7,029 research outputs found

    Neutrino Mass, Dark Matter, and Leptogenesis

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    It is proposed that dark matter is the origin of neutrino mass, thereby linking inexorably two undisputed (and seemingly unrelated) pieces of evidence for physics beyond the Standard Model. Leptogenesis at the TeV scale may also be possible, as well as a measurable contribution to the muon anomalous magnetic moment.Comment: 7 pages, 2 figure

    Quark Mass Matrices from a Softly Broken U(1) Symmetry

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    Assigning U(1) charges to the quarks of the standard model, and allowing one extra scalar doublet with m^2 > 0, the correct pattern of the up and down quark mass matrices is obtained, together with their charged-current mixing matrix.Comment: 10 pages, no figur

    Gauged B-3L_\tau, low-energy unification and proton decay

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    We point out that if there is a gauged B−3LτB-3L_\tau symmetry at low energy, it can prevent fast proton decay. This may help building models with theories with extra dimensions at the TeV scale. For purpose of illustration we present an explicit model with large extra dimensions. The Higgs required for a realistic fermion masses and mixing are included. The problem of neutrino masses are solved with triplet Higgs scalars. The proton remains stable even after the B−3LτB-3L_\tau symmetry breaking.Comment: 8 pages, Late

    Verifiable Origin of Neutrino Mass at TeV Scale

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    The physics responsible for neutrino mass may reside at or below the TeV energy scale. The neutrino mass matrix in the (Îœe,ΜΌ,Μτ)(\nu_e, \nu_\mu, \nu_\tau) basis may then be deduced from future high-energy accelerator experiments. The newly observed excess in the muon anomalous magnetic moment may also be related.Comment: 9 pages, 1 figure, talk at TAUP 200

    Splitting of Three Nearly Mass-Degenerate Neutrinos

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    Assuming the canonical seesaw mechanism together with an SO(3) family symmetry for leptons, broken only by the charged-lepton masses, I show that the three neutrinos of Majorana mass m0m_0 are split radiatively in two loops by a maximum finite calculable amount of order 10−9m010^{-9} m_0. This is very suitable for dark matter and vacuum solar neutrino oscillations. I also discuss how atmospheric neutrino oscillations can be incorporated.Comment: 11 pages including 1 figure, slightly revised version to appear in Physics Letters

    Tripartite Neutrino Mass Matrix

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    The 3 X 3 Majorana neutrino mass matrix is written as a sum of 3 terms, i.e. M_nu = M_A + M_B + M_C, where M_A is proportional to the identity matrix and M_B and M_C are invariant under different Z_3 transformations. This M_nu is very suitable for understanding atmospheric and solar neutrino oscillations, with sin^2 (2 theta_atm) and tan^2 (theta_sol) fixed at 1 and 0.5 respectively, in excellent agreement with present data. It has in fact been proposed before, but only as an ansatz. This paper uncovers its underlying symmetry, thus allowing a complete theory of leptons and quarks to be constructed.Comment: 9 pages, no figur

    Nearly Mass-Degenerate Majorana Neutrinos: Double Beta Decay and Neutrino Oscillations

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    Assuming equal tree-level Majorana masses for the standard-model neutrinos, either from the canonical seesaw mechanism or from a heavy scalar triplet, I discuss how their radiative splitting may be relevant to neutrinoless double beta decay and neutrino oscillations.Comment: 12 pages, including 4 figures, talk at NANP9

    Neutrino Mass from Triplet and Doublet Scalars at the TeV Scale

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    If the minimal standard model of particle interactions is extended to include a scalar triplet with lepton number L=−2L=-2 and a scalar doublet with L=−1L=-1, neutrino masses mΜ∌Ό124v2/M5∌10−2m_\nu \sim \mu_{12}^4 v^2/M^5 \sim 10^{-2} eV is possible, where v∌102v \sim 10^2 GeV is the electroweak symmetry breaking scale, M∌1M \sim 1 TeV is the typical mass of the new scalars, and ÎŒ12∌1\mu_{12} \sim 1 GeV is a soft lepton-number-violating parameter.Comment: 6 pages, no figur

    Schizophrenic active neutrinos and exotic sterile neutrinos

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    We implement a schizophrenic scenario for the active neutrinos in a model in which there are also exotic right-handed neutrinos making a model with a local U(1)_(B-L) anomaly free. Two of right-handed neutrinos carry B-L=-4 while the third one carries B-L=5.Comment: I, A. C. B. Machado, apologize for having submitted the wrong file before. This is in fact the version to be published in Physics Letters B 698 (2011) pp. 128-13

    Anomalous quantum-critical scaling corrections in two-dimensional antiferromagnets

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    We study the N\'eel-paramagnetic quantum phase transition in two-dimensional dimerized S=1/2S=1/2 Heisenberg antiferromagnets using finite-size scaling of quantum Monte Carlo data. We resolve the long standing issue of the role of cubic interactions arising in the bond-operator representation when the dimer pattern lacks a certain symmetry. We find non-monotonic (monotonic) size dependence in the staggered (columnar) dimerized model, where cubic interactions are (are not) present. We conclude that there is an irrelevant field in the staggered model that is not present in the columnar case, but, at variance with previous claims, it is not the leading irrelevant field. The new exponent is ω2≈1.25\omega_2 \approx 1.25 and the prefactor of the correction L−ω2L^{-\omega_2} is large and comes with a different sign from that of the formally leading conventional correction with exponent ω1≈0.78\omega_1 \approx 0.78. Our study highlights the possibility of competing scaling corrections at quantum critical points.Comment: 6 pages, 6 figure
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