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Related papers: Neutrino Decay and Solar Neutrino Seasonal Effect

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We present the results of the observations performed in the occasion of the June 21, 2001 total solar eclipse, looking for visible photons emitted trough a possible radiative decay of solar neutrinos. We establish lower limits for the…

High Energy Physics - Experiment · Physics 2008-11-26 S. Cecchini , D. Centomo , G. Giacomelli , R. Giacomelli , V. Popa , C. G. Serbanut , R. Serra

Using the data from SuperKamiokande, Kamiokande and Homestake solar neutrino experiments we derive an upper bound on the magnetic moment of the neutrino and find $\mu_{\nu_e}\leq(2.2-2.3)\times 10^{-10}\mu_{B}$, within four different…

High Energy Physics - Phenomenology · Physics 2009-10-30 Joao Pulido , Ana M. Mourao

An analysis of neutrino electron scattering as applied to the SuperKamiokande solar neutrino experiment with the data from the Homestake experiment leads to an upper bound on the neutrino magnetic moment in the range…

High Energy Physics - Phenomenology · Physics 2007-05-23 Joao Pulido , Ana M. Mourao

Limiting ourselves to two flavor approximation the motion of the neutrino flux in the solar matter and twisting magnetic field is considered. For the neutrino system described by the 4-component wave function $\Psi^T = (\nu_{eL}, \nu_{XL},…

High Energy Physics - Phenomenology · Physics 2016-10-26 O. M. Boyarkin , G. G. Boyarkina

The multi-ton-scale liquid xenon detectors, with an excellent energy resolution of a few keV, will be constructed to probe the dark-matter particles. In this paper, we show that precision measurements of the low-energy solar neutrinos via…

High Energy Physics - Phenomenology · Physics 2019-02-15 Guo-yuan Huang , Shun Zhou

The decay of the free neutron into a proton, electron, and antineutrino is the prototype semileptonic weak decay and the simplest example of nuclear beta decay. The nucleon vector and axial vector weak coupling constants G_V and G_A…

Nuclear Experiment · Physics 2014-11-14 F. E. Wietfeldt

Neutrino oscillation experiments and direct bounds on absolute masses constrain neutrino mass differences to fall into the microwave energy range, for most of the allowed parameter space. As a consequence of these recent phenomenological…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. Mirizzi , D. Montanino , P. D. Serpico

Gamma radiation associated with radon decay exhibits variations in both time of year and time of day. The annual oscillation has its maximum value in June, suggestive of a galactic influence. Measurements made at midnight show strong…

Solar and Stellar Astrophysics · Physics 2017-05-12 P. A. Sturrock , G. Steinitz , E. Fischbach

We investigate the status of the neutrino decay solution to the solar neutrino problem in the context of the recent results from Sudbury Neutrino Observatory (SNO). We present the results of global $\chi^2$-analysis for both two and three…

High Energy Physics - Phenomenology · Physics 2008-11-26 Abhijit Bandyopadhyay , Sandhya Choubey , Srubabati Goswami

We probe for evidence of invisible neutrino decay in the latest NOvA and T2K data. It is seen that both NOvA and T2K data sets are better fitted when one allows for invisible neutrino decay. We consider a scenario where only the third…

High Energy Physics - Phenomenology · Physics 2018-09-26 Sandhya Choubey , Debajyoti Dutta , Dipyaman Pramanik

It is shown how deviations of neutrino flavor mix from the canonical 1 : 1 : 1 in high energy astrophysical neutrinos can provide evidence for neutrino decays with lifetimes as long as $10^4 s/eV$.

High Energy Physics - Phenomenology · Physics 2007-05-23 S. Pakvasa

Various recent observational developments are here used to make a more critical analysis of the parameter space of the decaying neutrino theory for the ionisation of the interstellar medium. These developments involve phenomena inside our…

Astrophysics · Physics 2016-08-30 D. W. Sciama

We investigate the solar neutrino problem assuming simultaneous presence of MSW transitions in the sun and neutrino decay on the way from sun to earth. We do a global $\chi^2$-analysis of the data on total rates in Cl, Ga and…

High Energy Physics - Phenomenology · Physics 2009-11-07 Abhijit Bandyopadhyay , Sandhya Choubey , Srubabati Goswami

In this paper we consider the hypothesis that neutrinos are fermionic tachyons with helicity 1/2. We propose an effective model of interactions of these neutrinos and analyze dominant effects under the above hypothesis: the three-body…

High Energy Physics - Phenomenology · Physics 2007-05-23 Pawel Caban , Jakub Rembielinski , Kordian A. Smolinski

We report a reanalysis of data on the measured decay rate ratio $^{22}$Na/$^{44}$Ti which were originally published by Norman et al., and interpreted as supporting the conventional hypothesis that nuclear decay rates are constant and not…

A new tension is emerging between the tight cosmological upper bounds on the total neutrino mass ($\sum m_\nu \lesssim 0.06 \, \rm{eV}$) and the lower limits from oscillation experiments, with potentially far-reaching implications for…

Cosmology and Nongalactic Astrophysics · Physics 2026-01-09 Guillermo Franco Abellán

Motivated by a pilot experiment conducted by F.Vannucci et al. during a solar eclipse, we work out the geometry governing the radiative decays of solar neutrinos. Surprisingly, although a smaller proportion of the photons can be detected,…

High Energy Physics - Phenomenology · Physics 2009-10-31 J. -M. Frère , D. Monderen

We investigate the status of a scenario involving oscillations and decay for charged and neutral current data from the MINOS and T2K experiments. We first present an analysis of charged current neutrino and anti-neutrino data from MINOS in…

High Energy Physics - Phenomenology · Physics 2014-12-23 R. A. Gomes , A. L. G. Gomes , O. L. G. Peres

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…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. B. Balantekin

Neutrinos mix and have mass differences, so decays from one to another must occur. But how fast? The best direct limits on non-radiative decays, based on solar and atmospheric neutrinos, are weak, $\tau \gtrsim 10^{-3}$ s ($m$/eV) or much…

High Energy Astrophysical Phenomena · Physics 2017-03-29 Mauricio Bustamante , John F. Beacom , Kohta Murase