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相关论文: Macroscopic Forces driven by Resonant Neutrino Con…

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Using the exact propagators in a constant magnetic field, the neutrino self-energy has been calculated to all orders in the field strength $B$ within the minimal extension of the Weinberg-Salam model with massive Dirac neutrinos. A neutrino…

高能物理 - 唯象学 · 物理学 2020-11-03 Andrea Erdas , Zachary Metzler

With the recent findings from various astrophysical results hinting towards possible existence of strange quark matters with the baryonic resonances such as $\Lambda^0, \Sigma^0, \Xi, \Omega$ in the core of neutron stars, we investigate the…

高能物理 - 唯象学 · 物理学 2022-08-18 Hiranmaya Mishra , Prasanta K. Panigrahi , Sudhanwa Patra , Utpal Sarkar

The results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed. The data concern different event topologies with average neutrino energies of ~ 4 and ~ 50 GeV. The Multiple Coulomb Scattering of muons…

高能物理 - 实验 · 物理学 2019-08-14 G. Giacomelli

We discuss the effects of resonant $\nu_e \to \nu_s$ and $\bar{\nu}_e \to \bar{\nu}_s$ ($\nu_s$ is a sterile neutrino) conversions in the dense medium of a supernova. In particular, we assume the sterile neutrino $\nu_s$ to be in the hot…

高能物理 - 唯象学 · 物理学 2009-09-17 H. Nunokawa , J. T. Peltoniemi , A. Rossi , J. W. F. Valle

Radiative transition of massless neutrino $\nu_l \to \nu_l + \gamma$ ($l = e, \mu, \tau$) in a strong magnetic field is investigated in the framework of the Standard Model. The process probability and the mean values of the neutrino energy…

高能物理 - 唯象学 · 物理学 2007-05-23 A. A. Gvozdev , N. V. Mikheev , L. A. Vassilevskaya

The exchange of a pair of low-mass neutrinos between electrons, protons and neutrons produces a "long-range" $1/r^5$ potential, which can be sought for in phenomena originating on the atomic and sub-atomic length scales. We calculate the…

原子物理 · 物理学 2018-06-06 Yevgeny V. Stadnik

This talk summarizes the results of recent calculations of how fluctuations within the solar medium can influence resonant neutrino oscillations within the sun. Although initial calculations pointed to helioseismic waves as possibly…

高能物理 - 唯象学 · 物理学 2009-10-30 C. P. Burgess

Physics potential of future measurements of atmospheric neutrinos is explored. Observation of $\Delta m^2_{21}$ driven sub-dominant effects and $\theta_{13}$ driven large matter effects in atmospheric neutrinos can be used to study the…

高能物理 - 唯象学 · 物理学 2007-05-23 Sandhya Choubey

Non-standard interactions (NSI) of neutrinos with matter mediated by a scalar field would induce medium-dependent neutrino masses which can modify oscillation probabilities. Generating observable effects requires an ultra-light scalar…

高能物理 - 唯象学 · 物理学 2020-06-03 K. S. Babu , Garv Chauhan , P. S. Bhupal Dev

Positive evidence for neutrino oscillations is mounting from the solar and atmospheric neutrino anomalies and the LSND experiment. Accordingly, the neutrino mass differences appear to lie in the sub-eV range and at least some of the mixing…

高能物理 - 唯象学 · 物理学 2007-05-23 G. Raffelt

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

Do neutrinos have nonzero masses? If they do, then these masses are very tiny, and can be sought only in very sensitive experiments. The most sensitive of these search for neutrino oscillation, a quantum interference effect which requires…

高能物理 - 唯象学 · 物理学 2017-08-23 Boris Kayser

We consider neutrinos with varying masses which arise in scenarios relating neutrino masses to the dark energy density in the universe. We point out that the neutrino mass variation can lead to level crossing and thus a cosmo MSW effect,…

天体物理学 · 物理学 2008-11-26 Pham Quang Hung , Heinrich Päs

Neutrinos dominate the energetics of core-collapse supernovae, and are believed to play an important role in driving the explosion. The development of a spatially multidimensional neutrino radiative transfer code is a key part of the…

天体物理学 · 物理学 2007-05-23 Christian Y. Cardall

We consider the matter effects on neutrinos moving in background on the basis of the corresponding quantum wave equations. Both Dirac and Majorana neutrino cases are discussed. The effects for Dirac neutrino reflection and trapping as well…

高能物理 - 唯象学 · 物理学 2008-11-26 Alexander Grigoriev , Alexander Studenikin , Alexei Ternov

In astrophysical environments such as core-collapse supernovae and neutron star-neutron star or neutron star-black hole mergers where dense neutrino media are present, matter-neutrino resonances (MNRs) can occur when the neutrino…

高能物理 - 唯象学 · 物理学 2015-11-24 Meng-Ru Wu , Huaiyu Duan , Yong-Zhong Qian

This talk summarizes our recent work which studied the impact of resonant neutrino conversion induced by some non-standard neutrino properties beyond mass and mixing, such as neutrino magnetic moment, lepton-flavor non-universality as well…

高能物理 - 唯象学 · 物理学 2007-05-23 Hiroshi Nunokawa

Astrophysical implications of neutrino mass and mixings are discussed. The status of solar and atmospheric neutrino problems, and recent developments concerning nuclear physics input to solar models and solar opacities are reviewed.…

高能物理 - 唯象学 · 物理学 2009-10-28 A. B. Balantekin

A review of the problem of neutrino mass, mixing and oscillations is given. Possible phenomenological schemes of neutrino mixing are discussed. The most important consequences of neutrino mixing--neutrino oscillations are considered in some…

高能物理 - 唯象学 · 物理学 2007-05-23 W. M. Alberico , S. M. Bilenky

We investigate the effects of random density fluctuations on neutrino oscillations in the Sun environment. We show how the average of certain quantities which can be used to describe the MSW effect can be computed analytically. We examine…

高能物理 - 唯象学 · 物理学 2016-09-01 Emilio Torrente-Lujan