8,984 research outputs found

    Effect of Dynamical Coulomb Correlations on the Fermi Surface of Na_0.3CoO_2

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    The t2g quasi-particle spectra of Na_0.3CoO_2 are calculated within the dynamical mean field theory. It is shown that as a result of dynamical Coulomb correlations charge is transfered from the nearly filled e_g' subbands to the a_1g band, thereby reducing orbital polarization among Co t2g states. Dynamical correlations therefore stabilize the small e_g' Fermi surface pockets, in contrast to angle-resolved photoemission data, which do not reveal these pockets.Comment: 4 pages, to appear in PR

    Total Width of 125 GeV Higgs Boson

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    By using the LHC and Tevatron measurements of the cross sections to various decay channels relative to the standard model Higgs boson, the total width of the putative 125 GeV Higgs boson is determined as 6.1 +7.7-2.9 MeV. We describe a way to estimate the branching fraction for Higgs decay to dark matter. We also discuss a No-Go theorem for the gammagamma signal of the Higgs boson at the LHC.Comment: 11 pages, 2 figure

    Searching for Stoponium along with the Higgs boson

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    Stoponium, a bound state of top squark and its antiparticle in a supersymmetric model, may be found in the ongoing Higgs searches at the LHC. Its WW and ZZ detection ratios relative to the Standard Model Higgs boson can be more than unity from WW* threshold to the two Higgs threshold. The gamma gamma channel is equally promising. Some regions of the stoponium mass below 150 GeV are already being probed by the ATLAS and CMS experiments.Comment: 10 pages 5 figure

    Correlation between Superconducting Transition Temperature TcT_c and Increase of Nuclear Spin-Lattice Relaxation Rate Devided by Temperature 1/T1T1/T_1T at TcT_c in the Hydrate Cobaltate Nax_{x}CoO2â‹…y_{2}\cdot yH2_{2}O

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    We have performed Co-nuclear quadrupole resonance (NQR) studies on Nax_{x}CoO2â‹…y_{2}\cdot yH2_{2}O compounds with different Na (xx) and hydrate (yy) contents. Two samples with different Na contents but nearly the same TcT_c values (xx = 0.348, TcT_c = 4.7 K ; xx = 0.339, TcT_c = 4.6 K) were investigated. The spin-lattice relaxation rate 1/T11/T_1 in the superconducting (SC) and normal states is almost the same for the two samples except just above TcT_c. NQR measurements were also performed on different-hydrate-content samples with different TcT_c values, which were prepared from the same Na-content (xx = 0.348) sample. From measurements of 1/T11/T_1 using the different-hydrate-content samples, it was found that a low-TcT_c sample with Tc=3.9T_c = 3.9 K has a larger residual density of states (DOS) in the SC state and a smaller increase of 1/T1T1/T_1T just above TcT_c than a high-TcT_c sample with TcT_c = 4.7 K. The former behavior is consistent with that observed in unconventional superconductors, and the latter suggests the relationship between TcT_c and the increase in DOS just above TcT_c. This increase, which is seemingly associated with the two-dimensionality of the CoO2_2 plane, is considered to be one of the most important factors for the occurrence of superconductivity.Comment: 5 pages, 5 figures, To be published in J. Phys. Soc. Jp

    Effects to Scalar Meson Decays of Strong Mixing between Low and High Mass Scalar Mesons

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    We analyze the mass spectroscopy of low and high mass scalar mesons and get the result that the coupling strengths of the mixing between low and high mass scalar mesons are very strong and the strengths of mixing for I=1,1/2I=1, 1/2 scalar mesons and those of I=0 scalar mesons are almost same. Next, we analyze the decay widths and decay ratios of these mesons and get the results that the coupling constants A′A' for I=1,1/2I=1, 1/2 which represents the coupling of high mass scalar meson N′N' -> two pseudoscalar mesons PPPP are almost same as the coupling A′A' for the I=0. On the other hand, the coupling constant AA for I=1,I=1/2I=1, I=1/2 which represents the low mass scalar meson NN -> PPPP are far from the coupling constant AA for I=0. We consider a resolution for this discrepancy. Coupling constant A′′A'' for glueball GG -> PPPP is smaller than the coupling A′A'. θP\theta_P is 40∘∼50∘40^\circ \sim 50^\circ.Comment: 15 pages, 6 figure

    Rise of Kp Total Cross Section and Universality

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    The increase of the measured hadronic total cross sections at the highest energies is empirically described by squared log of center-of-mass energy sqrt s as sigma(tot)= B (log s)2, consistent with the energy dependence of the Froissart unitarity bound. The coefficient B is argued to have a universal value, but this is not proved directly from QCD. In the previous tests of this universality, the p(pbar)p, pi p, and K p forward scatterings were analyzed independently and found to be consistent with B(pp) = B(pip) = B(Kp), although the determined value of B(Kp) had large uncertainty. In the present work, we have further analyzed forward Kp scattering to obtain a more exact value of B(Kp). Making use of continuous moment sum rules(CMSR) we have fully exploited the information of low-energy scattering data to predict the high-energy behavior of the amplitude hrough duality. The estimation of B(Kp) is improved remarkably, and our result strongly supports the universality of B.Comment: 12 pages, 3 figure

    Estimates of isospin breaking contributions to baryon masses

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    We estimate the isospin breaking contributions to the baryon masses which we analyzed recently using a loop expansion in the heavy baryon approximation to chiral effective field theory. To one loop, the isospin breaking corrections come from the effects of the d,ud, u quark mass difference, the Coulomb and magnetic moment interactions, and effective point interactions attributable to color-magnetic effects. The addition of the first meson loop corrections introduces new structure. We estimate the resulting low-energy, long-range contributions to the mass splittings by regularizing the loop integrals using connections to dynamical models for finite-size baryons. We find that the resulting contributions to the isospin breaking corrections are of the right general size, have the correct sign pattern, and agree with the experimental values within the margin of error.Comment: 15 pages, 5 figures; changed title and conten

    Evidence for Strong-coupling S-wave Superconductivity in MgB2 :11B NMR Study

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    We have investigated a gap structure in a newly-discovered superconductor, MgB2 through the measurement of 11B nuclear spin-lattice relaxation rate, ^{11}(1/T_1). ^{11}(1/T_1) is proportional to the temperature (T) in the normal state, and decreases exponentially in the superconducting (SC) state, revealing a tiny coherence peak just below T_c. The T dependence of 1/T_1 in the SC state can be accounted for by an s-wave SC model with a large gap size of 2\Delta /k_BT_c \sim 5 which suggests to be in a strong-coupling regime.Comment: 2 pages with 1 figur

    Detectability of the First Cosmic Explosions

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    We present a fully self-consistent simulation of a synthetic survey of the furthermost cosmic explosions. The appearance of the first generation of stars (Population III) in the Universe represents a critical point during cosmic evolution, signaling the end of the dark ages, a period of absence of light sources. Despite their importance, there is no confirmed detection of Population III stars so far. A fraction of these primordial stars are expected to die as pair-instability supernovae (PISNe), and should be bright enough to be observed up to a few hundred million years after the big bang. While the quest for Population III stars continues, detailed theoretical models and computer simulations serve as a testbed for their observability. With the upcoming near-infrared missions, estimates of the feasibility of detecting PISNe are not only timely but imperative. To address this problem, we combine state-of-the-art cosmological and radiative simulations into a complete and self-consistent framework, which includes detailed features of the observational process. We show that a dedicated observational strategy using ≲8\lesssim 8 per cent of total allocation time of the James Webb Space Telescope mission can provide us up to ∼9−15\sim 9-15 detectable PISNe per year.Comment: 9 pages, 8 figures. Minor corrections added to match published versio
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