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      Seesaw induced electroweak scale, the hierarchy problem and sub-eV neutrino masses

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          Abstract

          We describe a model for the scalar sector where all interactions occur either at an ultra-high scale L_U ~ 10^{16}-10^{19} GeV or at an intermediate scale L_I ~ 10^{9}-10^{11} GeV. The interaction of physics on these two scales results in an SU(2) Higgs condensate at the electroweak (EW) scale, L_{EW}, through a seesaw-like Higgs mechanism, L_{EW} ~ L_I^2/L_U, while the breaking of the SM SU(2)XU(1) gauge symmetry occurs at the intermediate scale L_I. The EW scale is, therefore, not fundamental but is naturally generated in terms of ultra-high energy phenomena and so the hierarchy problem is alleviated. We show that the class of such ``seesaw Higgs'' models predict the existence of sub-eV neutrino masses which are generated through a ``two-step'' seesaw mechanism in terms of the same two ultra-high scales: m_nu ~ L_I^4/L_U^3 ~ L_{EW}^2/L_U. The neutrinos can be either Dirac or Majorana, depending on the structure of the scalar potential. We also show that our seesaw Higgs model can be naturally embedded in theories with tiny extra dimensions of size R ~ 1/L_U ~ 10^{-16} fm, where the seesaw induced EW scale arises from a violation of a symmetry at a distant brane; in particular, in the scenario presented there are 7 tiny extra dimensions.

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          An Alternative to Compactification

          Conventional wisdom states that Newton's force law implies only four non-compact dimensions. We demonstrate that this is not necessarily true in the presence of a non-factorizable background geometry. The specific example we study is a single 3-brane embedded in five dimensions. We show that even without a gap in the Kaluza-Klein spectrum, four-dimensional Newtonian and general relativistic gravity is reproduced to more than adequate precision.
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            Threshold Effects in SO(10) Grandunified Models and Solar Neutrino Puzzle

            , (2009)
            We compute the threshold uncertainties due to unknown masses of the Higgs bosons on the predictions for the intermediate and unification scales, \(M_I\) and \(M_U\) respectively in SO(10) models.We focus on models with separate breaking scales for Parity and \(SU(2)_R\) symmetries since they provide a natural realization of the see-saw mechanism for neutrino masses. For the two step symmetry breaking chains ,where left-right symmetric gauge groups appear at the intermediate scale, we find that parity invariance of the theory at the unification scale drastically reduces the GUT threshold effects in some cases. Including the effects of the intermediate scale thresholds ,we compute the uncertainty in the above mass scales and study their implications for proton lifetime and neutrino masses. An important outcome of our analysis is that if the currently favored nonadiabatic MSW solution to the solar neutrino puzzle is accepted , it will rule out the \(SU(2)_LXSU(2)_RXU(1)_{B-L}X SU(3)_c\) as an intermediate symmetry for SO(10) breaking whereas the intermediate symmetry \(SU(2)_LXSU(2)_RXSU(4)_c\), is quite consistent with it.
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              Verifiable Model of Neutrino Masses from Large Extra Dimensions

              We propose a new scenario of neutrino masses with a Higgs triplet \((\xi^{++},\xi^+,\xi^0)\) in a theory of large extra dimensions. Lepton number violation in a distant brane acts as the source of a very small trilinear coupling of \(\xi\) to the standard Higgs doublet in our brane. Small realistic Majorana neutrino masses are \underline{naturally} obtained with the fundamental scale \(M_* \sim {\cal O}(1)\) TeV, foretelling the possible discovery of \(\xi\) \((m_\xi\lsim M_*)\) at future colliders. Decays of \(\xi^{++}\) into same-sign dileptons are fixed by the neutrino mass matrix. Observation of \(\mu-e\) conversion in nuclei is predicted.
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                Author and article information

                Journal
                17 August 2004
                2005-09-19
                Article
                10.1140/epjc/s2005-02403-x
                hep-ph/0408191
                137acf7b-d066-4c0a-a0bb-52145003a035
                History
                Custom metadata
                BNL-HET-04/10
                Eur.Phys.J.C45:219-225,2006
                latex, 25 pages, no figures. Version 2 is a shorter version (as accepted in EPJC), not including the discussion on the heavy seesaw Higgs model
                hep-ph

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