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相关论文: Testing the LMA solution with solar neutrinos inde…

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Solar neutrino experiments have yet to see directly the transition region between matter-enhanced and vacuum oscillations. The transition region is particularly sensitive to models of non-standard neutrino interactions and propagation. We…

高能物理 - 唯象学 · 物理学 2015-06-16 R. Bonventre , A. LaTorre , J. R. Klein , G. D. Orebi Gann , S. Seibert , O. Wasalski

The neutrino community is convinced that if the LMA solution is indeed correct, the prospects for next-generation, long-baseline neutrino experiments are very exciting. In this work we will argue that the prospects are not less exiting if…

高能物理 - 唯象学 · 物理学 2007-05-23 Gabriela Barenboim , Andre de Gouvea

Measuring all neutrino components is the most direct way to test the standard solar model (SSM). Despite the great results obtained so far, important questions such as the solar metallicity remain open. A precise measurement of the solar pp…

高能物理 - 实验 · 物理学 2019-01-30 Lino Miramonti

Assuming 3 neutrino mixing and massive Majorana neutrinos, we analyze the implications of the results of the solar neutrino experiments, including the latest SNO data, which favor the LMA MSW solution of the solar neutrino problem with…

高能物理 - 唯象学 · 物理学 2010-04-05 S. Pascoli , S. T. Petcov

We reconsider the impact of $\bar\nu_e \leftrightarrow \bar\nu_{\mu,\tau}$ neutrino oscillations on the observed $\bar\nu_e$ signal of supernova SN 1987A. Performing a maximum-likelihood analysis using as fit parameters the released binding…

高能物理 - 唯象学 · 物理学 2009-10-31 M. Kachelriess , R. Tomas , J. W. F. Valle

In presence of non standard interactions, the solar neutrino data is consistent with two solutions, one close to the standard LMA solution with $\sin^2\theta_{12} \simeq 0.3$ and another with $\sin^2\theta_{12}^D \simeq…

高能物理 - 唯象学 · 物理学 2021-02-03 Sandhya Choubey , Dipyaman Pramanik

An updated analysis of all available neutrino oscillation evidence in Solar experiments including the latest $SNO$ data is presented. Predictions for total rates and day-night asymmetry in Borexino are calculated. Our analysis features the…

高能物理 - 唯象学 · 物理学 2014-11-17 P. Aliani , V. Antonelli , M. Picariello , E. Torrente-Lujan

Within the framework of an SO(10) GUT model that can accommodate both the LMA and LOW solar neutrino mixing solutions by appropriate choice of the right-handed Majorana matrix elements, we present explicit predictions for the neutrino…

高能物理 - 唯象学 · 物理学 2009-11-07 Carl H. Albright , S. Geer

We review neutrino oscillation physics, including the determination of mass splittings and mixings from current solar, atmospheric, reactor and accelerator neutrino data. A brief discussion is given of cosmological and astrophysical…

高能物理 - 唯象学 · 物理学 2009-09-17 S. Pakvasa , J. W. F. Valle

The study of neutrinos is fundamental to connect astrophysics and elementary particle physics. In this last decade solar neutrino experiments and KamLAND confirmed the LMA solution and further clarified the mass and oscillation pattern.…

太阳与恒星天体物理 · 物理学 2017-08-23 Vito Antonelli , Lino Miramonti

We present the results of a Bayesian analysis of solar neutrino data in terms of nu_e->nu_{mu,tau} oscillations, independent from the Standard Solar Model predictions for the solar neutrino fluxes. We show that such a model independent…

高能物理 - 唯象学 · 物理学 2009-11-07 M. V. Garzelli , C. Giunti

The Homestake result is about ~ 2 \sigma lower than the Ar-production rate, Q_{Ar}, predicted by the LMA MSW solution of the solar neutrino problem. Also there is no apparent upturn of the energy spectrum (R \equiv N_{obs}/N_{SSM}) at low…

高能物理 - 唯象学 · 物理学 2008-11-26 P. C. de Holanda , A. Yu. Smirnov

We analyze the expected signals of two future neutrino experiments, kamLAND and BOREXINO. We show that with just these experiments, we will hopefully be able to determine which of the existing solutions to the solar neutrino problem is the…

高能物理 - 唯象学 · 物理学 2007-05-23 P. Aliani , V. Antonelli , R. Ferrari , M. Picariello , E. Torrente-Lujan

We perform a global analysis of the latest solar neutrino data including the SNO result on the CC-event rate. This result further favors the LMA solution of the solar neutrino problem. The best fit values of parameters we find are: \Delta…

高能物理 - 唯象学 · 物理学 2009-11-07 P. I. Krastev , A. Yu. Smirnov

Large Mixing Angle (LMA) neutrino oscillation is the main solution for the long-standing Solar Neutrino Problem (SNP). Whether there is any subdominant effect accompanying the dominant LMA solution can not be ruled out at the moment, but…

高能物理 - 唯象学 · 物理学 2009-11-11 Bhag C. Chauhan

The robustness of the large mixing angle (LMA) oscillation (OSC) interpretation of the solar neutrino data is considered in a more general framework where non-standard neutrino interactions (NSI) are present. Such interactions may be…

高能物理 - 唯象学 · 物理学 2009-11-10 O. G. Miranda , M. A. Tortola , J. W. F. Valle

Recent SNO results give strong evidence that the solar neutrinos undergo the flavor conversion. Main issue now is the identification of the mechanism of conversion. The LMA MSW solution with $\Delta m^2 = (5 - 7) \cdot 10^{-5}$ eV$^2$,…

高能物理 - 唯象学 · 物理学 2011-01-31 A. Yu. Smirnov

The first results from the KamLAND experiment have provided confirmational evidence for the Large Mixing Angle (LMA) MSW solution to the solar neutrino problem. We do a global analysis of solar and the recently announced KamLAND data (both…

高能物理 - 唯象学 · 物理学 2009-11-07 Abhijit Bandyopadhyay , Sandhya Choubey , Raj Gandhi , Srubabati Goswami , D. P. Roy

We discuss the status of the solutions of the solar neutrino problem in terms of oscillations of $\nu_e$ into active or sterile neutrinos. We present the results of a global fit to the full data set corresponding to the latest data…

高能物理 - 唯象学 · 物理学 2009-10-31 M. C. Gonzalez-Garcia , C. Peña-Garay

We study neutrino oscillations and the level-crossing probability PLZ in power-law potential profiles A(r)\propto r^n. We give local and global adiabaticity conditions valid for all mixing angles theta and discuss different representations…

高能物理 - 唯象学 · 物理学 2009-09-25 M. Kachelriess , A. Strumia , R. Tomas , J. W. F. Valle
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