8,373 research outputs found

    Pauli-Potential and Green Function Monte-Carlo Method for Many-Fermion Systems

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    The time evolution of a many-fermion system can be described by a Green's function corresponding to an effective potential, which takes anti-symmetrization of the wave function into account, called the Pauli-potential. We show that this idea can be combined with the Green's Function Monte Carlo method to accurately simulate a system of many non-relativistic fermions. The method is illustrated by the example of systems of several (2-9) fermions in a square well.Comment: 12 pages, LaTeX, 4 figure

    Upper bound on the cutoff in lattice Electroweak theory

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    We investigate numerically lattice Weinberg - Salam model without fermions for realistic values of the fine structure constant and the Weinberg angle. We also analyze the data of the previous numerical investigations of lattice Electroweak theory. We have found that moving along the line of constant physics when the lattice spacing aa is decreased, one should leave the physical Higgs phase of the theory at a certain value of aa. Our estimate of the minimal value of the lattice spacing is ac=[430±40Gev]−1a_c = [430\pm 40 {\rm Gev}]^{-1}.Comment: Latex, 21 pages, 3 figures, to appear in JHE

    The heavy-quark pole masses in the Hamiltonian approach

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    From the fact that the nonperturbative self-energy contribution CSEC_{\rm SE} to the heavy meson mass is small: CSE(bbˉ)=0C_{\rm SE}(b\bar{b})=0; CSE(ccˉ)≅−40C_{\rm SE}(c\bar{c})\cong -40 MeV \cite{ref.01}, strong restrictions on the pole masses mbm_b and mcm_c are obtained. The analysis of the bbˉb\bar{b} and the ccˉc\bar{c} spectra with the use of relativistic (string) Hamiltonian gives mbm_b(2-loop)=4.78±0.05=4.78\pm 0.05 GeV and mcm_c(2-loop)=1.39±0.06=1.39 \pm 0.06 GeV which correspond to the MSˉ\bar{\rm MS} running mass mˉb(mˉb)=4.19±0.04\bar{m}_b(\bar{m}_b)=4.19\pm 0.04 GeV and mˉc(mˉc)=1.10±0.05\bar{m}_c(\bar{m}_c)=1.10\pm 0.05 GeV. The masses ωc\omega_c and ωb\omega_b, which define the heavy quarkonia spin structure, are shown to be by ∼200\sim 200 MeV larger than the pole ones.Comment: 18 pages, no figures, 8 table

    The Hyperfine Splittings in Bottomonium and the Bq(q=n,s,c)B_q (q=n,s,c) Mesons

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    A universal description of the hyperfine splittings (HFS) in bottomonium and the Bq(q=n,s,c)B_q (q=n,s,c) mesons is obtained with a universal strong coupling constant αs(μ)=0.305(2)\alpha_s(\mu)=0.305(2) in a spin-spin potential. Other characteristics are calculated within the Field Correlator Method, taking the freezing value of the strong coupling independent of nfn_f. The HFS M(B∗)−M(B)=45.3(3)M(B^*)- M(B)=45.3(3) MeV, M(Bs∗)−M(Bs)=46.5(3)M(B_s^*) - M(B_s)=46.5(3) MeV are obtained in full agreement with experiment both for nf=3n_f=3 and nf=4n_f=4. In bottomonium, M(Υ(9460))−M(ηb)=70.0(4)M(\Upsilon(9460))- M(\eta_b)=70.0(4) MeV for nf=5n_f=5 agrees with the BaBar data, while a smaller HFS, equal to 64(1) MeV, is obtained for nf=4n_f=4. We predict HFS M(Υ(2S))−M(ηb(2S))=36(1)M(\Upsilon(2S))-M(\eta_b(2S))=36(1) MeV, M(Υ(3S))−M(η(3S))=27(1)M(\Upsilon(3S))- M(\eta(3S))=27(1) MeV, and M(Bc∗)−M(Bc)=57.5(10)M(B_c^*) - M(B_c)= 57.5(10) MeV, which gives M(Bc∗)=6334(1)M(B_c^*)=6334(1) MeV, M(Bc(21S0))=6865(5)M(B_c(2 {}^1S_0))=6865(5) MeV, and M(Bc∗(2S3S1))=6901(5)M(B_c^*(2S {}^3S_1))=6901(5) MeV.Comment: 5 pages revtex

    Effect of disorder on the conductance of a Cu atomic point contact

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    We present a systematic study of the effect of the disorder in copper point contacts. We show that peaks in the conductance histogram of copper point contacts shift upon addition of nickel impurities. The shift increases initially linerarly with the nickel concentration, thus confirming that it is due to disorder in the nanowire, in accordance with predictions. In general, this shift is modelled as a resistance R_s which is placed in series with the contact resistance R_c. However, we obtain different R_s values for the two peaks in the histogram, R_s being larger for the peak at higher conductance.Comment: 6 pages, 4 figure

    Nambu monopoles in lattice Electroweak theory

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    We considered the lattice electroweak theory at realistic values of α\alpha and θW\theta_W and for large values of the Higgs mass. We investigated numerically the properties of topological objects that are identified with quantum Nambu monopoles. We have found that the action density near the Nambu monopole worldlines exceeds the density averaged over the lattice in the physical region of the phase diagram. Moreover, their percolation probability is found to be an order parameter for the transition between the symmetric and the broken phases. Therefore, these monopoles indeed appear as real physical objects. However, we have found that their density on the lattice increases with increasing ultraviolet cutoff. Thus we conclude, that the conventional lattice electroweak theory is not able to predict the density of Nambu monopoles. This means that the description of Nambu monopole physics based on the lattice Weinberg - Salam model with finite ultraviolet cutoff is incomplete. We expect that the correct description may be obtained only within the lattice theory that involves the description of TeV - scale physics.Comment: LATE

    Magnetic properties of Co doped Nb clusters

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    From magnetic deflection experiments on isolated Co doped Nb clusters we made the interesting observation of some clusters being magnetic, while others appear to be non-magnetic. There are in principle two explanations for this behavior. Either the local moment at the Co site is completely quenched or it is screened by the delocalized electrons of the cluster, i.e. the Kondo effect. In order to reveal the physical origin, we conducted a combined theoretical and experimental investigation. First, we established the ground state geometry of the clusters by comparing the experimental vibrational spectra with those obtained from a density functional theory study. Then, we performed an analyses based on the Anderson impurity model. It appears that the non-magnetic clusters are due to a complete quenching of the local Co moment and not due to the Kondo effect. In addition, the magnetic behavior of the clusters can be understood from an inspection of their electronic structure. Here magnetism is favored when the effective hybridization around the chemical potential is small, while the absence of magnetism is signalled by a large effective hybridization around the chemical potential.Comment: 14 pages, 8 figure
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