中文
相关论文

相关论文: Global Analysis of Solar Neutrino and KamLAND Data

200 篇论文

We present new constraints on the neutrino oscillation parameters $/textyen Delta m^{2}_{21}$, $/textyen theta_{12}$, and $/textyen theta_{13}$ from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes data…

高能物理 - 实验 · 物理学 2012-08-27 The KamLAND Collaboration

However the allowed range of $\theta_{\odot}$ ($\theta_{12}$) did not change much with the inclusion of the KamLAND results. In this paper we probe if future data from KamLAND can increase the accuracy of the allowed range in…

高能物理 - 唯象学 · 物理学 2009-11-10 Abhijit Bandyopadhyay , Sandhya Choubey , Srubabati Goswami

In a previous paper [1], we presented a three-flavour oscillation analysis of the solar neutrino measurements and of the first data from the KamLAND experiment, in terms of the relevant mass-mixing parameters (delta m^2, theta_12,…

高能物理 - 唯象学 · 物理学 2009-10-07 G. L. Fogli , E. Lisi , A. Marrone , D. Montanino , A. Palazzo , A. M. Rotunno

The recent measurement of Delta_{sol} by the KamLAND experiment with very small errors, makes definitive predictions for the energy dependence of the solar neutrino survival probability P_{ee}. We fix Delta_{sol} to be the KamLAND best fit…

高能物理 - 唯象学 · 物理学 2011-03-31 Bipin Singh Koranga , Mohan Narayan , S. Uma Sankar

We present an updated analysis of all available solar and reactor neutrino data, emphasizing in particular the totality of the KamLAND results and including the SNO phase III spectrum data. In a two active-neutrino framework, we determine…

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 report results from a combined analysis of solar neutrino data from all phases of the Sudbury Neutrino Observatory. By exploiting particle identification information obtained from the proportional counters installed during the third…

核实验 · 物理学 2013-08-09 SNO Collaboration , B. Aharmim , S. N. Ahmed , A. E. Anthony , N. Barros , E. W. Beier , A. Bellerive , B. Beltran , M. Bergevin , S. D. Biller , K. Boudjemline , M. G. Boulay , B. Cai , Y. D. Chan , D. Chauhan , M. Chen , B. T. Cleveland , G. A. Cox , X. Dai , H. Deng , J. A. Detwiler , M. DiMarco , P. J. Doe , G. Doucas , P. -L. Drouin , F. A. Duncan , M. Dunford , E. D. Earle , S. R. Elliott , H. C. Evans , G. T. Ewan , J. Farine , H. Fergani , F. Fleurot , R. J. Ford , J. A. Formaggio , N. Gagnon , J. TM. Goon , K. Graham , E. Guillian , S. Habib , R. L. Hahn , A. L. Hallin , E. D. Hallman , P. J. Harvey , R. Hazama , W. J. Heintzelman , J. Heise , R. L. Helmer , A. Hime , C. Howard , M. Huang , P. Jagam , B. Jamieson , N. A. Jelley , M. Jerkins , K. J. Keeter , J. R. Klein , L. L. Kormos , M. Kos , C. Kraus , C. B. Krauss , A Kruger , T. Kutter , C. C. M. Kyba , R. Lange , J. Law , I. T. Lawson , K. T. Lesko , J. R. Leslie , J. C. Loach , R. MacLellan , S. Majerus , H. B. Mak , J. Maneira , R. Martin , N. McCauley , A. B. McDonald , S. R. McGee , M. L. Miller , B. Monreal , J. Monroe , B. G. Nickel , A. J. Noble , H. M. O'Keeffe , N. S. Oblath , R. W. Ollerhead , G. D. Orebi Gann , S. M. Oser , R. A. Ott , S. J. M. Peeters , A. W. P. Poon , G. Prior , S. D. Reitzner , K. Rielage , B. C. Robertson , R. G. H. Robertson , R. C. Rosten , M. H. Schwendener , J. A. Secrest , S. R. Seibert , O. Simard , J. J. Simpson , P. Skensved , T. J. Sonley , L. C. Stonehill , G. Tešić , N. Tolich , T. Tsui , R. Van Berg , B. A. VanDevender , C. J. Virtue , H. Wan Chan Tseung , D. L. Wark , P. J. S. Watson , J. Wendland , N. West , J. F. Wilkerson , J. R. Wilson , J. M. Wouters , A. Wright , M. Yeh , F. Zhang , K. Zuber

We have performed analysis of the solar neutrino data including results from the SNO salt phase as well as the combined analysis of the solar and the KamLAND results. The best fit values of neutrino parameters are Delta m^2 = 7.1e-5 eV^2,…

高能物理 - 唯象学 · 物理学 2011-05-23 P. C. de Holanda , A. Yu. Smirnov

We present the constraints on neutrino oscillation parameters $\Delta m^2_{\odot}$ and $\theta_{\odot}$ governing the solar neutrino oscillations from two generation analysis of solar and KamLAND data. We include the latest 766.3 ton year…

高能物理 - 唯象学 · 物理学 2014-11-18 Srubabati Goswami , Abhijit Bandyopadhyay , Sandhya Choubey

We investigate the impact of the 766.3 Ty KamLAND spectrum data on the determination of the solar neutrino oscillation parameters. We show that the observed spectrum distortion in the KamLAND experiment firmly establishes $\Delta m^2_{21}$…

高能物理 - 唯象学 · 物理学 2008-11-26 Abhijit Bandyopadhyay , Sandhya Choubey , Srubabati Goswami , S. T. Petcov , D. P. Roy

We explore whether KamLAND and solar data may end up inconsistent when analyzed in terms of two-flavor neutrino oscillations. If this turned out to be the case, one would be led to conclude that there is more new physics, besides neutrino…

高能物理 - 唯象学 · 物理学 2008-11-26 Andre de Gouvea , Carlos Pena-Garay

We analyze the cumulative data from the latest SNO, KamLAND and other solar neutrino experiments in the standard scenario of three oscillating active neutrinos. We determine the solar neutrino oscillation parameters and obtain new bounds on…

高能物理 - 唯象学 · 物理学 2009-09-15 A. B. Balantekin , V. Barger , D. Marfatia , S. Pakvasa , H. Yuksel

We explore the impact of the data from the KamLAND experiment in constraining neutrino mass and mixing angles involved in solar neutrino oscillations. In particular we discuss the precision with which we can determine the the mass squared…

高能物理 - 唯象学 · 物理学 2009-11-10 Srubabati Goswami , Abhijit Bandyopadhyay , Sandhya Choubey

If the solution to the solar neutrino puzzle falls in the LMA region, KamLAND should be able to measure with good precision the corresponding oscillation parameters after a few years of data taking. Assuming a positive signal, we study…

高能物理 - 唯象学 · 物理学 2009-11-07 M. C. Gonzalez-Garcia , C. Peña-Garay

We compare, using a three neutrino analysis, the allowed neutrino oscillation parameters and solar neutrino fluxes determined by the experimental data available Before and After Neutrino 2004. New data available after Neutrino2004 include…

高能物理 - 唯象学 · 物理学 2014-11-17 John N. Bahcall , M. C. Gonzalez-Garcia , Carlos Pena-Garay

Solar neutrino oscillations are supported by KamLAND's antineutrino measurements, but certain solar neutrino data - the observed shape of the ${}^8$B flux and the difference between day and night counting rates measured in Super-Kamiokande…

高能物理 - 唯象学 · 物理学 2018-01-01 Francesco Vissani

We present an updated analysis of all available solar and reactor neutrino data, emphasizing in particular the totality of the KamLAND (314d live time) results and including for the first time the solar $SNO$ (391d live time, phase II…

高能物理 - 唯象学 · 物理学 2007-05-23 V. Antonelli , E. Torrente-Lujan

An updated analysis of all available neutrino oscillation evidence in Reactor (Kamland, first 145 days of data) and Solar experiments (SK day and night spectra, global rates from Homestake, SAGE and GALLEX) including the $SNO CC$ and $NC$…

高能物理 - 唯象学 · 物理学 2016-09-06 P. Aliani , V. Antonelli , M. Picariello , E. Torrente-Lujan

We do a re-analysis to asses the impact of the results of the Borexino experiment and the recent 2.8 KTy KamLAND data on the solar neutrino oscillation parameters. The current Borexino results are found to have no impact on the allowed…

高能物理 - 唯象学 · 物理学 2008-05-01 Abhijit Bandyopadhyay , Sandhya Choubey , Srubabati Goswami , S. T. Petcov , D. P. Roy

We consider the impact of the recent KamLAND data on neutrino oscillations, the first terrestrial neutrino experiment that can probe the solar neutrino anomaly. By combining the first 145.1 days of KamLAND data with the full sample of…

高能物理 - 唯象学 · 物理学 2009-09-17 M. Maltoni , T. Schwetz , J. W. F. Valle

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
‹ 上一页 1 2 3 10 下一页 ›