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相关论文: Towards a realistic neutrino mass formula: part tw…

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Averaged neutrino masses defined by $\la m_\nu\ra_{ab} \equiv\left| \sum_{j=1}^{3}U_{aj}U_{bj}m_j\right|$ ($a,b=e,\mu,\tau$) are reanalyzed using up-to-date observed MNS parameters and neutrino masses by the neutrino oscillation experiments…

高能物理 - 唯象学 · 物理学 2015-10-22 Takeshi Fukuyama , Hiroyuki Nishiura

A four-parameter Majorana neutrino mass matrix is proposed, which is exactly diagonalizable with two mixing angles, one of which is pi/4 and the other large but less than pi/4. The form of this mass matrix allows seven realizations of the…

高能物理 - 唯象学 · 物理学 2009-11-07 Ernest Ma

Two 3x3 matrices playing the role of annihilation and creation operators in the neutrino-flavor space of nu_e, nu_mu, nu_tau are applied to construct the off-diagonal part of neutrino effective mass matrix M. The construction leads to a new…

高能物理 - 唯象学 · 物理学 2007-05-23 Wojciech Krolikowski

A method developed from the Dualized Standard Model for calculating the quark CKM matrix and masses is applied to the parallel problem in neutrino oscillations. Taking the parameters determined from quarks and the masses of two neutrinos:…

高能物理 - 唯象学 · 物理学 2010-11-23 J Bordes , HM Chan , J. Pfaudler , ST Tsou

We discuss neutrino sector in models with two Higgs doublet and one singlet scalar fields under local $U(1)_{L_\alpha- L_\beta}$ symmetry. A neutrino mass matrix is formulated for these models where the matrix is generated via type-I seesaw…

高能物理 - 唯象学 · 物理学 2025-01-28 Yuanchao Lou , Takaaki Nomura

Two schemes of mixing of four massive neutrinos with two close neutrino masses separated by a gap of Delta m^2 about 1 eV^2 can accommodate solar, atmospheric and LSND neutrino oscillation data. It is shown that long-baseline nu(e)->nu(x)…

高能物理 - 唯象学 · 物理学 2007-05-23 S. M. Bilenky , C. Giunti , W. Grimus

In the context of the supersymmetric flipped $SU(5)\otimes U(1)$ GUT model, we have studied in detail the neutrino mass spectrum, obtaining an approximate formula for the corresponding effective three-generation mass matrix. It is found…

高能物理 - 唯象学 · 物理学 2009-10-22 Stefano Ranfone

We investigate the Majorana neutrino mass matrix $M_{\nu}$ with one parameter in the context of two texture zeros and its symmetry realization by non-Abelian discrete symmetry. From numerical calculation, we confirm that the textures…

高能物理 - 唯象学 · 物理学 2013-11-12 Yuji Kajiyama , Akari Sato , Wakako Sato , Aya Suzuki

Theory suggests the existence of neutrino masses, but little more. Facts are coming close to reveal our fantasy: solar and atmospheric neutrino data strongly indicate the need for neutrino conversions, while LSND provides an intriguing…

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

Using data from atmospheric neutrino mixing, and a simple functional form for mixing angles, the absolute values of three neutrino masses are calculated: $m_3\cong 5.37\times 10^{-2} eV$, $m_2\cong 1.94\times 10^{-2} eV$, $m_1\cong…

高能物理 - 唯象学 · 物理学 2010-12-17 Saul Barshay , Georg Kreyerhoff

With a mass at least six orders of magnitudes smaller than the mass of an electron -- but non-zero -- neutrinos are a clear misfit in the Standard Model of Particle Physics. On the one hand, its tiny mass makes the neutrino one of the most…

核实验 · 物理学 2016-06-22 Susanne Mertens

Maximum mixing in atmospheric neutrino oscillation, as well as vanishing of the MNS matrix element $U_{e3}$, are consequences of a 2-3 symmetry, under which the neutrino mass matrix is invariant under the interchange of second and third…

高能物理 - 唯象学 · 物理学 2009-11-07 C. S. Lam

Considering the mass splitting between three active neutrinos, we represent the new constraints on the sum of neutrino mass $\sum m_\nu$ by updating the anisotropic analysis of Baryon Acoustic Oscillation (BAO) scale in the CMASS and LOWZ…

宇宙学与河外天体物理 · 物理学 2016-09-21 Qing-Guo Huang , Ke Wang , Sai Wang

There are two basic theoretical approaches to obtaining neutrino mass and mixing. In the minimalist approach, one adds just enough new stuff to the Minimal Standard Model to get $m_\nu \neq 0$ and $U_{\alpha i} \neq 1$. In the holistic…

高能物理 - 唯象学 · 物理学 2009-10-31 Ernest Ma

The neutrino mixing sum rule $\theta_{12} - \theta_{13}\cos(\delta) \approx \theta^\nu_{12}$ provides a possibility to explore the structure of the neutrino mass matrix in the presence of charged lepton corrections, since it relates the 1-2…

高能物理 - 唯象学 · 物理学 2010-10-27 S. Antusch , P. Huber , S. F. King , T. Schwetz

We discuss what information about the neutrino mass spectrum and the elements of the neutrino mixing matrix can be inferred from the results of neutrino oscillation experiments. The cases of three and four massive neutrinos are considered.…

高能物理 - 唯象学 · 物理学 2009-10-30 S. M. Bilenky , C. Giunti , W. Grimus

The various experiments on neutrino oscillation evidenced that neutrinos have indeed non-zero masses but cannot tell us the absolute neutrino mass scale. This scale of neutrino masses is very important for understanding the evolution and…

高能物理 - 实验 · 物理学 2013-09-05 Christian Weinheimer , Kai Zuber

In the framework of a mass formula proposed previously (transforming in a specific way three free parameters into three masses), a simple empirical sum rule for three charged-lepton masses is found, predicting m_\tau = 1776.9926 MeV, when…

高能物理 - 唯象学 · 物理学 2007-05-23 Wojciech Krolikowski

By assuming the existence of a pseudopotential smooth enough to do Hartree-Fock variations and good enough to describe nuclear structure, we construct mass formulae that rely on general scaling arguments and on a schematic reading of shell…

核理论 · 物理学 2008-11-26 J. Duflo , A. P. Zuker

When three Majorana neutrinos describe the solar and atmospheric neutrino data via oscillations, a nonzero measurement of neutrinoless double beta ($0\nu\beta\beta$) decay can determine the sum of neutrino masses $\sum m_\nu$ if the solar…

高能物理 - 唯象学 · 物理学 2009-09-15 V. Barger , K. Whisnant