33,180 research outputs found

    Is U3Ni3Sn4 best described as near a quantum critical point?

    Full text link
    Although most known non-Fermi liquid (NFL) materials are structurally or chemically disordered, the role of this disorder remains unclear. In particular, very few systems have been discovered that may be stoichiometric and well ordered. To test whether U3Ni3Sn4 belongs in this latter class, we present measurements of the x-ray absorption fine structure (XAFS) of polycrystalline and single-crystal U3Ni3Sn4 samples that are consistent with no measurable local structural disorder. We also present temperature-dependent specific heat data in applied magnetic fields as high as 8 T that show features that are inconsistent with the antiferromagnetic Griffiths' phase model, but do support the conclusion that a Fermi liquid/NFL crossover temperature increases with applied field. These results are inconsistent with theoretical explanations that require strong disorder effects, but do support the view that U3Ni3Sn4 is a stoichiometric, ordered material that exhibits NFL behavior, and is best described as being near an antiferromagnetic quantum critical point.Comment: 9 pages, 8 figures, in press with PR

    Self-interacting dark matter and Higgs bosons in the SU(3)_C x SU(3)_L x U(1)_N model with right-handed neutrinos

    Full text link
    We investigate the possibility that dark matter could be made from CP-even and CP- odd Higgs bosons in the SU(3)_C X SU(3)_L X U(1)_N (3-3-1) model with right-handed neutrinos. This self-interacting dark matters are stable without imposing of new symmetry and should be weak-interacting.Comment: 7 pages, Latex, To appear in Europhys. Let

    A General SU(2) Formulation for Quantum Searching with Certainty

    Get PDF
    A general quantum search algorithm with arbitrary unitary transformations and an arbitrary initial state is considered in this work. To serach a marked state with certainty, we have derived, using an SU(2) representation: (1) the matching condition relating the phase rotations in the algorithm, (2) a concise formula for evaluating the required number of iterations for the search, and (3) the final state after the search, with a phase angle in its amplitude of unity modulus. Moreover, the optimal choices and modifications of the phase angles in the Grover kernel is also studied.Comment: 8 pages, 2 figure

    X-ray Emission of Baryonic Gas in the Universe: Luminosity-Temperature Relationship and Soft-Band Background

    Full text link
    We study the X-ray emission of baryon fluid in the universe using the WIGEON cosmological hydrodynamic simulations. It has been revealed that cosmic baryon fluid in the nonlinear regime behaves like Burgers turbulence, i.e. the fluid field consists of shocks. Like turbulence in incompressible fluid, the Burgers turbulence plays an important role in converting the kinetic energy of the fluid to thermal energy and heats the gas. We show that the simulation sample of the Λ\LambdaCDM model without adding extra heating sources can fit well the observed distributions of X-ray luminosity versus temperature (LxL_{\rm x} vs. TT) of galaxy groups and is also consistent with the distributions of X-ray luminosity versus velocity dispersion (LxL_{\rm x} vs. σ\sigma). Because the baryonic gas is multiphase, the Lx−TL_{\rm x}-T and Lx−σL_{\rm x}-\sigma distributions are significantly scattered. If we describe the relationships by power laws Lx∝TαLTL_{\rm x}\propto T^{\alpha_{LT}} and Lx∝σαLVL_{\rm x}\propto \sigma^{\alpha_{LV}}, we find αLT>2.5\alpha_{LT}>2.5 and αLV>2.1\alpha_{LV}>2.1. The X-ray background in the soft 0.5−20.5-2 keV band emitted by the baryonic gas in the temperature range 105<T<10710^5<T<10^7 K has also been calculated. We show that of the total background, (1) no more than 2% comes from the region with temperature less than 106.510^{6.5} K, and (2) no more than 7% is from the region of dark matter with mass density ρdm<50ρˉdm\rho_{\rm dm}<50 \bar{\rho}_{\rm dm}. The region of ρdm>50ρˉdm\rho_{\rm dm}>50\bar{\rho}_{\rm dm} is generally clustered and discretely distributed. Therefore, almost all of the soft X-ray background comes from clustered sources, and the contribution from truly diffuse gas is probably negligible. This point agrees with current X-ray observations.Comment: 32 pages including 14 figures and 2 tables. Final version for publication in Ap

    Constraining New Forces in the Casimir Regime Using the Isoelectronic Technique

    Get PDF
    We report the first isoelectronic differential force measurements between a Au-coated probe and two Au-coated films, made out of Au and Ge. These measurements, performed at submicron separations using soft microelectromechanical torsional oscillators, eliminate the need for a detailed understanding of the probe-film Casimir interaction. The observed differential signal is directly converted into limits on the parameters α\alpha and λ\lambda which characterize Yukawa-like deviations from Newtonian gravity. We find \alpha \lsim 10^{12} for λ∌200\lambda \sim 200 nm, an improvement of ∌\sim 10 over previous limits.Comment: 10 pages, 4 figure

    Tensor coupling effects on spin symmetry in anti-Lambda spectrum of hypernuclei

    Full text link
    The effects of ΛˉΛˉω\bar\Lambda\bar\Lambda\omega-tensor coupling on the spin symmetry of Λˉ\bar{\Lambda} spectra in Λˉ\bar{\Lambda}-nucleus systems have been studied with the relativistic mean-field theory. Taking 12^{12}C+Λˉ\bar{\Lambda} as an example, it is found that the tensor coupling enlarges the spin-orbit splittings of Λˉ\bar\Lambda by an order of magnitude although its effects on the wave functions of Λˉ\bar{\Lambda} are negligible. Similar conclusions has been observed in Λˉ\bar{\Lambda}-nucleus of different mass regions, including 16^{16}O+Λˉ\bar{\Lambda}, 40^{40}Ca+Λˉ\bar{\Lambda} and 208^{208}Pb+Λˉ\bar{\Lambda}. It indicates that the spin symmetry in anti-lambda-nucleus systems is still good irrespective of the tensor coupling.Comment: 12 pages, 3 figures

    Effects of dynamical phases in Shor's factoring algorithm with operational delays

    Full text link
    Ideal quantum algorithms usually assume that quantum computing is performed continuously by a sequence of unitary transformations. However, there always exist idle finite time intervals between consecutive operations in a realistic quantum computing process. During these delays, coherent "errors" will accumulate from the dynamical phases of the superposed wave functions. Here we explore the sensitivity of Shor's quantum factoring algorithm to such errors. Our results clearly show a severe sensitivity of Shor's factorization algorithm to the presence of delay times between successive unitary transformations. Specifically, in the presence of these {\it coherent "errors"}, the probability of obtaining the correct answer decreases exponentially with the number of qubits of the work register. A particularly simple phase-matching approach is proposed in this paper to {\it avoid} or suppress these {\it coherent errors} when using Shor's algorithm to factorize integers. The robustness of this phase-matching condition is evaluated analytically or numerically for the factorization of several integers: 4,15,214, 15, 21, and 33.Comment: 8 pages with 5 figure

    Using Muonic Hydrogen in Optical Spectroscopy Experiment to Detect Extra Dimensions

    Full text link
    Considering that gravitational force might deviate from Newton's inverse-square law (ISL) and become much stronger in small scale, we propose a kind of optical spectroscopy experiment to detect this possible deviation and take electronic, muonic and tauonic hydrogen atoms as examples. This experiment might be used to indirectly detect the deviation of ISL down to nanometer scale and to explore the possibility of three extra dimensions in ADD's model, while current direct gravity tests cannot break through micron scale and go beyond two extra dimensions scenario.Comment: 9 pages, 2 figures. To appear in IJT
    • 

    corecore