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相关论文: Neutrino parameters from matter effects in $P_{ee}…

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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 study matter effects which arise in the muon neutrino oscillation and survival probabilities relevant to atmospheric neutrino and very long baseline beam experiments. The inter-relations between the three probabilities P_{\mu e}, P_{\mu…

高能物理 - 唯象学 · 物理学 2009-11-10 Raj Gandhi , Pomita Ghoshal , Srubabati Goswami , Poonam Mehta , S Uma Sankar

We calculate matter effects on neutrino oscillations relevant for long baseline neutrino oscillation experiments. In particular, we compare the results obtained with simplifying approximations for the density profile in the Earth versus…

高能物理 - 唯象学 · 物理学 2010-12-13 Irina Mocioiu , Robert Shrock

We explore the earth matter effects on the energy spectra of neutrinos from a supernova. We show that the observations of the energy spectra of $\nu_e$ and $\bar{\nu}_e$ from a galactic supernova may enable us to identify the solar neutrino…

高能物理 - 唯象学 · 物理学 2007-05-23 Amol S. Dighe

We discuss the possibility for matter effects in the three-neutrino oscillations of the atmospheric nu_e (bar{nu}_e) and nu_mu (bar{nu}_mu), driven by one neutrino mass squared difference, |Delta m2_{31}| >> Delta m2_{21}, to be observable…

高能物理 - 唯象学 · 物理学 2007-05-23 Jose Bernabeu , Sergio Palomares-Ruiz

Matter effects in neutrino propagation translate into effective parameters for the oscillation and fake CP- and CPT-odd quantities, even in a scenario, such as $\Delta_{12}=0$, where no genuine CP violation is present. This fact seems to…

高能物理 - 唯象学 · 物理学 2014-11-17 M. C. Banuls , G. Barenboim , J. Bernabeu

Recently it is advocated that high intensity and low energy $(E_\nu \sim 2 GeV)$ neutrino beams should be built to probe the $(13)$ mixing angle $\phi$ to a level of a few parts in $10^4$. Experiments using such beams will have better…

高能物理 - 唯象学 · 物理学 2009-10-31 Mohan Narayan , S. Uma Sankar

We study the matter effects to neutrino oscillations \nu_\mu \to \nu_e and \nu_\mu \to \nu_\mu at very long baselines. It has been observed that, for a very long baseline L~10000 km, the resonance peak for the \nu_\mu \to \nu_e oscillation…

高能物理 - 唯象学 · 物理学 2007-05-23 Guey-Lin Lin , Yoshiaki Umeda

The effect of matter enhanced neutrino oscillations on atmosheric neutrinos is investigated systematically in the framework of one mass dominant model of three neutrinos. The resonance conditions of neutrino crossing the earth are…

高能物理 - 唯象学 · 物理学 2007-05-23 Shoichi Midorikawa

We show that in the framework of three light neutrino species with hierarchical masses and assuming no fine tuning between the entries of the neutrino mass matrix, one can use the solar neutrino data to obtain information on the element…

高能物理 - 唯象学 · 物理学 2008-11-26 E. Kh. Akhmedov , G. C. Branco , M. N. Rebelo

Assuming three-neutrino mixing, we study the capabilities of very long baseline neutrino oscillation experiments to verify and test the MSW effect and to measure the lepton mixing angle theta_13. We suppose that intense neutrino and…

高能物理 - 唯象学 · 物理学 2014-11-17 M. Freund , M. Lindner , S. T. Petcov , A. Romanino

In this paper we focus on the Earth matter effects for the solar parameter determination by a medium baseline reactor experiment such as JUNO. We derive perturbative expansions for the mixing angles $\theta_{12}$ and $\theta_{13}$ as well…

高能物理 - 唯象学 · 物理学 2020-03-12 Amir N. Khan , Hiroshi Nunokawa , Stephen J. Parke

The pattern of oscillation parameters emerging from current experimental data can be further elucidated by the observation of matter effects. In contrast to planned experiments with conventional neutrino beams, atmospheric neutrinos offer…

高能物理 - 唯象学 · 物理学 2011-09-13 T. Tabarelli de Fatis

Experiments strongly suggest that the flavour mixing responsible for the atmospheric neutrino anomaly is very close to being maximal. Thus, it is of great theoretical as well as experimental importance to measure any possible deviation from…

高能物理 - 唯象学 · 物理学 2009-11-10 Debajyoti Choudhury , Anindya Datta

In this paper, we first calculate the realistic Earth matter effects in the detection of type II supernova neutrinos at the Daya Bay reactor neutrino experiment which is currently under construction. It is found that the Earth matter…

高能物理 - 唯象学 · 物理学 2009-06-19 Xin-Heng Guo , Ming-Yang Huang , Bing-Lin Young

We discuss the possibility to observe matter effects in atmospheric neutrino oscillations. The main conclusion is that an impact on the nu_mu survival probability requires the action of the MSW resonance, which becomes visible for baselines…

高能物理 - 唯象学 · 物理学 2015-07-27 J. Bernabeu , S. Palomares-Ruiz

We investigate the effects of a nonzero leptonic mixing angle $\theta_{13}$ on the solar neutrino day-night asymmetry. Using a constant matter density profile for the Earth and well-motivated approximations, we derive analytical expressions…

高能物理 - 唯象学 · 物理学 2009-11-10 Mattias Blennow , Tommy Ohlsson , Hakan Snellman

After some preliminary arguments suggesting that neutrino mixings with inverted mass pattern may be easier to understand within the framework of a local horizontal symmetry SU(2)_H acting on leptons, we construct a specific extension of the…

高能物理 - 唯象学 · 物理学 2014-11-17 R. Kuchimanchi , R. N. Mohapatra

The observed flavor oscillations of solar and atmospheric neutrinos determine several elements of the leptonic mixing matrix, but leave open the small mixing angle Theta_13, a possible CP-violating phase, the mass ordering, the absolute…

天体物理学 · 物理学 2017-08-23 G. G. Raffelt

We re-fit for the neutrino mass-squared difference $\Delta m^2$ in the threefold maximal (ie. tri-maximal) mixing scenario using recent CHOOZ and SUPER-K data, taking account of matter effects in the Earth. While matter effects have little…

高能物理 - 唯象学 · 物理学 2011-07-19 P. F. Harrison , D. H. Perkins , W. G. Scott
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