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相关论文: Addendum to: Global constraints on absolute neutri…

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We present a concise formula to relate the effective mass term of the neutrinoless double beta decay to a single neutrino mass, two Majorana CP-violating phases and four observables of neutrino oscillations for a generic neutrino mass…

高能物理 - 唯象学 · 物理学 2009-11-07 Zhi-zhong Xing

We have studied the constraints imposed by the results of neutrino oscillation experiments on the effective Majorana mass |<m>| that characterizes the contribution of Majorana neutrino masses to the matrix element of neutrinoless…

高能物理 - 唯象学 · 物理学 2016-08-25 S. M. Bilenky , C. Giunti , C. W. Kim , M. Monteno

The discovery of neutrino oscillations has shown that neutrinos, in contradiction to a prediction of the minimal standard model, have mass. Oscillations do not yield a value for the mass, but do set a lower limit of 0.02 eV on the average…

核实验 · 物理学 2015-02-03 R. G. Hamish Robertson

We study the constraints imposed by neutrino oscillation experiments on the minimal extensions of the Standard Model (SM) with $n_R$ gauge singlet fermions ("right-handed neutrinos"), that can account for neutrino masses. We consider the…

高能物理 - 唯象学 · 物理学 2012-09-18 A. Donini , P. Hernandez , J. Lopez-Pavon , M. Maltoni

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

A randomly generated complex symmetric matrix using Adaptive Monte Carlo method, is taken as a general form of Majorana neutrino mass matrix, which is diagonalized by the use of eigenvectors. We extract all the neutrino oscillation…

高能物理 - 唯象学 · 物理学 2024-07-30 Y Monitar Singh , Mayengbam Kishan Singh , N Nimai Singh

Proposed medium-baseline reactor neutrino experiments offer unprecedented opportunities to probe, at the same time, the mass-mixing parameters which govern $\nu_e$ oscillations both at short wavelength (delta m^2 and theta_{12}) and at long…

高能物理 - 唯象学 · 物理学 2014-01-15 F. Capozzi , E. Lisi , A. Marrone

A range of experimental results point to the existence of a massive neutrino. The recent high precision measurements of the cosmic microwave background and the large scale surveys of galaxies can be used to place an upper bound on this…

天体物理学 · 物理学 2009-06-12 C. Zunckel , P. G Ferreira

We present cosmological upper limits on the sum of active neutrino masses using large-scale power spectrum data from the WiggleZ Dark Energy Survey and from the Sloan Digital Sky Survey - Data Release 7 (SDSS-DR7) sample of Luminous Red…

宇宙学与河外天体物理 · 物理学 2016-04-29 Antonio J. Cuesta , Viviana Niro , Licia Verde

We will investigate numerically a seesaw model with $A_4$ flavor symmetry to find allowed regions satisfying the current experimental neutrino oscillation data, then use them to predict physical consequences. Namely, the lightest active…

高能物理 - 唯象学 · 物理学 2020-04-01 T. Phong Nguyen , L. T. Hue , D. T. Si , T. T. Thuc

We examine the potential for a ``natural'' three-neutrino mixing scheme to satisfy available data and astrophysical arguments. By ``natural'' we mean no sterile neutrinos, and a neutrino mass hierarchy similar to that of the charged…

天体物理学 · 物理学 2011-03-10 Christian Y. Cardall , George M. Fuller

We present an analysis of the global neutrino oscillation data including the LSND result in terms of four-neutrino mass schemes and a CPT violating three-neutrino framework. We find that the strong preference of oscillations into active…

高能物理 - 唯象学 · 物理学 2007-05-23 Thomas Schwetz

All existing solar and atmospheric neutrino oscillation data are described by the standard two-neutrino formulas with neutrino mass squared differences that satisfy the hierarchy relation $\Delta m^{2}_{sol} \ll \Delta m^{2}_{atm}$. We…

高能物理 - 唯象学 · 物理学 2007-05-23 S. M. Bilenky

We have analyzed the results of reactor and accelerator neutrino oscillation experiments in the framework of a general model with mixing of three neutrino fields and a neutrino mass hierarchy that can accommodate the results of the solar…

高能物理 - 唯象学 · 物理学 2009-10-28 S. M. Bilenky , A. Bottino , C. Giunti , C. W. Kim

We have studied bounds on the neutrino mass using new data from the WMAP 3 year data, the Sloan Digital Sky Survey measurement of the baryon acoustic peak, the Type Ia supernovae from SNLS, and the Lyman-alpha forest. We find that even in…

天体物理学 · 物理学 2009-11-11 Ariel Goobar , Steen Hannestad , Edvard Mortsell , Huitzu Tu

I review the interpretation of solar and atmospheric neutrino data in terms neutrino oscillations and describe some ways to account for the required neutrino masses and mixing angles from first principles, both within top-down and bottom-up…

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

We discuss the physics potential of intermediate $L \sim 20 \div 30$ km baseline experiments at reactor facilities, assuming that the solar neutrino oscillation parameters $\Delta m^2_{\odot}$ and $\theta_{\odot}$ lie in the high-LMA…

高能物理 - 唯象学 · 物理学 2011-02-11 Sandhya Choubey , S. T. Petcov , M. Piai

Assuming four-neutrino mixing and massive Majorana neutrinos, we study the implications of the neutrino oscillation solutions of the solar and atmospheric neutrino problems, of the results of the LSND experiment and of the constraints on…

高能物理 - 唯象学 · 物理学 2010-05-28 S. M. Bilenky , S. Pascoli , S. T. Petcov

We present updated results from the NOvA experiment for $\nu_\mu\rightarrow\nu_\mu$ and $\nu_\mu\rightarrow\nu_e$ oscillations from an exposure of $8.85\times10^{20}$ protons on target, which represents an increase of 46% compared to our…

高能物理 - 实验 · 物理学 2018-08-29 M. A. Acero , P. Adamson , L. Aliaga T. Alion , V. Allakhverdian , N. Anfimov A. Antoshkin , E. Arrieta-Diaz , A. Aurisano A. Back , C. Backhouse , M. Baird N. Balashov , B. A. Bambah , K. Bays B. Behera , S. Bending , R. Bernstein V. Bhatnagar , B. Bhuyan , J. Bian T. Blackburn , J. Blair , A. Bolshakova P. Bour , C. Bromberg , J. Brown N. Buchanan , A. Butkevich , V. Bychkov M. Campbell , T. J. Carroll , E. Catano-Mur A. Cedeno , S. Childress , B. C. Choudhary B. Chowdhury , T. E. Coan , M. Colo J. Cooper , L. Corwin , L. Cremonesi D. Cronin-Hennessy , G. S. Davies , J. P. Davies S. De Rijck , P. F. Derwent , R. Dharmapalan P. Ding , Z. Djurcic , E. C. Dukes P. Dung , H. Duyang , S. Edayath R. Ehrlich , G. J. Feldman , M. J. Frank H. R. Gallagher , R. Gandrajula , F. Gao S. Germani , A. Giri , R. A. Gomes M. C. Goodman , V. Grichine , M. Groh R. Group , D. Grover , B. Guo A. Habig , F. Hakl , J. Hartnell R. Hatcher , A. Hatzikoutelis , K. Heller A. Himmel , A. Holin , B. Howard J. Huang , J. Hylen , F. Jediny M. Judah , I. Kakorin , D. Kalra D. M. Kaplan , R. Keloth , O. Klimov L. W. Koerner , L. Kolupaeva , S. Kotelnikov I. Kourbanis , A. Kreymer , Ch. Kulenberg A. Kumar , C. Kuruppu , V. Kus T. Lackey , K. Lang , S. Lin M. Lokajicek , J. Lozier , S. Luchuk K. Maan , S. Magill , W. A. Mann M. L. Marshak , V. Matveev , D. P. Méndez M. D. Messier , H. Meyer , T. Miao W. H. Miller , S. R. Mishra , A. Mislivec R. Mohanta , A. Moren , L. Mualem M. Muether , S. Mufson , R. Murphy J. Musser , D. Naples , N. Nayak J. K. Nelson , R. Nichol , E. Niner A. Norman , T. Nosek , Y. Oksuzian A. Olshevskiy , T. Olson , J. Paley R. B. Patterson , G. Pawloski , D. Pershey O. Petrova , R. Petti , S. Phan-Budd R. K. Plunkett , B. Potukuchi , C. Principato F. Psihas , A. Radovic , R. A. Rameika B. Rebel , P. Rojas , V. Ryabov K. Sachdev , O. Samoylov , M. C. Sanchez J. Sepulveda-Quiroz , P. Shanahan , A. Sheshukov P. Singh , V. Singh , E. Smith J. Smolik , P. Snopok , N. Solomey E. Song , A. Sousa , K. Soustruznik M. Strait , L. Suter , R. L. Talaga P. Tas , R. B. Thayyullathil , J. Thomas E. Tiras , S. C. Tognini , D. Torbunov J. Tripathi , A. Tsaris , Y. Torun J. Urheim , P. Vahle , J. Vasel L. Vinton , P. Vokac , A. Vold T. Vrba , B. Wang , T. K. Warburton M. Wetstein , D. Whittington , S. G. Wojcicki J. Wolcott , S. Yang , S. Yu J. Zalesak , B. Zamorano , R. Zwaska

A simple and natural extension of the standard Lambda cold dark matter ($\Lambda$CDM) model is to allow relic neutrinos to have finite chemical potentials. We confront this $\Lambda$CDM$\xi$ model, a $\Lambda$CDM with neutrino mass $M_\nu$…

高能物理 - 唯象学 · 物理学 2025-09-03 Shek Yeung , Wangzheng Zhang , Ming-chung Chu
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