133 research outputs found

    Matching the BPS Spectra of Heterotic - Type I - Type I' Strings

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    We give a detailed discussion of the matching of the BPS states of heterotic, type I and type I' theories in d=9 for general backgrounds. This allows us to explicitly identify these (composite) brane states in the type I' theory that lead to gauge symmetry enhancement at critical points in moduli space. An example is the enhancement of SO(16)×SO(16)SO(16)\times SO(16) to E8×E8E_8\times E_8.Comment: 11 pages; minor typos in eq. (3), (4) and on page 9 have been corrected; two footnotes taking into account additional references have been added; version to appear in Physics Letters

    Implications of non-universality of soft terms in supersymmetric grand unified theories

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    Most discussions of supersymmetric grand unified theories assume universality of the soft supersymmetry breaking terms at the grand scale. We point out that the behaviour of these theories might change significantly in the presence of non--universal soft terms. Particularly in SO(10)--like models with a large value of tanβ\beta we observe a decisive change of predictions, allowing the presence of relatively light gauginos as well as small supersymmetric corrections to the b--quark mass. Some results remain rather stable, including the μ\mu--M1/2M_{1/2} correlation. Models with small tanβ\beta seem to be less affected by non--universality which mainly leads to the new possibility of small m0m_{0} (i.e. the squark and slepton soft mass parameter), excluded in the universal case.Comment: 15 pages (Latex) plus 5 figures (uuencoded postscript file). TUM-HEP 201/9

    Polydisperse Versus Monodisperse Microbubbles:A Simulation Study for Contrast-Enhanced Ultrasound Imaging

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    Objective: Contrast-enhanced ultrasound (CEUS) presents distinct advantages in diagnostic echography. Utilizing microbubbles (MBs) as conventional contrast agents enhances vascular visualization and organ perfusion, facilitating real-time, non-invasive procedures. There is a current tendency to replace traditional polydisperse MBs with novel monodisperse formulations in an attempt to optimize contrast enhancement and guarantee consistent behavior and reliable imaging outcomes. This study investigates the contrast enhancement achieved using various-sized monodisperse MBs and their influence on non-linear imaging artifacts observed in traditional CEUS. Methods: To explore the differences between monodisperse and polydisperse populations without excessive experimentation, numerical simulations are employed for delivering precise, objective and expeditious results. The iterative non-linear contrast source (INCS) method has previously demonstrated efficacy when simulating ultrasound propagation in large populations in which each bubble has individual properties and several orders of multiple scattering are significant. Therefore, this method is employed to realistically simulate both monodisperse and polydisperse MBs. Results: Our findings in CEUS imaging indicate that scattering from resonant monodisperse MBs is 11.8 dB stronger than scattering from polydisperse MBs. Furthermore, the amplitude of non-linear imaging artifacts downstream of the monodisperse population is 19.4 dB stronger compared with polydisperse suspension. Conclusion: Investigating the impact of multiple scattering on polydisperse populations compared with various monodisperse suspensions has revealed that monodisperse MBs are more effective contrast agents, especially when at resonance. Despite the strong signal-to-noise ratio of monodisperse populations, imaging artifacts caused by non-linear wave propagation are also enhanced, resulting in further mis-classification of MBs as tissue.</p

    Nonlinear interaction of two cross-propagating plane waves

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    An ideal contrast-enhanced ultrasound image should display microbubble-induced nonlinearities while avoiding wave propagation nonlinearities. One of the most successful ultrasound pulse sequences to disentangle these nonlinear effects relies on the transmission of cross-propagating plane waves. However, theory describing the noncollinear nonlinear interaction of two finite plane waves has not been fully developed and a better understanding of these effects would improve contrast-enhanced ultrasound imaging further. Here, local nonlinear interactions at the intersection of two plane-waves are investigated by extending the Westervelt equation with a term including the Lagrangian density. The Iterative Nonlinear Contrast Source (INCS) method is employed to numerically solve this full nonlinear wave equation for two 3D finite cross-propagating pulsed plane waves. In addition, analytical expressions for the cross-propagation of two infinite continuous plane waves are derived. Numerical results obtained with INCS show good agreement with the analytical expressions. Overall, the generated results show that the pressure associated with local nonlinear effects is two orders of magnitude lower than the pressure associated with global nonlinear effects. Local nonlinear effects are therefore expected to be negligible in the context of single-shot ultrasound imaging, but they may influence approaches that subtract pressure fields such as amplitude modulation or pulse inversion

    Predictions for Higgs and SUSY spectra from SO(10) Yukawa Unification with mu > 0

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    We use t,b,τt, b, \tau Yukawa unification to constrain SUSY parameter space. We find a narrow region survives for μ>0\mu > 0 (suggested by \bsgam and the anomalous magnetic moment of the muon) with A01.9m16A_0 \sim - 1.9 m_{16}, m101.4m16m_{10} \sim 1.4 m_{16}, m1612003000m_{16} \sim 1200 -3000 \gev and μ,M1/2100500\mu, M_{1/2} \sim 100 - 500 \gev. Demanding Yukawa unification thus makes definite predictions for Higgs and sparticle masses.Comment: 10 pages, 3 figures, revised version to be published in PR

    5d quivers and their AdS(6) duals

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    We consider an infinite class of 5d supersymmetric gauge theories involving products of symplectic and unitary groups that arise from D4-branes at orbifold singularities in Type I' string theory. The theories are argued to be dual to warped AdS(6)x S4/Zn backgrounds in massive Type IIA supergravity. In particular, this demonstrates the existence of supersymmetric 5d fixed points of quiver type. We analyze the spectrum of gauge fields and charged states in the supergravity dual, and find a precise agreement with the symmetries and charged operators in the quiver theories. We also comment on other brane objects in the supergravity dual and their interpretation in the field theories.Comment: 29 pages, 15 figure

    Non-Universal Soft SUSY Breaking and Dark Matter

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    An analysis is given of the effects of non-universal soft SUSY breaking masses in the Higgs sector and in the third generation squark sector, and it is shown that they are highly coupled. Analytic expressions are obtained for their effects on the parameters μ,mA\mu,m_A and on the third generation squark masses. Non-universality effects on dark matter event rates in neutralino-nucleus scattering are analysed. It is found that the effects are maximal in the range mχ~165m_{\tilde\chi_1}\leq 65~GeV where the relic density is governed by the Z and Higgs poles. In this range the minimum event rates can be increased or decreased by factors of O(10) depending on the sign of non-universality. Above this range Landau pole effects arising from the heavy top mass tend to suppress the non-universality effects. The effect of more precise measurements of cosmological parameters on event rates, which is expected to occur in the next round of COBE like sattelite experiments, is also investigated. Implications for the analysis for dark matter searches are discussed.Comment: 28 pages, latex, and 7 fig

    Sparticle Mass Spectra from SO(10) Grand Unified Models with Yukawa Coupling Unification

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    We examine the spectrum of superparticles obtained from the minimal SO(10) grand unified model, where it is assumed the gauge symmetry breaking yields the Minimal Supersymmetric Standard Model (MSSM) as the effective theory at MGUT2×1016M_{GUT}\sim 2\times 10^{16} GeV. In this model, unification of Yukawa couplings implies a value of tanβ4555\tan\beta\sim 45-55. At such high values of tanβ\tan\beta, assuming universality of scalar masses, the usual mechanism of radiative electroweak symmetry breaking breaks down. We show that a set of weak scale sparticle masses consistent with radiative electroweak symmetry breaking can be generated by imposing non-universal GUT scale scalar masses consistent with universality within SO(10) plus extra DD-term contributions associated with the reduction in rank of the gauge symmetry group when SO(10) spontaneously breaks to SU(3)×SU(2)×U(1)SU(3)\times SU(2)\times U(1). We comment upon the consequences of the sparticle mass spectrum for collider searches for supersymmetry. One implication of SO(10) unification is that the light bottom squark can be by far the lightest of the squarks. This motivates a dedicated search for bottom squark pair production at ppˉp\bar{p} and e+ee^+e^- colliders.Comment: 12 page REVTEX file including 3 PS figures; revised manuscript includes minor changes to coincide with published versio

    Probing EWSB Naturalness in Unified SUSY Models with Dark Matter

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    We have studied Electroweak Symmetry Breaking (EWSB) fine-tuning in the context of two unified Supersymmetry scenarios: the Constrained Minimal Supersymmetric Model (CMSSM) and models with Non-Universal Higgs Masses (NUHM), in light of current and upcoming direct detection dark matter experiments. We consider both those models that satisfy a one-sided bound on the relic density of neutralinos, Ωχh2<0.12\Omega_{\chi} h^2 < 0.12, and also the subset that satisfy the two-sided bound in which the relic density is within the 2 sigma best fit of WMAP7 + BAO + H0 data. We find that current direct detection searches for dark matter probe the least fine-tuned regions of parameter-space, or equivalently those of lowest Higgs mass parameter μ\mu, and will tend to probe progressively more and more fine-tuned models, though the trend is more pronounced in the CMSSM than in the NUHM. Additionally, we examine several subsets of model points, categorized by common mass hierarchies; M_{\chi_0} \sim M_{\chi^\pm}, M_{\chi_0} \sim M_{\stau}, M_{\chi_0} \sim M_{\stop_1}, the light and heavy Higgs poles, and any additional models classified as "other"; the relevance of these mass hierarchies is their connection to the preferred neutralino annihilation channel that determines the relic abundance. For each of these subsets of models we investigated the degree of fine-tuning and discoverability in current and next generation direct detection experiments.Comment: 26 pages, 10 figures. v2: references added. v3: matches published versio

    The Search for Supersymmetry at the Tevatron Collider

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    We review the status of searches for Supersymmetry at the Tevatron Collider. After discussing the theoretical aspects relevant to the production and decay of supersymmetric particles at the Tevatron, we present the current results for Runs Ia and Ib as of the summer of 1997. To appear in the book "Perspectives in Supersymmetry", edited by G.L. Kane, World Scientific.Comment: 84 pages with 31 figures imbedded using psfig.tex. Uses sprocl.st
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