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相关论文: Cosmological implications of a class of SO(10) mod…

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We report on some phenomenological implications of a class of unified models based on SO(10) gauge group, with intermediate symmetry group containing SU(2)_R. Interesting predictions for neutrino masses are discussed, which are relevant…

高能物理 - 唯象学 · 物理学 2007-05-23 F. Buccella , G. Mangano , L. Rosa

We review the status of a class of gauge unified models based on SO(10) group. After a pedagogical introduction to SO(10) gauge theories, we discuss the main phenomenological implications of these models. The upper limit on proton lifetime…

高能物理 - 唯象学 · 物理学 2011-04-15 F. Buccella , G. Mangano , O. Pisanti , L. Rosa

The implications on neutrino physics and on the dynamical generation of the baryonic asymmetry of a class of $SO(10)$ non-supersymmetric models are discussed.

高能物理 - 唯象学 · 物理学 2009-10-28 G. Amelino-Camelia , O. Pisanti , L. Rosa

We review the status of a class of gauge unified models based on SO(10) group and discuss the main phenomenological implications of these models in particular for neutrino masses.

高能物理 - 唯象学 · 物理学 2007-05-23 F. Buccella , O. Pisanti

We review in this talk various SUSY SO(10) models. Specifically, we discuss how small neutrino masses are generated in and generic predictions of different SO(10) models. A comparison of the predictions of these models for…

高能物理 - 唯象学 · 物理学 2009-11-10 Mu-Chun Chen , K. T. Mahanthappa

In this talk I discuss the qualitative features of an SO(10) SUSY GUT with an SU(2)x U(1)$^n$ family symmetry. I then describe the global fit of this theory to precision electroweak data [including charged fermion masses and mixing angles].…

高能物理 - 唯象学 · 物理学 2009-10-31 Stuart Raby

Massive neutrinos are a generic prediction of SO(10), and models of unification cry for supersymmetry. Since we have a rather detailed information on neutrino and charged fermion masses, the real question is: how/whether it is possible to…

高能物理 - 唯象学 · 物理学 2007-05-23 Borut Bajc , Goran Senjanovic , Francesco Vissani

Cosmological consequences of a coupling between massive neutrinos and dark energy are investigated. In such models, the neutrino mass is a function of a scalar field, which plays the role of dark energy. The background evolution, as well as…

天体物理学 · 物理学 2010-04-06 A. W. Brookfield , C. van de Bruck , D. F. Mota , D. Tocchini-Valentini

The implications of the deficit of solar neutrinos are discussed. If all of the experiments are taken literally the relative suppressions render an astrophysical explanation unlikely. Allowing MSW conversions, the data simultaneously…

高能物理 - 唯象学 · 物理学 2007-05-23 Paul Langacker

It was recently suggested that in a class of supersymmetric SO(10) models with Higgs multiplets in 10, and a single $126+\bar{126}$ representations, if the $\bar{126}$ contributes both to the right handed neutrino masses as well as to the…

高能物理 - 唯象学 · 物理学 2009-10-30 B. Brahmachari , R. N. Mohapatra

We construct a realistic model based on SUSY SO(10) with U(2) flavor symmetry. A set of symmetric mass textures give rise to very good predictions; 15 masses and 6 mixing angles are predicted by 11 parameters. Both the vacuum oscillation…

高能物理 - 唯象学 · 物理学 2007-05-23 Mu-Chun Chen , K. T. Mahanthappa

In the last few years physicists have been looking at $SO(10)$ GUT models with renewed attention because it has been realized that the SU(5) minimal model cannot unify the strong, electromagnetic and weak interactions in a way consistent…

高能物理 - 唯象学 · 物理学 2009-09-25 F. Acampora , G. Amelino-Camelia , F. Buccella , O. Pisanti , L. Rosa , T. Tuzi

Cosmology yields the most restrictive limits on neutrino masses and conversely, massive neutrinos would contribute to the cosmic dark-matter density and would play an important role for the formation of structure in the universe. Neutrino…

高能物理 - 唯象学 · 物理学 2015-06-25 G. G. Raffelt

The symmetry between quarks and leptons suggests that neutrinos should have mass. As embodied in the grand unified theory SO(10) this yields masses that can only be detected by neutrino oscillations. Such oscillations could be very…

高能物理 - 唯象学 · 物理学 2008-11-26 Lincoln Wolfenstein

We present a systematic search for SUSY-SO(10) models which predict the neutrino properties. The models are based on the five sets of quark mass matrices, with texture zeros, discussed recently by Roberts, Ramond and Ross. We found 8 such…

高能物理 - 唯象学 · 物理学 2016-09-01 Y. Achiman , T. Greiner

The simplest scenario for the three known light neutrinos that fits the solar and atmospheric neutrino deficit and a mixed dark matter (MDM) picture of the universe requires them to be highly degenerate with $m_{\nu} \sim$ 1 - 2 eV. We…

高能物理 - 唯象学 · 物理学 2009-10-28 D. G. Lee , R. N. Mohapatra

We show that certain models for neutrino masses that lead to the MSW explanation of the solar neutrino data and/or the hot dark matter component in the universe can also naturally allow for the successful generation of the cosmological…

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

In this work a mass model based on a SO(10) GUT with a global U(1) family symmetry is discussed which leads to an asymmetric Nearest Neighbour Interaction structure for the fermionic mass matrices. As a result of the analysis one gets three…

高能物理 - 唯象学 · 物理学 2009-09-25 Carsten Merten

Astrophysical and cosmological arguments and observations give us the most restrictive constraints on neutrino masses, electromagnetic couplings, and other properties. Conversely, massive neutrinos would contribute to the cosmic dark-matter…

高能物理 - 唯象学 · 物理学 2007-05-23 Georg G. Raffelt

In this paper we consider the cosmological implications of dark energy models with a coupled system of a dynamical scalar field (the quintessence) and the neutrinos. By detailed numerical calculations we study the various possibilities on…

高能物理 - 唯象学 · 物理学 2007-05-23 Xiao-Jun Bi , Bo Feng , Hong Li , Xinmin Zhang
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