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相关论文: Neutrino oscillations in low density medium

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We present compact analytic expressions for 3-flavor neutrino oscillation probabilities with invisible neutrino decay, where matter effects have been explicitly included. We take into account the possibility that the oscillation and decay…

高能物理 - 唯象学 · 物理学 2023-01-18 Dibya S. Chattopadhyay , Kaustav Chakraborty , Amol Dighe , Srubabati Goswami

Because the propagation of neutrinos is affected by the presence of Earth matter, it opens new possibilities to probe the Earth's interior. Different approaches range from techniques based upon the interaction of high energy (above TeV)…

地球物理 · 物理学 2008-11-26 Walter Winter

We examine scenarios in which a dark sector (dark matter, dark radiation, or dark energy) couples to the active neutrinos. For light and weakly-coupled exotic sectors we find that scalar, vector, or tensor dark backgrounds may appreciably…

高能物理 - 唯象学 · 物理学 2018-07-18 Francesco Capozzi , Ian M. Shoemaker , Luca Vecchi

Oscillations of three neutrinos with all squared mass splittings around 10^{-3} eV^2 are not firmly excluded by solar neutrino experiments. We carefully verify that they are also perfectly compatible with atmospheric neutrino experiments:…

高能物理 - 唯象学 · 物理学 2009-10-31 Alessandro Strumia

We study flavor oscillations of low energy neutrinos propagating in dense matter of a rotating neutron star. On the basis of the exact solutions of the wave equations for neutrinos mass eigenstates we derive the transition probability for…

高能物理 - 唯象学 · 物理学 2017-08-23 Maxim Dvornikov

The effects originated in dispersion with time on spreading of wave packets for the time-integrated two-flavor neutrino oscillation probabilities in vacuum are studied in the context of a field theory treatment. The neutrino flavor states…

高能物理 - 唯象学 · 物理学 2014-01-10 Y. F. Perez , C. J. Quimbay

When neutrinos travel through matter with a periodic density profile, the neutrino oscillation probability can be enhanced if certain conditions are satisfied. In a two-neutrino framework, the condition for parametric resonance is known.…

高能物理 - 唯象学 · 物理学 2015-06-23 Kara M. Merfeld , David C. Latimer

The complete description of neutrino oscillations require the wave packet treatment. For terrestrial experiments the contribution from the interaction of neutrino with the Earth matter would modify oscillation pattern, i.e., the dependence…

高能物理 - 唯象学 · 物理学 2012-06-06 Nan Qin , Bo-Qiang Ma

We point out that the measurement of the $L/E$ distribution of atmospheric neutrino events with sufficient resolution in order to observe the characteristic modulations of neutrino oscillations would provide a unique way to test the…

高能物理 - 唯象学 · 物理学 2007-05-23 G. Mannocchi , L. Periale , P. Picchi , F. Pietropaolo , S. Ragazzi , A. Rubbia

There are several new features in production, oscillations and detection of the atmospheric neutrinos of low energies, E<100 MeV. The flavor ratio, r, of muon to electron neutrino fluxes is substantially smaller than 2 and decreases with…

高能物理 - 唯象学 · 物理学 2009-06-30 O. L. G. Peres , A. Yu. Smirnov

The dispersion relation of energetic (few TeV) neutrinos traversing a medium is studied. We use the real time formalism of thermal field theory and we include the effects from the propagator of the W gauge boson. We consider then the MSW…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Nicolaidis , G. Tsirigoti , J. Hansson

We calculate matter effects on neutrino oscillations relevant for long baseline experiments. In particular, we compare the results obtained with constant density along the neutrino path versus results obtained by incorporating the actual…

高能物理 - 唯象学 · 物理学 2009-10-31 Irina Mocioiu , Robert Shrock

We focus on the implications of the oscillations for the shape of nuclear beta-spectrum (=direct search for nu mass). This is of interest because of the existing bound, m_(nu_e)<2.2 eV, that could improve by one order of magnitude with…

高能物理 - 唯象学 · 物理学 2009-10-31 Francesco Vissani

We examine the general structure of the formulae of neutrino oscillations proposed by Blasone and Vitiello(BV). Reconstructing their formulae with the retarded propagators of the flavor neutrino fields for the case of many flavors, we can…

高能物理 - 唯象学 · 物理学 2009-11-07 K. Fujii , C. Habe , T. Yabuki

The neutrinos from a Type II supernova provide perhaps our best opportunity to probe cosmologically interesting muon and/or tauon neutrino masses. This is because matter enhanced neutrino oscillations can lead to an anomalously hot nu_e…

天体物理学 · 物理学 2010-12-02 G. M. Fuller , W. C. Haxton , G. C. McLaughlin

We adapt to neutrino physics a general formulation for particle propagation in fluctuating media, initially developed for applications to electromagnetism and neutron optics. In leading approximation this formalism leads to the usual MSW…

高能物理 - 唯象学 · 物理学 2014-11-17 C. P. Burgess , D. Michaud

During a period of about two decades we have realized a programme of systematic investigations of different aspects of neutrino propagation in extreme external environments and have predicted and studied several new phenomena that are…

高能物理 - 唯象学 · 物理学 2020-09-04 Alexander Studenikin

We consider two-family neutrino oscillations in a medium of continuously-varying density as a limit of the process in a series of constant-density layers. We construct analytic expressions for the conversion amplitude at high energies…

高能物理 - 唯象学 · 物理学 2008-11-26 Paul M. Fishbane , Peter Kaus

We show how two different scales for oscillations between $e$ and $\mu$ neutrinos, characterized by different mixing angles and effective mass scales, can arise in a simple and theoretically attractive framework. One scale characterizes…

高能物理 - 唯象学 · 物理学 2011-05-12 K. S. Babu , Jogesh C. Pati , Frank Wilczek