899 research outputs found

    Chargino Production at an e-e- Collider

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    The chargino pair production in eee^-e^- collisions with their subsequent decays are considered within SUSY models with R-parity violation and with lepton number non-conservation. The production process (s=1\sqrt{s}=1 TeV) is predicted to be large in a wide range of both sneutrino and chargino masses. The influence of all virtual sneutrino states and their mixings with electrons are taken into account. Some specific situations are pointed out when significant suppressions of the cross section can take place. The chargino decays are discussed for either the chargino as LSP or the chargino as heavier sparticle. In both cases unique signals are possible with up to six charged fermions and without missing energy.Comment: 9 page

    Dijet resonances, widths and all that

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    The search for heavy resonances in the dijet channel is part of the on-going physics programme, both at the Tevatron and at the LHC. Lower limits have been placed on the masses of dijet resonances predicted in a wide variety of models. However, across experiments, the search strategy assumes that the effect of the new particles is well-approximated by on-shell production and subsequent decay into a pair of jets. We examine the impact of off-shell effects on such searches, particularly for strongly interacting resonances.Comment: Version published in JHE

    Selectron Studies at e-e- and e+e- Colliders

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    Selectrons may be studied in both e-e- and e+e- collisions at future linear colliders. Relative to e+e-, the e-e- mode benefits from negligible backgrounds and \beta threshold behavior for identical selectron pair production, but suffers from luminosity degradation and increased initial state radiation and beamstrahlung. We include all of these effects and compare the potential for selectron mass measurements in the two modes. The virtues of the e-e- collider far outweigh its disadvantages. In particular, the selectron mass may be measured to 100 MeV with a total integrated luminosity of 1 fb^-1, while more than 100 fb^-1 is required in e+e- collisions for similar precision.Comment: 16 pages, 11 figure

    Fourier Analysis of Gapped Time Series: Improved Estimates of Solar and Stellar Oscillation Parameters

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    Quantitative helio- and asteroseismology require very precise measurements of the frequencies, amplitudes, and lifetimes of the global modes of stellar oscillation. It is common knowledge that the precision of these measurements depends on the total length (T), quality, and completeness of the observations. Except in a few simple cases, the effect of gaps in the data on measurement precision is poorly understood, in particular in Fourier space where the convolution of the observable with the observation window introduces correlations between different frequencies. Here we describe and implement a rather general method to retrieve maximum likelihood estimates of the oscillation parameters, taking into account the proper statistics of the observations. Our fitting method applies in complex Fourier space and exploits the phase information. We consider both solar-like stochastic oscillations and long-lived harmonic oscillations, plus random noise. Using numerical simulations, we demonstrate the existence of cases for which our improved fitting method is less biased and has a greater precision than when the frequency correlations are ignored. This is especially true of low signal-to-noise solar-like oscillations. For example, we discuss a case where the precision on the mode frequency estimate is increased by a factor of five, for a duty cycle of 15%. In the case of long-lived sinusoidal oscillations, a proper treatment of the frequency correlations does not provide any significant improvement; nevertheless we confirm that the mode frequency can be measured from gapped data at a much better precision than the 1/T Rayleigh resolution.Comment: Accepted for publication in Solar Physics Topical Issue "Helioseismology, Asteroseismology, and MHD Connections

    Axigluon Couplings in the Presence of Extra Color-Octet Spin-One Fields

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    In this paper, we study how the interaction of the axigluon with quarks is modified when we introduce new color-octet spin-one fields in a chiral color model. We show that in this case the strength of this interaction is not completely determined by the gauge symmetry any more and can be significantly weaker than the one predicted in the original chiral color model. In this way, we reinterpret the non-observability of the axigluon at the Tevatron, not as a limit on the axigluon mass, but as a limit on the strength of the axigluon coupling to quarks

    MScMS-II: an innovative IR-based indoor coordinate measuring system for large-scale metrology applications

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    According to the current great interest concerning large-scale metrology applications in many different fields of manufacturing industry, technologies and techniques for dimensional measurement have recently shown a substantial improvement. Ease-of-use, logistic and economic issues, as well as metrological performance are assuming a more and more important role among system requirements. This paper describes the architecture and the working principles of a novel infrared (IR) optical-based system, designed to perform low-cost and easy indoor coordinate measurements of large-size objects. The system consists of a distributed network-based layout, whose modularity allows fitting differently sized and shaped working volumes by adequately increasing the number of sensing units. Differently from existing spatially distributed metrological instruments, the remote sensor devices are intended to provide embedded data elaboration capabilities, in order to share the overall computational load. The overall system functionalities, including distributed layout configuration, network self-calibration, 3D point localization, and measurement data elaboration, are discussed. A preliminary metrological characterization of system performance, based on experimental testing, is also presente

    Lepton flavor violating signals of a little Higgs model at the high energy linear e+ee^{+}e^{-} colliders

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    Littlest Higgs (LH)(LH) model predicts the existence of the doubly charged scalars Φ±±\Phi^{\pm\pm}, which generally have large flavor changing couplings to leptons. We calculate the contributions of Φ±±\Phi^{\pm\pm} to the lepton flavor violating (LFV)(LFV) processes liljγl_{i}\to l_{j}\gamma and liljlklkl_{i}\to l_{j}l_{k}l_{k}, and compare our numerical results with the current experimental upper limits on these processes. We find that some of these processes can give severe constraints on the coupling constant YijY_{ij} and the mass parameter MΦM_{\Phi}. Taking into account the constraints on these free parameters, we further discuss the possible lepton flavor violating signals of Φ±±\Phi^{\pm\pm} at the high energy linear e+ee^{+}e^{-} collider (ILC)(ILC) experiments. Our numerical results show that the possible signals of Φ±±\Phi^{\pm\pm} might be detected via the subprocesses e±e±l±l±e^{\pm}e^{\pm}\to l^{\pm}l^{\pm} in the future ILCILC experiments.Comment: 16 pages, 7 figures. Discussions and references added, typos correcte

    Realistic constraints on the doubly charged bilepton couplings from Bhabha scattering with LEP data

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    Upper limits on doubly charged bilepton couplings and masses are extracted from LEP data for Bhabha scattering at energy range s=183202\sqrt{s}=183-202 GeV using standard model program ZFITTER which calculates radiative corrections. We find that gL2/ML2<O(105)GeV2g_{L}^{2}/M_{L}^{2}<O(10^{-5})GeV^{-2} at 95% C.L. for scalar and vector bileptons.Comment: 5 pages, 1 EPS figur
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