3,365 research outputs found

    Vanishing Str M^2 in the presence of anomalous U_A(1)

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    We show that the presence of an anomalous UA(1)\rm U_A(1) factor in the gauge group of string-derived models may have the new and important phenomenological consequence of allowing the vanishing of StrM2{\rm Str}\,{\cal M}^2 in the ``shifted" vacuum, that results in the process of cancelling the anomalous UA(1)\rm U_A(1). The feasibility of this effect seems to be enhanced by a vanishing vacuum energy, and by a ``small" value of StrM2{\rm Str}\,{\cal M}^2 in the original vacuum. In the class of free-fermionic models with vanishing vacuum energy that we focus on, a necessary condition for this mechanism to be effective is that StrM2>0{\rm Str}\,{\cal M}^2>0 in the original vacuum. A vanishing StrM2{\rm Str}\,{\cal M}^2 ameliorates the cosmological constant problem and is a necessary element in the stability of the no-scale mechanism.Comment: 7 pages, no figures, LaTe

    Direct detection of dark matter in SU(5)xU(1) supergravity

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    We compute the scattering rates for the lightest neutralino χ10\chi^0_1 in the forthcoming germanium (73Ge+76Ge)(^{73}{\rm Ge}+^{76}{\rm Ge}) detector and a proposed lead detector (207Pb)(^{207}{\rm Pb}), within the framework of SU(5)×U(1)SU(5)\times U(1) supergravity. We find that in only a small portion (\lsim10\%) of the parameter spaces of this class of models, are the rates in the germanium detector above the expected initial experimental sensitivity of 0.1 events/kg/day. However, a much larger portion (\lsim40\%) of the parameter spaces could be probed with an improved background rejection capability (0.01 events/kg/day) and/or a more sensitive detector (207Pb)(^{207}{\rm Pb}).Comment: 10 pages, Latex, 4 figures included (uuencoded

    LEP and radiative electroweak breaking close the light gluino window

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    We show that the LEP lower bound on the chargino mass, in conjunction with the well motivated theoretical requirement of radiative electroweak symmetry breaking, imply an upper bound on the lightest Higgs boson mass (m_h\lsim62\GeV) in a supersymmetry breaking scenario where the gluino mass is a few GeV. Moreover, Higgs searches at LEP in the context of this model require m_h\gsim61\GeV. The remaining experimentally allowed region in the five-dimensional parameter space of this light gluino model is severely fine-tuned (with tanβ=1.881.89\tan\beta=1.88-1.89 and m_t=114.0-114.3\GeV) and cosmologically troublesome (with a neutralino relic abundance over {\it five-hundred times larger than allowed}). Modest improvements in sensitivity in LEP Higgs searches and Tevatron top-quark searches should soon exclude this theoretically disfavored model completely.Comment: 6 pages, no figures, tex (harvmac), CERN-TH.6890, CTP-TAMU-25/9

    String Unification and Leptophobic ZZ' in Flipped SU(5)

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    We summarize recent developments in the prediction for αs(MZ)\alpha_s(M_Z), self-consistent string unification and the dynamical determination of mass scales, and leptophobic ZZ' gauge bosons in the context of stringy flipped SU(5). [To appear in Proceedings of Fourth International Conference on Supersymmetry (SUSY96), University of Maryland (May 1996).]Comment: 5 pages, LaTeX (uses espcrc2.sty), 5 figures (included

    The top-quark mass in SU(5)xU(1) supergravity

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    We show that the currently experimentally preferred values of the top-quark mass (\ie, 130\lsim m_t\lsim180\GeV) are naturally understood in the context of string models, where the top-quark Yukawa coupling at the string scale is generically given by λt=O(g)\lambda_t={\cal O}(g), with gg the unified gauge coupling. A detailed study of the Yukawa sector of SU(5)×U(1)SU(5)\times U(1) supergravity shows that the ratio of the bottom-quark to tau-lepton Yukawa couplings at the string scale is required to be in the range 0.7\lsim\lambda_b/\lambda_\tau\lsim1, depending on the values of mtm_t and mbm_b. This result is consistent with SU(5)×U(1)SU(5)\times U(1) symmetry, which does {\em not} require the equality of these Yukawa couplings in the unbroken symmetry phase of the theory. As a means of possibly predicting the value of mtm_t, we propose a procedure whereby the size of the allowed parameter space is determined as a function of mtm_t, since all sparticle and Higgs-boson masses and couplings depend non-trivially on mtm_t. At present, no significant preference for particular values of mtm_t in SU(5)×U(1)SU(5)\times U(1) supergravity is observed, except that high-precision LEP data requires m_t\lsim180\GeV.Comment: latex, 10 pages, 4 figures (included), CERN-TH.7138/94, CTP-TAMU-05/9

    The Search for a realistic flipped SU(5) string model

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    We present an extensive search for a general class of flipped SU(5)SU(5) models built within the free fermionic formulation of the heterotic string. We describe a set of algorithms which constitute the basis for a computer program capable of generating systematically the massless spectrum and the superpotential of all possible models within the class we consider. Our search through the huge parameter space to be explored is simplified considerably by the constraint of N=1N=1 spacetime supersymmetry and the need for extra Q,QˉQ,\bar Q representations beyond the standard ones in order to possibly achieve string gauge coupling unification at scales of {\cal O}(10^{18}\GeV). Our results are remarkably simple and evidence the large degree of redundancy in this kind of constructions. We find one model with gauge group SU(5)\times U(1)_\ty\times SO(10)_h\times SU(4)_h\times U(1)^5 and fairly acceptable phenomenological properties. We study the DD- and FF-flatness constraints and the symmetry breaking pattern in this model and conclude that string gauge coupling unification is quite possible.Comment: 44 page

    Supersymmetric photonic signals at LEP

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    We explore and contrast the single-photon and diphoton signals expected at LEP 2, that arise from neutralino-gravitino (e^+ e^- -> chi + gravitino -> gamma + E_miss) and neutralino-neutralino (e^+ e^- -> chi + chi -> gamma + gamma + E_miss) production in supersymmetric models with a light gravitino. LEP 1 limits imply that one may observe either one, but not both, of these signals at LEP 2, depending on the values of the neutralino and gravitino masses: single-photons for m_chi > Mz and m_gravitino < 3 x 10^-5 eV; diphotons for m_chi < Mz and all allowed values of m_gravitino.Comment: 11 pages, LaTeX, 4 figures (included). Shortened version to appear in Physical Review Letter

    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 MLEP101516M_{\rm LEP}\sim10^{15-16}~GeV scale, and the M51M_{51} scale of SU(5) and U(1) unification with the theoretical Mstring5×1017M_{\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

    Status of the superworld: from theory to experiment

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    Review to appear in Progress in Particle and Nuclear Physics. Contents: {1}Introduction}{1} {2}High precision LEP data and convergence of couplings: physics is not Euclidean geometry}{2} {3}Interconnections between the measured quantities due to Unification}{7} {4}The origin of MSUSYM_{SUSY} and why it should be abandoned: masses and spectra are needed}{13} {5}The new step forward: Supergravity}{21} {6}The SU(5) Supergravity Model}{22} {7}SU(5)xU(1) Supergravity}{32} {8}Detailed calculations for the Tevatron}{47} {9}Detailed calculations for LEP}{48} {10}Detailed calculations for HERA}{53} {11}Detailed calculations for Underground Labs and Underwater facilities}{55} {12}Detailed calculations for indirect experimental detection}{65} {13}The problem of mass and mtm_t}{73} {14}Conclusions}{77}Comment: 90 pages, 41 figures (not included), latex. Send requests for hard copies to "[email protected]". CERN-TH.7136/94, CTP-TAMU-80/9
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