuki Umeda

Predicting the flavor composition of neutrinos from supernovae is a challenging task, primarily due to the high neutrino densities at their core. In such an environment, neutrino self-interactions give rise to collective effects that have…

高能物理 - 唯象学 · 物理学 2025-06-03 Antonio Capanema , Yago Porto , Maria Manuela Saez

When the neutrino density is very high, as in core-collapse supernovae, neutrino-neutrino interactions are not negligible and can appreciably affect the evolution of flavour. The physics of these phenomena is briefly highlighted, and their…

高能物理 - 唯象学 · 物理学 2009-05-18 Irene Tamborra

Neutrino flavor evolution inside a core-collapse supernova is a topic of active research. The core of a supernova is an intense source of neutrinos and antineutrinos. Self-interaction among neutrinos (as well as antineutrinos) gives rise to…

高能天体物理现象 · 物理学 2025-02-20 Indrajit Ghose , Amitabha Lahiri

Supersymmetric theories generally have new flavor violation sources in the squark and slepton mass matrices. If significant lepton flavor violation exists, selectron and smuon should be nearly degenerate. This leads to the phenomenon of…

高能物理 - 唯象学 · 物理学 2007-05-23 Hsin-Chia Cheng

The timescale of de-leptonization by neutrino loss and associated contraction of a proto-neutron star is short compared to the time to progagate a shock through the helium core of a massive star, and so the de-leptonization phase does not…

天体物理学 · 物理学 2008-11-26 J. Craig Wheeler , Shizuka Akiyama

Complementary to high-energy experimental efforts, indirect astrophysical searches of particles beyond the standard model have long been pursued. The present article follows the latter approach and considers, for the first time, the…

高能天体物理现象 · 物理学 2025-01-15 Tobias Fischer , Jorge Martin Camalich , Hristijan Kochankovski , Laura Tolos

Flavor-dependent neutrino emission is critical to the evolution of a supernova and its neutrino signal. In the dense anisotropic interior of the star, neutrino-neutrino forward-scattering can lead to fast collective neutrino oscillations,…

高能物理 - 唯象学 · 物理学 2021-02-22 Soumya Bhattacharyya , Basudeb Dasgupta

Dirac leptogenesis (or Dirac neutrinogenesis), in which neutrinos are purely Dirac particles, is an interesting alternative to the standard leptogenesis scenario. In its supersymmetric version, the modified form of the superpotential…

高能物理 - 唯象学 · 物理学 2008-11-26 Brooks Thomas , Manuel Toharia

Supernova neutrinos can exhibit a rich variety of flavor conversion mechanisms. In particular, they can experience "fast" self-induced flavor conversions almost immediately above the core. Very recently, a novel method has been proposed to…

高能物理 - 唯象学 · 物理学 2017-09-13 Francesco Capozzi , Basudeb Dasgupta , Eligio Lisi , Antonio Marrone , Alessandro Mirizzi

We examine coherent active-active channel neutrino flavor evolution in environments where neutrino-neutrino forward scattering can engender large-scale collective flavor transformation. We point out a key quantity, the "total effective…

天体物理学 · 物理学 2008-11-26 Huaiyu Duan , George M. Fuller , Yong-Zhong Qian

A core-collapse supernova (SN) releases almost all of its energy in the form of neutrinos, which provide a unique opportunity to probe the working machinery of a SN. These sites are prone to neutrino-neutrino refractive effects, which can…

高能物理 - 唯象学 · 物理学 2024-06-03 Manibrata Sen

We perform numerical simulations of fast collective neutrino flavor conversions in an one-dimensional box mimicking a system with the periodic boundary condition in one spatial direction and translation symmetry in the other two dimensions.…

高能物理 - 唯象学 · 物理学 2021-11-09 Meng-Ru Wu , Manu George , Chun-Yu Lin , Zewei Xiong

We study the effects of non-standard self-interactions (NSSI) of neutrinos streaming out of a core-collapse supernova. We show that with NSSI, the standard linear stability analysis gives rise to linearly as well as exponentially growing…

高能物理 - 唯象学 · 物理学 2018-02-21 Amol Dighe , Manibrata Sen

Neutrino self-interactions are known to lead to non-linear collective flavor oscillations in a core-collapse supernova. We point out new possible effects of non-standard self-interactions (NSSI) of neutrinos on flavor conversions in a…

高能物理 - 唯象学 · 物理学 2017-06-05 Anirban Das , Amol Dighe , Manibrata Sen

The minimal supersymmetric standard model with a low scale see-saw mechanism is presented. Within this framework, the lepton flavour violation in the charged lepton sector is thoroughly studied. Special attention is paid to the individual…

高能物理 - 唯象学 · 物理学 2013-12-05 Luka Popov

We explore the implications of symmetries that remain unbroken at the self-dual point $\tau=i$ in modular invariant theories. Assuming that (a) the three generations of lepton doublets transform as an irreducible representation of a finite…

高能物理 - 唯象学 · 物理学 2024-10-02 Monal Kashav , Ketan M. Patel

Charged-current neutrino processes such as $\nu_e + n \rightleftharpoons p + e^-$ and $\bar\nu_e + p \rightleftharpoons n + e^+$ destroy the flavor coherence among the weak-interaction states of a single neutrino and thus damp its flavor…

高能物理 - 唯象学 · 物理学 2023-10-04 Zewei Xiong , Lucas Johns , Meng-Ru Wu , Huaiyu Duan