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相关论文: Neutrino Propagation Through Helioseismic Waves

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In this talk I summarize recent work done in collaboration with Cliff Burgess and Denis Michaud, in which we performed a detailed investigation of how solar neutrinos propagate through helioseismic waves. We find that the MSW solar neutrino…

高能物理 - 唯象学 · 物理学 2016-09-06 P. Bamert

We summarize a general formulation of particle propagation in fluctuating media, as applied to the description of neutrino propagation through the sun. It contains the familiar MSW effective hamiltonian, plus corrections which describe…

高能物理 - 唯象学 · 物理学 2007-05-23 C. P. Burgess , D. Michaud

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

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

This review has two parts. The first part summarizes the current observational constraints on fluctuations in the solar medium deep within the solar Radiative Zone, and shows how the KamLAND and SNO-salt data combine to make the…

高能物理 - 唯象学 · 物理学 2007-05-23 C. P. Burgess N. S. Dzhalilov , M. Maltoni , T. I. Rashba , V. B. Semikoz , M. Tortola , J. W. F. Valle

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

We study the effect of random matter density fluctuations in the sun on resonant neutrino conversion in matter by solving numerically the evolution equation for the neutrino system including the full effect of the random matter density…

高能物理 - 唯象学 · 物理学 2007-05-23 A. A. Bykov , M. C. Gonzalez-Garcia , C. Peña-Garay , V. Yu. Popov , V. B. Semikoz

The description of neutrino propagation through a fluctuating medium is summarized. Fluctuation-Dissipation-Theorem arguments relate microscopic fluctuations to thermodynamic quantities, allowing these to be very generally studied in…

高能物理 - 唯象学 · 物理学 2016-09-06 C. P. Burgess

We present the evolution equation describing MSW conversion, derived in the framework of the Schr\"odinger approach, in the presence of matter density fluctuations. Then we analyse the effect of such fluctuations in the MSW scenario as a…

高能物理 - 唯象学 · 物理学 2009-10-28 Anna Rossi

The generalized dynamics describing the propagation of neutrinos in randomly fluctuating media is analyzed: it takes into account matter-induced, decoherence phenomena that go beyond the standard MSW effect. A widely adopted density…

高能物理 - 唯象学 · 物理学 2009-11-10 F. Benatti , R. Floreanini

We consider the effect on matter-enhanced neutrino flavor transformation of a randomly fluctuating, delta-correlated matter density. The fluctuations will produce a distribution of neutrino survival probabilities. We find the mean and…

天体物理学 · 物理学 2008-11-26 A. B. Balantekin , J. M. Fetter , F. N. Loreti

Gravitational waves (GWs) can alter the neutrino propagation distance and thus affect neutrino oscillations. This can result in a complete disappearance of the oscillatory behavior that competes with other sources of neutrino decoherence.…

高能物理 - 唯象学 · 物理学 2024-11-12 Dominik Hellmann , Sara Krieg , Heinrich Päs , Mustafa Tabet

We present a theory of neutrino oscillations in a dense medium which goes beyond the effective matter potential used in the description of the MSW effect. We show how the purity of the neutrino state is degraded by neutrino interactions…

高能物理 - 唯象学 · 物理学 2021-07-20 Antonio Capolupo , Salvatore Marco Giampaolo , Aniello Quaranta

We develop the Redfield equation for delta-correlated gaussian noise and apply it to the case of two neutrino flavor or spin precession in the presence of a noisy matter density or magnetic field, respectively. The criteria under which…

核理论 · 物理学 2009-12-30 F. N. Loreti , A. B. Balantekin

We study the effect of coherent and incoherent broadening on neutrino oscillations both in vacuum and in the presence of matter (the MSW effect). We show under very general assumptions that it is not possible to distinguish experimentally…

高能物理 - 唯象学 · 物理学 2009-10-28 Ken Kiers , Shmuel Nussinov , Nathan Weiss

We present a generalization of the resonant neutrino conversion in matter, including a random component in the matter density profile. The study is focused on the effect of such matter perturbations upon both large and small mixing angle…

高能物理 - 唯象学 · 物理学 2007-05-23 H. Nunokawa , A. Rossi , V. B. Semikoz , J. W. F. Valle

Helioseismology has provided very precise information about the solar internal sound speed and density throughout most of the solar interior. The results are generally quite close to the properties of standard solar models. Since the solar…

天体物理学 · 物理学 2007-05-23 J. Christensen-Dalsgaard

We present a generalization of the resonant neutrino conversion in matter, including a random component in the matter density profile. The study is focused on the effect of such matter perturbations upon both large and small mixing angle…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Rossi

Recent work on neutrino propagation in stochastic media and its implications for the Sun and core-collapse supernovae are reviewed. It is shown that recent results from Sudbury Neutrino Observatory and SuperKamiokande combined with a best…

高能物理 - 唯象学 · 物理学 2008-11-26 A. B. Balantekin

We study the properties of neutrinos propagating in an isotropic magnetized medium in the two physical approximations of degenerate Fermi gas and classical plasma. The dispersion relation shows that, for peculiar configurations of the…

高能物理 - 唯象学 · 物理学 2009-09-25 S. Esposito , G. Capone
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