1,065 research outputs found

    Perspectives for the detection and measurement of Supersymmetry in the focus point region of mSUGRA models with the ATLAS detector at LHC

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    This paper discusses the ATLAS potential to study Supersymmetry for the "Focus-Point" region of the parameter space of mSUGRA models. The potential to discovery a deviation from Standard Model expectations with the first few fb1{fb}^{-1} of LHC data was studied using the parametrized simulation of the ATLAS detector. Several signatures were considered, involving hard jets, large missing energy, and either bb-tagged jets, opposite-sign isolated electron or muon pairs, or top quarks reconstructed exploiting their fully hadronic decays. With only 1 fb1{fb}^{-1} of data each of these signatures may allow to observe an excess of events over Standard Model expectation with a statistical significance exceeding 5 standard deviations. An analytical expression was derived for the shape of the distribution of the dilepton invariant mass arising from the three-body leptonic decay of the neutralinos under the hypothesis of heavy scalars, which is appropriate for the focus-point scenario. The resulting function was used to fit the distribution of the dilepton invariant mass obtained with simulated LHC data, and to extract the value of two kinematic endpoints measuring the χ~20χ~10\tilde \chi^0_2 - \tilde \chi^0_1 and the χ~30χ~10\tilde \chi^0_3 - \tilde \chi^0_1 mass differences. This information was used to constrain the MSSM parameter space compatible with the data

    Doping and temperature dependence of incommensurate antiferromagnetism in underdoped lanthanum cuprates

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    The doping, temperature and energy dependence of the dynamical spin structure factors of the underdoped lanthanum cuprates in the normal state is studied within the t-J model using the fermion-spin transformation technique. Incommensurate peaks are found at [(1±δ)π,π][(1\pm\delta)\pi,\pi], [π,(1±δ)π][\pi,(1\pm\delta)\pi] at relatively low temperatures with δ\delta linearly increasing with doping at the beginning and then saturating at higher dopings. These peaks broaden and weaken in amplitude with temperature and energy, in good agreement with experiments. The theory also predicts a rotation of these peaks by π/4\pi/4 at even higher temperatures, being shifted to [(1±δ/2)π,(1±δ/2)π][(1\pm \delta/\sqrt{2})\pi,(1\pm \delta/\sqrt{2})\pi].Comment: 11 pages, PDF file, six figures are included, accepted for publication in Physical Review

    CMB Power Spectrum from Noncommutative Spacetime

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    Very recent CMB data of WMAP offers an opportunity to test inflation models, in particular, the running of spectral index is quite new and can be used to rule out some models. We show that an noncommutative spacetime inflation model gives a good explanation of these new results. In fitting the data, we also obtain a relationship between the noncommutative parameter (string scale) and the ending time of inflation.Comment: 8 pages, 2 figures; v2: refs. added and minor corrections; v3: further minor correctio

    WMAP constraint on the P-term inflationary model

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    In light of WMAP results, we examine the observational constraint on the P-term inflation. With the tunable parameter ff, P-term inflation contains richer physics than D-term and F-term inflationary models. We find the logarithmic derivative spectral index with n>1n>1 on large scales and n<1n<1 on small scales in agreement to observation. We obtained a reasonable range for the choice of the gauge coupling constant gg in order to meet the requirements of WMAP observation and the expected number of the e-foldings. Although tuning ff and gg we can have larger values for the logarithmic derivative of the spectral index, it is not possible to satisfy all observational requirements for both, the spectral index and its logarithmic derivative at the same time.Comment: 6 pages, double column, 13 figures included. Version appearing in the Physical Review

    Properties and Applications of the Electrohydraulic Servosystem of the Hydraulic Excavator

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    The service of a hydraulic excavator is complicated by poor environment. The safety and stability of the control system are influenced by external factors. The object of the study is the electrohydraulic servosystem of the hydraulic excavator. The mathematical and simulation models using AMESIM for the servosystem are constructed. Then the pressure and flow characteristics are analyzed. The design and optimization of the electrohydraulic servosystem and its application in excavator engineering are described. The operation process is graphically presented by a curve, which steeply slopes up (rising period) and then flattens out (stabilization period), those periods are shortened by 38.0 and 40.5%, respectively, the delay tracking period decreased by 52.6%, and anti-interference is reliable.Эксплуатация гидравлического экскаватора осложняется наличием неблагоприятной рабочей среды. Показано воздействие внешних факторов на надежность и стабильность системы контроля. Исследована электрогидравлическая сервосистема гидравлического экскаватора. Построены математическая и имитационная модели для сервосистемы с использованием программы AMESIM. Выполнен анализ характеристик давления и текучести. Описаны конструкция и оптимизация электрогидравлической сервосистемы, а также ее применение в экскаваторной технике. Процесс функционирования электрогидравлической сервосистемы представлен кривой, которая круто идет вверх (период подъема), а затем выходит на плато (период стабилизации), эти периоды сокращаются на 38,0 и 40,5% соответственно, период слежения за задержкой на 52,6% при эффективной помехоустойчивости

    Geochronological and geochemical constraints on Late Cryogenian to Early Ediacaran magmatic rocks on the northern Tarim Craton:implications for tectonic setting and affinity with Gondwana

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    The Tarim Craton provides a geologic record of both the fragmentation of the Rodinian supercontinent and the subsequent assembly of Gondwana. However, the timing and interactions of these radically different tectonic processes remain contested. A critical part of this debate revolves around the Late Cryogenian-Ediacaran igneous rocks along the Craton’s northern margin, specifically, whether they record super-plume related Rodinian breakup or Gondwanan orogeny. To address this issue, we present zircon U-Pb-Hf isotopic data and whole rock geochemistry from Late Cryogenian to Early Ediacaran granitoids of the northern Tarim Craton. U-Pb zircon ages reveal three magmatic periods along the northern Tarim margin: ca. 660–640 Ma, 635–625 Ma and 620–600 Ma, associated with small scale felsic and mafic magmas. These granitoids have an A2-type affinity and are enriched in alkalines, but are depleted in Nb, Ta, Sr, P and Ti. Elemental data and generally negative εHf(t) values (−13.96 to 1.65) suggest that they were mainly derived from partial melting of enriched, subduction-modified lithospheric mantle triggered by upwelling of the asthenospheric mantle along the active continental margin of northern Tarim. We suggest that the Tarim Craton travelled as an isolated plate for much of the Late Neoproterozoic, near the outer part of Rodinia and subsequently Gondwana. During this time it was affected by localized and periodic subduction-related intrusion and eruption. However, within the samples of this study, there is no U-Pb-Hf isotopic and whole-rock geochemical evidence to support either super-plume-related rifting (i.e. Rodinian breakup) or Pan-African orogeny (i.e. Gondwanan assembly).</p

    Application of a H 2 + -like model to helium atom. Solution of the wave equation at the ground state

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    The wave equation of helium atom is solved based on a “H 2 + -like” model. A good agreement between the theoretical and experimental ionization energies is obtained.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/43907/1/10053_2005_Article_BF01398893.pd

    The fermion dynamical symmetry model for the even--even and even--odd nuclei in the Xe--Ba region

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    The even--even and even--odd nuclei 126^{126}Xe-132^{132}Xe and 131^{131}Ba-137^{137}Ba are shown to have a well-realized SO8SO6SO3SO_8 \supset SO_6 \supset SO_3 fermion dynamical symmetry. Their low-lying energy levels can be described by a unified analytical expression with two (three) adjustable parameters for even--odd (even--even) nuclei that is derived from the fermion dynamical symmetry model. Analytical expressions are given for wavefunctions and for E2E2 transition rates that agree well with data. The distinction between the FDSM and IBM SO6SO_6 limits is discussed. The experimentally observed suppression of the the energy levels with increasing SO5SO_5 quantum number τ\tau can be explained as a perturbation of the pairing interaction on the SO6SO_6 symmetry, which leads to an SO5SO_5 Pairing effect for SO6SO_6 nuclei.Comment: submitted to Phys. Rev. C, LaTeX, 31 pages, 8 figures with postscript files available on request at [email protected]

    Suppressing CMB Quadrupole with a Bounce from Contracting Phase to Inflation

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    Recent released WMAP data show a low value of quadrupole in the CMB temperature fluctuations, which confirms the early observations by COBE. In this paper, a scenario, in which a contracting phase is followed by an inflationary phase, is constructed. We calculate the perturbation spectrum and show that this scenario can provide a reasonable explanation for lower CMB anisotropies on large angular scales.Comment: 5 pages, 3 figure

    Power-law entropy-corrected HDE and NADE in Brans-Dicke cosmology

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    Considering the power-law corrections to the black hole entropy, which appear in dealing with the entanglement of quantum fields inside and outside the horizon, the holographic energy density is modified accordingly. In this paper we study the power-law entropy-corrected holographic dark energy in the framework of Brans-Dicke theory. We investigate the cosmological implications of this model in detail. We also perform the study for the new agegraphic dark energy model and calculate some relevant cosmological parameters and their evolution. {As a result we find that this model can provide the present cosmic acceleration and even the equation of state parameter of this model can cross the phantom line wD=1w_D=-1 provided the model parameters are chosen suitably}.Comment: 14 pages, 2 figure, accepted by IJT
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