53,600 research outputs found

    Origins of the Isospin Violation of Dark Matter Interactions

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    Light dark matter (DM) with a large DM-nucleon spin-independent cross section and furthermore proper isospin violation (ISV) fn/fp≈−0.7f_n/f_p\approx-0.7 may provide a way to understand the confusing DM direct detection results. Combing with the stringent astrophysical and collider constraints, we systematically investigate the origin of ISV first via general operator analyses and further via specifying three kinds of (single) mediators: A light Z′Z' from chiral U(1)XU(1)_X, an approximate spectator Higgs doublet (It can explain the W+jjW+jj anomaly simultaneously) and color triplets. In addition, although Z′Z' from an exotic U(1)XU(1)_X mixing with U(1)YU(1)_Y generating fn=0f_n=0, we can combine it with the conventional Higgs to achieve proper ISV. As a concrete example, we propose the U(1)XU(1)_X model where the U(1)XU(1)_X charged light sneutrino is the inelastic DM, which dominantly annihilates to light dark states such as Z′Z' with sub-GeV mass. This model can address the recent GoGeNT annual modulation consistent with other DM direct detection results and free of exclusions.Comment: References added and English greatly improve

    Is the Number of Giant Arcs in LCDM Consistent With Observations?

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    We use high-resolution N-body simulations to study the galaxy-cluster cross-sections and the abundance of giant arcs in the Λ\LambdaCDM model. Clusters are selected from the simulations using the friends-of-friends method, and their cross-sections for forming giant arcs are analyzed. The background sources are assumed to follow a uniform ellipticity distribution from 0 to 0.5 and to have an area identical to a circular source with diameter 1\arcsec. We find that the optical depth scales as the source redshift approximately as \tau_{1''} = 2.25 \times 10^{-6}/[1+(\zs/3.14)^{-3.42}] (0.6<\zs<7). The amplitude is about 50% higher for an effective source diameter of 0.5\arcsec. The optimal lens redshift for giant arcs with the length-to-width ratio (L/WL/W) larger than 10 increases from 0.3 for \zs=1, to 0.5 for \zs=2, and to 0.7-0.8 for \zs>3. The optical depth is sensitive to the source redshift, in qualitative agreement with Wambsganss et al. (2004). However, our overall optical depth appears to be only ∼\sim 10% to 70% of those from previous studies. The differences can be mostly explained by different power spectrum normalizations (σ8\sigma_8) used and different ways of determining the L/WL/W ratio. Finite source size and ellipticity have modest effects on the optical depth. We also found that the number of highly magnified (with magnification ∣μ∣>10|\mu|>10) and ``undistorted'' images (with L/W<3L/W<3) is comparable to the number of giant arcs with ∣μ∣>10|\mu|>10 and L/W>10L/W>10. We conclude that our predicted rate of giant arcs may be lower than the observed rate, although the precise `discrepancy' is still unclear due to uncertainties both in theory and observations.Comment: Revised version after the referee's reports (32 pages,13figures). The paper has been significantly revised with many additions. The new version includes more detailed comparisons with previous studies, including the effects of source size and ellipticity. New discussions about the redshift distribution of lensing clusters and the width of giant arcs have been adde

    Defect Motion and Lattice Pinning Barrier in Josephson-Junction Ladders

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    We study motion of domain wall defects in a fully frustrated Josephson-unction ladder system, driven by small applied currents. For small system sizes, the energy barrier E_B to the defect motion is computed analytically via symmetry and topological considerations. More generally, we perform numerical simulations directly on the equations of motion, based on the resistively-shunted junction model, to study the dynamics of defects, varying the system size. Coherent motion of domain walls is observed for large system sizes. In the thermodynamical limit, we find E_B=0.1827 in units of the Josephson coupling energy.Comment: 7 pages, and to apear in Phys. Rev.

    Gauge/String-Gravity Duality and Froissart Bound

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    The gauge/string-gravity duality correspondence opened renewed hope and possibility to address some of the fundamental and non-perturbative QCD problems in particle physics, such as hadron spectrum and Regge behavior of the scattering amplitude at high energies. One of the most fundamental and long-standing problem is the high energy behavior of total cross-sections. According to a series of exhaustive tests by the COMPETE group, (1). total cross-sections have a universal Heisenberg behavior in energy corresponding to the maximal energy behavior allowed by the Froissart bound, i.e., A+Bln2(s/s0)A + B ln^2 (s/s_0) with B∼0.32mbB \sim 0.32 mb and s0∼34.41GeV2s_0 \sim 34.41 GeV^2 for all reactions, and (2). the factorization relation among σpp,even,σγp,andσγγ\sigma_{pp, even}, \sigma_{\gamma p}, and \sigma_{\gamma \gamma} is well satisfied by experiments. I discuss the recent interesting application of the gauge/string-gravity duality of AdS/CFTAdS/CFT correspondence with a deformed background metric so as to break the conformal symmetry that can lead to the Heisenberg behavior of rising total cross-sections, and present some preliminary results on the high energy QCD from Planckian scattering in AdSAdS and black-hole production.Comment: 10 pages, Presented to the Coral Gables Conference 2003, Launching of BelleE\'poque in High Energy Physics and Cosmology, 17 - 21 December 2003, Fort Lauderdale, Florid

    Weakly coupled s=1/2s = 1/2 quantum spin singlets in Ba3_{3}Cr2_{2}O8_{8}

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    Using single crystal inelastic neutron scattering with and without application of an external magnetic field and powder neutron diffraction, we have characterized magnetic interactions in Ba3_3Cr2_2O8_8. Even without field, we found that there exist three singlet-to-triplet excitation modes in (h,h,l)(h,h,l) scattering plane. Our complete analysis shows that the three modes are due to spatially anisotropic interdimer interactions that are induced by local distortions of the tetrahedron of oxygens surrounding the Jahn-Teller active Cr5+(3d1)^{5+} (3d^1). The strong intradimer coupling of J0=2.38(2)J_0 = 2.38(2) meV and weak interdimer interactions (∣Jinter∣≤0.52(2)|J_{\rm inter}| \leq 0.52(2) meV) makes Ba3_3Cr2_2O8_8 a good model system for weakly-coupled s=1/2s = 1/2 quantum spin dimers

    Higgs Boson Bounds in Three and Four Generation Scenarios

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    In light of recent experimental results, we present updated bounds on the lightest Higgs boson mass in the Standard Model (SM) and in the Minimal Supersymmetric extension of the Standard Model (MSSM). The vacuum stability lower bound on the pure SM Higgs boson mass when the SM is taken to be valid up to the Planck scale lies above the MSSM lightest Higgs boson mass upper bound for a large amount of SUSY parameter space. If the lightest Higgs boson is detected with a mass M_{H} < 134 GeV (150 GeV) for a top quark mass M_{top} = 172 GeV (179 GeV), it may indicate the existence of a fourth generation of fermions. The region of inconsistency is removed and the MSSM is salvagable for such values of M_{H} if one postulates the existence of a fourth generation of leptons and quarks with isodoublet degenerate masses M_{L} and M_{Q} such that 60 GeV 170 GeV.Comment: 7 pages, 4 figures. To be published in Physical Review

    Spin Fluctuation Induced Dephasing in a Mesoscopic Ring

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    We investigate the persistent current in a hybrid Aharonov-Bohm ring - quantum dot system coupled to a reservoir which provides spin fluctuations. It is shown that the spin exchange interaction between the quantum dot and the reservoir induces dephasing in the absence of direct charge transfer. We demonstrate an anomalous nature of this spin-fluctuation induced dephasing which tends to enhance the persistent current. We explain our result in terms of the separation of the spin from the charge degree of freedom. The nature of the spin fluctuation induced dephasing is analyzed in detail.Comment: 4 pages, 4 figure

    Synthesis of as-grown superconducting MgB_2 thin films by molecular beam epitaxy in UHV conditions

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    As-grown superconducting MgB_2 thin films have been grown on SrTiO_3(001), MgO(001), and Al_2O_3(0001) substrates by a molecular beam epitaxy (MBE) method with novel co-evaporation conditions of low deposition rate in ultra-high vacuum. The structural and physical properties of the films were studied by RHEED, XRD, electrical resistivity measurements, and SQUID magnetometer. The RHEED patterns indicate three-dimensional growth for MgB_2. The highest T_c determined by resistivity measurement was about 36K in these samples. And a clear Meissner effect below T_c was observed using magnetic susceptibility measurement. We will discuss the influence of B buffer layer on the structural and physical properties.Comment: 9 pages with 4 figures, ISS2003 proceedin
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