19,675 research outputs found

    Detecting the orbital character of the spin fluctuation in the Iron-based superconductors with the resonant inelastic X-ray scattering spectroscopy

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    The orbital distribution of the spin fluctuation in the iron-based superconductors(IBSs) is the key information needed to understand the magnetism, superconductivity and electronic nematicity in these multi-orbital systems. In this work, we propose that the resonant inelastic X-ray scattering(RIXS) technique can be used to probe selectively the spin fluctuation on different Fe 3d3d orbitals. In particular, the spin fluctuation on the three t2gt_{2g} orbitals, namely, the 3dxz3d_{xz}, 3dyz3d_{yz} and the 3dxy3d_{xy} orbital, can be selectively probed in the Οƒβ†’Ο€β€²\sigma\rightarrow\pi' scattering geometry by aligning the direction of the outgoing photon in the yy, xx and zz direction. Such orbital-resolved information on the spin fluctuation is invaluable for the study of the orbital-selective physics in the IBSs and can greatly advance our understanding on the relation between orbital ordering and spin nematicity in the IBSs and the orbital-selective pairing mechanism in these multi-orbital systems.Comment: 6 pages with new and more informative figures, the explicit form of the RIXS matrix element is provided, and the discussion part has been rewritte

    Vanishing pseudogap around (Ο€,0)(\pi,0) in an electron-doped high-Tc\mathrm{T_{c}} superconductor: a simple picture

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    Recent ARPES measurement on electron-doped cuprate Pr1.3βˆ’xLa0.7CexCuO4\mathrm{Pr}_{1.3-x}\mathrm{La}_{0.7}\mathrm{Ce}_{x}\mathrm{CuO}_{4} finds that the pseudogap along the boundary of the antiferromagnetic Brillouin zone(AFBZ) exhibits dramatic momentum dependence. In particular, the pseudogap vanishes in a finite region around the anti-nodal point, in which a single broadened peak emerges at the un-renormalized quasiparticle energy. Such an observation is argued to be inconsistent with the antiferromagnetic(AFM) band-folding picture, which predicts a constant pseudogap along the AFBZ boundary. On the other hand, it is claimed that the experimental results are consistent with the prediction of the cluster dynamical mean field theory(CDMFT) simulation on the Hubbard model, in which the pseudogap is interpreted as a s-wave splitting between the Hubbard bands and the in-gap states. Here we show that the observed momentum dependence of the pseudogap is indeed consistent with AFM band-folding picture, provided that we assume the existence of a strongly momentum dependent quasiparticle scattering rate. More specifically, we show that the quasiparticle scattering rate acts to reduce the spectral gap induced by AFM band-folding effect. The new quasiparticle poles corresponding to the AF-split bands can even be totally eliminated when the scattering rate exceeds the bare band folding gap, leaving the system with a single pole at the un-renormalized quasiparticle energy. We predict that the pseudogap should close in a square root fashion as we move toward (Ο€,0)(\pi,0) along the AFBZ boundary. Our results illustrates again that the quasiparticle scattering rate can play a much more profound role than simply broadening the quasiparticle peak in the quasiparticle dynamics of strongly correlated electron systems.Comment: 5 pages, 2 figures, new references adde

    Unparticle Physics Effects on D0-anti-D0 Mixing

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    The mixing of K0βˆ’K0Λ‰K^0-\bar{K^0}, D0βˆ’D0Λ‰D^0-\bar{D^0} and B(s)0βˆ’B(s)0Λ‰B_{(s)}^0-\bar{B^0_{(s)}} provides a sensitive probe to explore new physics beyond the Standard Model. The scale invariant unparticle physics recently proposed by Georgi can induce flavor-changing neutral current and contribute to the mixing at tree level. We investigate the unparticle effects on B0βˆ’B0Λ‰B^0-\bar{B^0} and D0βˆ’D0Λ‰D^0-\bar{D^0} mixing. Especially, the newly observed D0βˆ’D0Λ‰D^0-\bar{D^0} mixing sets the most stringent constraints on the coupling of the unparticle to quarks.Comment: 9 pages, some errors corrected, published versio

    Is Zc(3900)Z_c(3900) a molecular state

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    Assuming the newly observed Zc(3900)Z_c(3900) to be a molecular state of DDΛ‰βˆ—(Dβˆ—DΛ‰)D\bar D^*(D^{*} \bar D), we calculate the partial widths of Zc(3900)β†’J/ψ+Ο€;β€…β€ŠΟˆβ€²+Ο€;β€…β€ŠΞ·c+ρZ_c(3900)\to J/\psi+\pi;\; \psi'+\pi;\; \eta_c+\rho and DDΛ‰βˆ—D\bar D^* within the light front model (LFM). Zc(3900)β†’J/ψ+Ο€Z_c(3900)\to J/\psi+\pi is the channel by which Zc(3900)Z_c(3900) was observed, our calculation indicates that it is indeed one of the dominant modes whose width can be in the range of a few MeV depending on the model parameters. Similar to ZbZ_b and Zbβ€²Z_b', Voloshin suggested that there should be a resonance Zcβ€²Z_c' at 4030 MeV which can be a molecular state of Dβˆ—DΛ‰βˆ—D^*\bar D^*. Then we go on calculating its decay rates to all the aforementioned final states and as well the Dβˆ—DΛ‰βˆ—D^*\bar D^*. It is found that if Zc(3900)Z_c(3900) is a molecular state of 12(DDΛ‰βˆ—+Dβˆ—DΛ‰){1\over\sqrt 2}(D\bar D^*+D^*\bar D), the partial width of Zc(3900)β†’DDΛ‰βˆ—Z_c(3900)\to D\bar D^* is rather small, but the rate of Zc(3900)β†’Οˆ(2s)Ο€Z_c(3900)\to\psi(2s)\pi is even larger than Zc(3900)β†’J/ΟˆΟ€Z_c(3900)\to J/\psi\pi. The implications are discussed and it is indicated that with the luminosity of BES and BELLE, the experiments may finally determine if Zc(3900)Z_c(3900) is a molecular state or a tetraquark.Comment: 17 pages, 6 figures, 3 table

    Re-Study on the wave functions of Ξ₯(nS)\Upsilon(nS) states in LFQM and the radiative decays of Ξ₯(nS)β†’Ξ·b+Ξ³\Upsilon(nS)\to \eta_b+\gamma

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    The Light-front quark model (LFQM) has been applied to calculate the transition matrix elements of heavy hadron decays. However, it is noted that using the traditional wave functions of the LFQM given in literature, the theoretically determined decay constants of the Ξ₯(nS)\Upsilon(nS) obviously contradict to the data. It implies that the wave functions must be modified. Keeping the orthogonality among the nSnS states and fitting their decay constants we obtain a series of the wave functions for Ξ₯(nS)\Upsilon(nS). Based on these wave functions and by analogy to the hydrogen atom, we suggest a modified analytical form for the Ξ₯(nS)\Upsilon(nS) wave functions. By use of the modified wave functions, the obtained decay constants are close to the experimental data. Then we calculate the rates of radiative decays of Ξ₯(nS)β†’Ξ·b+Ξ³\Upsilon(nS)\to \eta_b+\gamma. Our predictions are consistent with the experimental data on decays Ξ₯(3S)β†’Ξ·b+Ξ³\Upsilon(3S)\to \eta_b+\gamma within the theoretical and experimental errors.Comment: 10 pages, 2 figures, 1 table. Typos corrected and more discussions added. accepted for publication in Physical Review
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