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相关论文: Renormalization Group Evolution of Dirac Neutrino …

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Starting with 'High Scale Mixing Unification' hypothesis, we investigate the renormalization group evolution of mixing parameters and masses for both Dirac and Majorana type neutrinos. Following this hypothesis, the PMNS mixing parameters…

高能物理 - 唯象学 · 物理学 2016-04-20 Rahul Srivastava

Starting with high scale mixing unification hypothesis, we investigate the renormalization group evolution of mixing parameters and masses for Dirac type neutrinos. Following this hypothesis, the PMNS mixing angles and phase are taken to be…

高能物理 - 唯象学 · 物理学 2015-07-01 Gauhar Abbas , Saurabh Gupta , G. Rajasekaran , Rahul Srivastava

We present a scenario of neutrino masses and mixing angles. Each generation includes a sterile right handed neutrino in addition to the usual left handed one. We assume a hierarchy in their Dirac masses similar to, but much larger than the…

高能物理 - 唯象学 · 物理学 2016-08-24 D. Ring

The neutrino mixing parameters are thoroughly studied using renormalization-group evolution of Dirac neutrinos with recently proposed parametrization of the neutrino mixing angles referred as `high-scale mixing relations'. The correlations…

高能物理 - 唯象学 · 物理学 2017-04-07 Gauhar Abbas , Mehran Zahiri Abyaneh , Rahul Srivastava

We derive simple analytical formulae for the renormalization group running of neutrino masses, leptonic mixing angles and CP phases, which allow an easy understanding of the running. Particularly for a small angle theta_13 the expressions…

高能物理 - 唯象学 · 物理学 2015-06-25 Stefan Antusch , Joern Kersten , Manfred Lindner , Michael Ratz

It is found that the seesaw mechanism not only explains the smallness of neutrino masses but also accounts for the large mixing angles simultaneously, even if the unification of the neutrino Dirac mass matrix with that of up-type quark…

高能物理 - 唯象学 · 物理学 2009-11-11 H. Tsujimoto

Enlightened by the idea of the 3 times 3 CKM angle matrix proposed recently by Harrison et al., we introduce the Dirac angle matrix Phi and the Majorana angle matrix Psi in the lepton sector for Dirac and Majorana neutrinos respectively. We…

高能物理 - 唯象学 · 物理学 2015-05-30 Shu Luo

The renormalization of general theories with inter-family mixing of Dirac and/or Majorana fermions is studied at the one-loop electroweak order. The phenomenological significance of the mixing-matrix renormalization is discussed, within the…

高能物理 - 唯象学 · 物理学 2009-10-28 Bernd A. Kniehl , Apostolos Pilaftsis

We study mixing of the Dirac neutrinos in the residual symmetries approach. The key difference from the Majorana case is that the Dirac mass matrix may have larger symmetries: $G_\nu=\mathbf{Z}_{n}$ with $n\geq3$. The symmetry group…

高能物理 - 唯象学 · 物理学 2015-12-02 Arman Esmaili , Alexei Yu. Smirnov

If neutrinos have masses, why are they so tiny? Are these masses of the Dirac type or of the Majorana type? We are already familiar with the mechanism of how to obtain a tiny Majorana neutrino mass by the famous see-saw mechanism. The…

高能物理 - 唯象学 · 物理学 2009-10-31 P. Q. Hung

Renormalization group (RG) evolution of the neutrino mass matrix may take the value of the mixing angle $\theta_{13}$ very close to zero, or make it vanish. On the other hand, starting from $\theta_{13}=0$ at the high scale it may be…

高能物理 - 唯象学 · 物理学 2010-04-28 Amol Dighe , Srubabati Goswami , Shamayita Ray

The observed pattern of neutrino mixing angles is in good agreement with the hypothesis of neutrino anarchy, which posits that Nature has chosen the entries of the leptonic mixing matrix at random. In this paper we investigate how stable…

高能物理 - 唯象学 · 物理学 2016-05-27 Vedran Brdar , Matthias König , Joachim Kopp

The most plausible see-saw explanation of the smallness of the neutrino masses is based on the assumption that total lepton number is violated at a large scale and neutrinos with definite masses are Majorana particles. In this review we…

高能物理 - 唯象学 · 物理学 2009-11-11 S. M. Bilenky

Motivated by the Super-Kamiokande atmospheric neutrino data, we discuss possible textures for Majorana and Dirac neutrino masses within the see-saw framework. The main purposes of this paper are twofold: first to obtain intuition from a…

高能物理 - 唯象学 · 物理学 2009-09-11 J. Ellis , G. K. Leontaris , S. Lola , D. V. Nanopoulos

The high scale mixing unification hypothesis recently proposed by three of us (R. N. M., M. K. P. and G. R.) states that if at the seesaw scale, the quark and lepton mixing matrices are equal then for quasi-degenerate neutrinos, radiative…

高能物理 - 唯象学 · 物理学 2008-11-26 S. K. Agarwalla , M. K. Parida , R. N. Mohapatra , G. Rajasekaran

We consider a scenario for the Quark-Lepton Complementarity relations between mixing angles in which the bi-maximal mixing follows from the neutrino mass matrix. According to this scenario in the lowest order the angle \theta_{12} is \sim…

高能物理 - 唯象学 · 物理学 2008-11-26 Michael A. Schmidt , Alexei Yu. Smirnov

The Littlest Seesaw (LS) model involves two right-handed neutrinos and a very constrained Dirac neutrino mass matrix, involving one texture zero and two independent Dirac masses, leading to a highly predictive scheme in which all neutrino…

高能物理 - 唯象学 · 物理学 2016-12-12 Stephen F. King , Jue Zhang , Shun Zhou

We investigate the renormalization group evolution of masses and mixing angles of Majorana neutrinos under the `High Scale Mixing Unification' hypothesis. Assuming the unification of quark-lepton mixing angles at a high scale, we show that…

高能物理 - 唯象学 · 物理学 2014-05-23 Gauhar Abbas , Saurabh Gupta , G. Rajasekaran , Rahul Srivastava

We derive renormalization group equations for neutrino masses, leptonic mixing angles and CP-violating phases running at energies above the seesaw threshold, both in the Standard Model and in the Minimal Supersymmetric Standard Model…

高能物理 - 唯象学 · 物理学 2009-11-11 Jianwei Mei

Majorana CP violating phases coming from heavy right-handed Majorana mass matrices ($M_{RR}$) are considered to estimate the masses of neutrinos.The effects of phases on quasi-degenerate neutrinos mass matrix obeying $\mu$-$\tau$ symmetry…

高能物理 - 唯象学 · 物理学 2023-11-28 Ng. K. Francis
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