20,081 research outputs found

    Tunneling into fractional quantum Hall liquids

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    Motivated by the recent experiment by Grayson et.al., we investigate a non-ohmic current-voltage characteristics for the tunneling into fractional quantum Hall liquids. We give a possible explanation for the experiment in terms of the chiral Tomonaga-Luttinger liquid theory. We study the interaction between the charge and neutral modes, and found that the leading order correction to the exponent α\alpha (I∌Vα)(I\sim V^\alpha) is of the order of Ï”\sqrt{\epsilon} (Ï”=vn/vc)(\epsilon=v_n/v_c), which reduces the exponent α\alpha. We suggest that it could explain the systematic discrepancy between the observed exponents and the exact α=1/Îœ\alpha =1/\nu dependence.Comment: Latex, 5 page

    A Layman's guide to SUSY GUTs

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    The determination of the most straightforward evidence for the existence of the Superworld requires a guide for non-experts (especially experimental physicists) for them to make their own judgement on the value of such predictions. For this purpose we review the most basic results of Super-Grand unification in a simple and clear way. We focus the attention on two specific models and their predictions. These two models represent an example of a direct comparison between a traditional unified-theory and a string-inspired approach to the solution of the many open problems of the Standard Model. We emphasize that viable models must satisfy {\em all} available experimental constraints and be as simple as theoretically possible. The two well defined supergravity models, SU(5)SU(5) and SU(5)×U(1)SU(5)\times U(1), can be described in terms of only a few parameters (five and three respectively) instead of the more than twenty needed in the MSSM model, \ie, the Minimal Supersymmetric extension of the Standard Model. A case of special interest is the strict no-scale SU(5)×U(1)SU(5)\times U(1) supergravity where all predictions depend on only one parameter (plus the top-quark mass). A general consequence of these analyses is that supersymmetric particles can be at the verge of discovery, lurking around the corner at present and near future facilities. This review should help anyone distinguish between well motivated predictions and predictions based on arbitrary choices of parameters in undefined models.Comment: 25 pages, Latex, 11 figures (not included), CERN-TH.7077/93, CTP-TAMU-65/93. A complete ps file (1.31MB) with embedded figures is available by request from [email protected]

    A new scenario for string unification

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    We present a new scenario for gauge coupling unification in flipped SU(5) string models, which identifies the M32M_{32} scale of SU(3) and SU(2) unification with the empirical MLEP∌1015−16M_{\rm LEP}\sim10^{15-16}~GeV scale, and the M51M_{51} scale of SU(5) and U(1) unification with the theoretical Mstring∌5×1017M_{\rm string}\sim5\times10^{17}~GeV string unification scale. The vacuum shift necessary for the cancellation of the anomalous UA(1)\rm U_A(1) and an SU(4) hidden sector with fractionally-charged particles, play a crucial role in the dynamical determination of all intermediate mass scales in this scenario.Comment: 8 pages, LaTeX, 2 figures (uuencoded

    Inferring Energy Bounds via Static Program Analysis and Evolutionary Modeling of Basic Blocks

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    The ever increasing number and complexity of energy-bound devices (such as the ones used in Internet of Things applications, smart phones, and mission critical systems) pose an important challenge on techniques to optimize their energy consumption and to verify that they will perform their function within the available energy budget. In this work we address this challenge from the software point of view and propose a novel parametric approach to estimating tight bounds on the energy consumed by program executions that are practical for their application to energy verification and optimization. Our approach divides a program into basic (branchless) blocks and estimates the maximal and minimal energy consumption for each block using an evolutionary algorithm. Then it combines the obtained values according to the program control flow, using static analysis, to infer functions that give both upper and lower bounds on the energy consumption of the whole program and its procedures as functions on input data sizes. We have tested our approach on (C-like) embedded programs running on the XMOS hardware platform. However, our method is general enough to be applied to other microprocessor architectures and programming languages. The bounds obtained by our prototype implementation can be tight while remaining on the safe side of budgets in practice, as shown by our experimental evaluation.Comment: Pre-proceedings paper presented at the 27th International Symposium on Logic-Based Program Synthesis and Transformation (LOPSTR 2017), Namur, Belgium, 10-12 October 2017 (arXiv:1708.07854). Improved version of the one presented at the HIP3ES 2016 workshop (v1): more experimental results (added benchmark to Table 1, added figure for new benchmark, added Table 3), improved Fig. 1, added Fig.

    The dilaton-dominated supersymmetry breaking scenario in the context of the non-minimal supersymmetric model

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    The phenomenological consequences of the dilaton-type soft supersymmetry breaking terms in the context of the next to minimal supersymmetric standard model are investigated. We always find a very low top quark mass. As a consequence such string vacua are excluded by recent experimental results. The viability of the solution of the Ό\mu term through the introduction of a gauge singlet field is also briefly discussed.Comment: 10 pages,LATE

    SUSY signals at HERA in the no-scale flipped SU(5) supergravity model

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    Sparticle production and detection at HERA are studied within the recently proposed no-scale flipped SU(5)SU(5) supergravity model. Among the various reaction channels that could lead to sparticle production at HERA, only the following are within its limit of sensitivity in this model: e−p→e~L,R−χi0+X,Îœ~eχ1−+Xe^-p\to \tilde e^-_{L,R}\chi^0_i+X, \tilde \nu_e\chi^-_1+X, where χi0(i=1,2)\chi^0_i(i=1,2) are the two lightest neutralinos and χ1−\chi^-_1 is the lightest chargino. We study the elastic and deep-inelastic contributions to the cross sections using the Weizs\"acker-Williams approximation. We find that the most promising supersymmetric production channel is right-handed selectron (e~R\tilde e_{R}) plus first neutralino (χ10\chi^0_1), with one hard electron and missing energy signature. The Îœ~eχ1−\tilde\nu_e\chi^-_1 channel leads to comparable rates but also allows jet final states. A right-handedly polarized electron beam at HERA would shut off the latter channel and allow preferentially the former one. With an integrated luminosity of {\cal L}=100\ipb, HERA can extend the present LEPI lower bounds on me~R,mÎœ~e,mχ10m_{\tilde e_R}, m_{\tilde\nu_e},m_{\chi^0_1} by \approx25\GeV, while {\cal L}=1000\ipb will make HERA competitive with LEPII. We also show that the Leading Proton Spectrometer (LPS) at HERA is an excellent supersymmetry detector which can provide indirect information about the sparticle masses by measuring the leading proton longitudinal momentum distribution.Comment: 11 pages, 8 figures (available upon request as uuencoded file or separate ps files), tex (harvmac) CTP-TAMU-15/93, CERN/LAA/93-1

    Precision Electroweak Tests of the Minimal and Flipped SU(5) Supergravity Models

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    We explore the one-loop electroweak radiative corrections in the minimal SU(5)SU(5) and the no-scale flipped SU(5)SU(5) supergravity models via explicit calculation of vacuum polarization contributions to the ϔ1,2,3\epsilon_{1,2,3} parameters. Experimentally, ϔ1,2,3\epsilon_{1,2,3} are obtained from a global fit to the LEP observables, and MW/MZM_W/M_Z measurements. We include q2q^2-dependent effects which have been neglected in most previous ``model-independent" analyses of this type. These effects induce a large systematic negative shift on ϔ1,2,3\epsilon_{1,2,3} for light chargino masses (m_{\chi^\pm_1}\lsim70\GeV). In agreement with previous general arguments, we find that for increasingly large sparticle masses, the heavy sector of both models rapidly decouples, \ie, the values for ϔ1,2,3\epsilon_{1,2,3} quickly asymptote to the Standard Model values with a {\it light} Higgs (m_{H_{SM}}\sim100\GeV). Specifically, at present the 90%90\% CL upper limit on the top-quark mass is m_t\lsim175\GeV in the no-scale flipped SU(5)SU(5) supergravity model. These bounds can be strengthened for increasing chargino masses in the 50-100\GeV interval. In particular, for m_t\gsim160\GeV, the Tevatron may be able to probe through gluino(g~\tilde g) and squark(q~\tilde q) production up to m_{\tilde g}\approx m_{\tilde q}\approx250\GeV, exploring at least half of the parameter space in this model.Comment: 15 pages,(6 ps figures available upon request), TeX(harvmac), CTP-TAMU-19/93, ACT-07/9

    Crossing the Phantom Divide Line in a DGP-Inspired F(R,ϕ)F(R,\phi)-Gravity

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    We study possible crossing of the phantom divide line in a DGP-inspired F(R,ϕ)F(R,\phi) braneworld scenario where scalar field and curvature quintessence are treated in a unified framework. With some specific form of F(R,ϕ)F(R,\phi) and by adopting a suitable ansatz, we show that there are appropriate regions of the parameters space which account for late-time acceleration and admit crossing of the phantom divide line.Comment: 23 Pages, 10 figs, Submitted to JCA

    Experimental aspects of SU(5)xU(1) supergravity

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    We study various aspects of SU(5)×U(1)SU(5)\times U(1) supergravity as they relate to the experimental verification or falsification of this model. We consider two string-inspired, universal, one-parameter, no-scale soft-supersymmetry-breaking scenarios, driven by the FF-terms of the moduli and dilaton fields. The model is described in terms of the supersymmetry mass scale (\ie, the chargino mass mχ1±m_{\chi^\pm_1}), tan⁥ÎČ\tan\beta, and the top-quark mass. We first determine the combined effect on the parameter space of all presently available direct and indirect experimental constraints, including the LEP lower bounds on sparticle and Higgs-boson masses, the b→sÎłb\to s\gamma rate, the anomalous magnetic moment of the muon, the high-precision electroweak parameters Ï”1,Ï”b\epsilon_1,\epsilon_b (which imply m_t\lsim180\GeV), and the muon fluxes in underground detectors (neutrino telescopes). For the still-allowed points in (mχ1±,tan⁥ÎČ)(m_{\chi^\pm_1},\tan\beta) parameter space, we re-evaluate the experimental situation at the Tevatron, LEPII, and HERA. In the 1994 run, the Tevatron could probe chargino masses as high as 100 GeV. At LEPII the parameter space could be explored with probes of different resolutions: Higgs boson searches, selectron searches, and chargino searches. Moreover, for m_t\lsim150\GeV, these Higgs-boson searches could explore all of the allowed parameter space with \sqrt{s}\lsim210\GeV.Comment: latex, 36 pages, 25 figures (not included). Figures are available via anonymous ftp from hplaa02.cern.ch (/pub/lopez) as either 33 ps files (Easpects*.ps, 8.1MB) or one uuencoded file (AllFigures.uu, 3.7MB

    Comment on "Contribution of drifting carriers to the Casimir-Lifshitz and Casimir-Polder interactions with semiconductor materials"

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    Recently D. A. R. Dalvit and S. K. Lamoreaux arXiv:0805.1676 [Phys. Rev. Lett. v.101, 163203 (2008)] suggested the modification of the reflection coefficients in the Lifshitz theory taking into account the screening effects and diffusion currents. We demonstrate that the suggested modification is thermodynamically and experimentally inconsistent.Comment: 2 pages, 1 figure; minor revisions are made in accordance with the text accepted for publication in Phys. Rev. Let
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