613 research outputs found

    Lepton Masses in a Minimal Model with Triplet Higgs Bosons and S3S_3 Flavor Symmetry

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    Viable neutrino and charged lepton masses and mixings are obtained by imposing a S3×Z4×Z3S_3 \times Z_4 \times Z_3 flavor symmetry in a model with a few additional Higgs. We use two SU(2)LSU(2)_L triplet Higgs which are arranged as a doublet of S3S_3, and standard model singlet Higgs which are also put as doublets of S3S_3. We break the S3S_3 symmetry in this minimal model by giving vacuum expectation values (VEV) to the additional Higgs fields. Dictated by the minimum condition for the scalar potential, we obtain certain VEV alignments which allow us to maintain μτ\mu-\tau symmetry in the neutrino sector, while breaking it maximally for the charged leptons. This helps us to simultaneously explain the hierarchical charged lepton masses, and the neutrino masses and mixings. In particular, we obtain maximal θ23\theta_{23} and zero θ13\theta_{13}. We allow for a mild breaking of the μτ\mu-\tau symmetry for the neutrinos and study the phenomenology. We give predictions for θ13\theta_{13} and the CP violating Jarlskog invariant JCPJ_{CP}, as a function of the μτ\mu-\tau symmetry breaking parameter. We also discuss possible collider signatures and phenomenology associated with lepton flavor violating processes.Comment: 29 pages, 5 figures. Version to be appeared in PRD. Phenomenology of Lepton flavor violation and possible collider signatures of this model have been include

    A Note on Estimation of Population Mean in Sample Survey using Auxiliary Information

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    In this paper we have suggested a class of estimators for population mean using auxiliary information in two-phase sampling. When the population mean  is not known, a class of estimators for finite population mean  of the study variable y has been suggested. Expressions of bias and mean squared error are obtained upto the first order of approximation. Asymptotically optimum estimators (AOE’s) are also identified with its mean squared error formula. We found that proposed class of estimator are better than usual ratio and other estimators

    A review: Solar cell current scenario and future trends

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    In recent years solar cell technology has achieved tremendous growth as sustainable source of energy. In last few years photovoltaic industries have emerged with an annual growth of 40%.Solar cells are renewable pollution free source of electrical energy which can easily replace traditional fossil fuels. In this article we have reviewed the previous and current status of various generations of solar cells and discussed about their future trends and aspects.&nbsp

    Research and development work on substitute electrical resistance alloys for heating elements

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    From the start of the Second Five- Year Plan great emphasis has been laid on production and utilisation of electric power in various industrial and domestic appliances. Electric heating is thus gradually repla- cing solid-fuels, gas and oil heating . Increasing application of electric heat with all its attendant advantages will fail to register full impact unless suitable electrical heating elements , having long high temperature service life are indigenously avai- lable at reasonable cost

    Confusing Sterile Neutrinos with Deviation from Tribimaximal Mixing at Neutrino Telescopes

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    We expound the impact of extra sterile species on the ultra high energy neutrino fluxes in neutrino telescopes. We use three types of well-known flux ratios and compare the values of these flux ratios in presence of sterile neutrinos, with those predicted by deviation from the tribimaximal mixing scheme. We show that in the upcoming neutrino telescopes, its easy to confuse between the signature of sterile neutrinos with that of the deviation from tribimaximal mixing. We also show that if the measured flux ratios acquire a value well outside the range predicted by the standard scenario with three active neutrinos only, it might be possible to tell the presence of extra sterile neutrinos by observing ultra high energy neutrinos in future neutrino telescopes.Comment: 22 pages, version to appear in Phys. Rev.

    An integrated magnetic programming technique for mechanical microresonators

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    Mechanical memory devices are needed for harsh environments where electronic components fail to operate. An integrated electro-Thermal technique for local magnetic annealing, which enables post-production programming capabilities for mechanical micro-resonators is presented. It is verified by a prototype with ferromagnetic resonating elements suspended on top of a polysilicon resistive heater. The magnetization (M-H) loop, with and without post-fabrication annealing are measured to prove the validity of technique.</p

    An integrated magnetic programming technique for mechanical microresonators

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    Mechanical memory devices are needed for harsh environments where electronic components fail to operate. An integrated electro-Thermal technique for local magnetic annealing, which enables post-production programming capabilities for mechanical micro-resonators is presented. It is verified by a prototype with ferromagnetic resonating elements suspended on top of a polysilicon resistive heater. The magnetization (M-H) loop, with and without post-fabrication annealing are measured to prove the validity of technique.</p

    Influence of backward-facing step on the mixing efficiency of multi microjets at supersonic flow

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    © 2020 IAA The injection of the fuel is a highly important process for the enhancement of the scramjets. In this article, the presence of the backward-facing step on the mixing of the multi-fuel jets is expansively studied. The primary attention of this article is to scrutinize the flow feature of the fuel jet under the backward-facing step. The mixing mechanism of the fuel is also studied to compare this injection system with conventional methods. To do this, a 3-dimensional model is chosen to consider the real physic of the problem. Reynolds Average Navier-Stocks equations are solved with a computational fluid dynamic method to visualize the flow pattern of the fuel jet at the free stream Mach number of 4. SST turbulence model is also used for the calculation of the viscosity. Our results indicate that increasing the jet space from 4 to 10 times of jet diameter in the presence of the backward-facing step increases the mixing efficiency up to 20% in the downstream. Our findings depict that augmenting the number of fuel injectors from 4 to 8 augments the mixing rate up to 15% inside the combustor

    On the Mass Eigenstate Composition of the 8B Neutrinos from the Sun

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    The present data of gallium experiments provide indirectly the only experimental limit on the fraction of ν2\nu_2 mass eigenstate for the 8^8B neutrinos from the Sun. However, if to use the experimental data alone, the fraction of ν2\nu_2 and, consequently, sin2θsolsin^2\theta_{sol} still is allowed to be varied within a rather broad range. The further experimental efforts are needed to clear this point.Comment: 13 pages, 1 figure, 1 table. Corrected version, published in JCAP04(2007)00

    Three Generation Neutrino Oscillation Parameters after SNO

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    We examine the solar neutrino problem in the context of the realistic three neutrino mixing scenario including the SNO charged current (CC) rate. The two independent mass squared differences Δm212\Delta m^2_{21} and Δm312Δm322\Delta m^2_{31} \approx \Delta m^2_{32} are taken to be in the solar and atmospheric ranges respectively. We incorporate the constraints on Δ\Deltam312^2_{31} as obtained by the SuperKamiokande atmospheric neutrino data and determine the allowed values of Δm212\Delta m^2_{21}, θ12\theta_{12} and θ13\theta_{13} from a combined analysis of solar and CHOOZ data. Our aim is to probe the changes in the values of the mass and mixing parameters with the inclusion of the SNO data as well as the changes in the two-generation parameter region obtained from the solar neutrino analysis with the inclusion of the third generation. We find that the inclusion of the SNO CC rate in the combined solar + CHOOZ analysis puts a more restrictive bound on θ13\theta_{13}. Since the allowed values of θ13\theta_{13} are constrained to very small values by the CHOOZ experiment there is no qualitative change over the two generation allowed regions in the Δm212tan2θ12\Delta m^2_{21} - \tan^2 \theta_{12} plane. The best-fit comes in the LMA region and no allowed area is obtained in the SMA region at 3σ\sigma level from combined solar and CHOOZ analysis.Comment: One reference added. Version to apprear in PR
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