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相关论文: Earth matter effects on the supernova neutrino spe…

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We analyze the neutrino conversions inside a supernova in the 3$\nu$ mixing scheme, and their effects on the neutrino spectra observed at the earth. We find that the observations of the energy spectra of neutrinos from a future galactic…

高能物理 - 唯象学 · 物理学 2009-10-31 Amol S. Dighe

We perform a detailed study of the Earth matter effects on supernova neutrinos. The dependences of these effects on the properties of the original neutrino fluxes, on the trajectory of the neutrinos inside the Earth and on the oscillation…

高能物理 - 唯象学 · 物理学 2016-09-06 C. Lunardini , A. Yu. Smirnov

The Earth effects on the energy spectra of supernova neutrinos are studied. We analyze numerically the time-integrated energy spectra of neutrino in a mantle-core-mantle step function model of the Earth's matter density profile. We consider…

高能物理 - 唯象学 · 物理学 2014-11-17 K. Takahashi , M. Watanabe , K. Sato

We study the role that the future detection of the neutrino burst from a galactic supernova can play in the reconstruction of the neutrino mass spectrum. We consider all possible 3$\nu$ mass and flavor spectra which describe the solar and…

高能物理 - 唯象学 · 物理学 2009-10-31 Amol S. Dighe , Alexei Yu. Smirnov

The neutrino oscillations in Earth matter introduce modulations in the supernova neutrino spectra. These modulations can be exploited to identify the presence of Earth effects on the spectra, which would enable us to put a limit on the…

高能物理 - 唯象学 · 物理学 2009-11-10 Amol S. Dighe , Mathias Th. Keil , Georg G. Raffelt

We study Earth matter effect in oscillation of supernovae neutrinos. We show that detecting Earth matter effect gives an independent measurement of spectra of supernovae neutrinos, i.e. the flavor difference of the spectra of supernovae…

高能物理 - 唯象学 · 物理学 2017-01-16 Wei Liao

We perform a detailed study of the Earth matter effects on supernova neutrinos with neutrino oscillation parameter LMA and small $\theta_{13}$. The Earth effects show significant dependences on the neutrino path length inside the Earth and…

高能物理 - 唯象学 · 物理学 2009-11-07 K. Takahashi , K. Sato

We calculated the matter effect, including both the Earth and supernova, on the detection of neutrinos from type II supernovae at the proposed Daya Bay reactor neutrino experiment. It is found that apart from the dependence on the flip…

高能物理 - 唯象学 · 物理学 2009-11-11 X. -H. Guo , Bing-Lin Young

Neutrino oscillations in the Earth matter may introduce peculiar modulations in the supernova (SN) neutrino spectra. The detection of this effect has been proposed as diagnostic tool for the neutrino mass hierarchy at "large" 1-3 leptonic…

高能物理 - 唯象学 · 物理学 2015-03-20 Enrico Borriello , Sovan Chakraborty , Alessandro Mirizzi , Pasquale Dario Serpico , Irene Tamborra

A nearby core collapse supernova will produce a burst of neutrinos in several detectors worldwide. With reasonably high probability, the Earth will shadow the neutrino flux in one or more detectors. In such a case, for allowed oscillation…

天体物理仪器与方法 · 物理学 2010-04-06 Kate Scholberg , Armin Burgmeier , Roger Wendell

The observation of Earth matter effects in the spectrum of neutrinos coming from a next galactic core-collapse supernova (CCSN) could, in principle, reveal if neutrino mass ordering is normal or inverted. One of the possible ways to…

高能物理 - 唯象学 · 物理学 2022-01-12 Edwin A. Delgado , Hiroshi Nunokawa , Alexander A. Quiroga

Matter effects on neutrino oscillations in both, a supernova and the Earth, change the observed supernova neutrino spectra. We calculate the expected number of supernova neutrino interactions for ICARUS, SK and SNO detectors as a function…

高能物理 - 唯象学 · 物理学 2007-05-23 B. Bekman , J. Holeczek , J. Kisiel

We consider the supernova shock effects, the Mikheyev-Smirnov-Wolfenstein (MSW) effects, the collective effects, and the Earth matter effects in the detection of type II supernova neutrinos on the Earth. It is found that the event number of…

高能天体物理现象 · 物理学 2014-11-20 Ming-Yang Huang , Xin-Heng Guo , Bing-Lin Young

We introduce an integrated algorithm for full scale investigation of the earth regeneration effect of solar neutrinos with all three active neutrinos. We illustrate that the earth effect on low energy solar neutrinos ($E_\nu < 20$ MeV)…

高能物理 - 唯象学 · 物理学 2014-11-17 Jai Sam Kim , Kyungsoo Lee

We show that the earth matter effects in the ${\rm {\nu_e \to \nu_e}}$ survival probability can be used to cleanly determine the third leptonic mixing angle $\theta_{13}$ and the sign of the atmospheric neutrino mass squared difference,…

高能物理 - 唯象学 · 物理学 2008-11-26 Sanjib Kumar Agarwalla , Sandhya Choubey , Srubabati Goswami , Amitava Raychaudhuri

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

The Earth matter effects on supernova (SN) neutrinos can be identified at a single detector through peaks in the Fourier transform of their ``inverse energy'' spectrum. The positions of these peaks are independent of the SN models and…

高能物理 - 唯象学 · 物理学 2009-11-10 A. S. Dighe , M. Kachelriess , G. G. Raffelt , R. Tomas

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 present a formalism for the matter effects in the Earth on low energy neutrino fluxes which is both accurate and has all advantages of a full analytic treatment. The oscillation probabilities are calculated up to second order term in…

高能物理 - 唯象学 · 物理学 2009-11-10 A. N. Ioannisian , N. A. Kazarian , A. Yu. Smirnov , D. Wyler

We calculate the expected galactic supernova neutrino signal at large next-generation underground detectors. At different epochs after the explosion, the primary fluxes can be quite different. For these primary neutrino fluxes, spectral…

高能物理 - 唯象学 · 物理学 2010-08-03 Sandhya Choubey , Basudeb Dasgupta , Amol Dighe , Alessandro Mirizzi
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