8,407 research outputs found

    Peak-Dip-Hump from Holographic Superconductivity

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    We study the fermionic spectral function in a holographic superconductor model. At zero temperature, the black hole has zero horizon and hence the entropy of the system is zero after the back reaction of the condensate is taken into account. We find the system exhibits the famous peak-dip-hump lineshape with a sharp low-energy peak followed by a dip then a hump at higher energies. This feature is widely observed in the spectrum of several high-T_c superconductors. We also find a linear relation between the gap in the fermionic spectrum and the condensate, indicating the condensate is formed by fermion pairing.Comment: 4 pages, revtex

    The nature of ZbZ_b states from a combined analysis of Υ(5S)hb(mP)π+π\Upsilon(5S)\rightarrow h_b(mP) \pi^+ \pi^- and Υ(5S)B()Bˉ()π\Upsilon(5S)\rightarrow B^{(\ast)}\bar B^{(\ast)}\pi

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    With a combined analysis of data on Υ(5S)hb(1P,2P)π+π\Upsilon(5S)\rightarrow h_b(1P,2P)\pi^+\pi^- and Υ(5S)B()Bˉ()π\Upsilon(5S)\rightarrow B^{(\ast)}\bar B^{(\ast)}\pi in an effective field theory approach, we determine resonance parameters of ZbZ_b states in two scenarios. In one scenario we assume that ZbZ_b states are pure molecular states, while in the other one we assume that ZbZ_b states contain compact components. We find that the present data favor that there should be some compact components inside Zb()Z_b^{(\prime)} associated with the molecular components. By fitting the invariant mass spectra of Υ(5S)hb(1P,2P)π+π\Upsilon(5S)\rightarrow h_b(1P,2P)\pi^+\pi^- and Υ(5S)B()Bˉπ\Upsilon(5S)\rightarrow B^{(\ast)}\bar B^{\ast}\pi, we determine that the probability of finding the compact components in ZbZ_b states may be as large as about 40%40\%.Comment: Discussions added, version published in EPJ

    Dynamic Interrelation of Births and Deaths: Evidence from Plant Level Data

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    In this paper, the dynamic panel data method is used to investigate the dynamic interrelation of plant births and plant deaths. The dynamic panel data method considers the endogenous problem and individual effects. Empirical findings support the multiplier effect. In addition, exit does not cause entry, whereas entry causes exit.

    Ruling out the supersoft high-density symmetry energy from the discovery of PSR J0740+6620 with mass 2.140.09+0.10M2.14^{+0.10}_{-0.09}M_\odot

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    Using the very recently reported mass 2.140.09+0.10M2.14^{+0.10}_{-0.09}M_\odot of PSR J0740+6620 together with the data of finite nuclei and the constraints on the equation of state of symmetric nuclear matter at suprasaturation densities from flow data in heavy-ion collisions, we show that the symmetry energy Esym(n)E_{\rm sym}(n) cannot be supersoft so that it becomes negative at suprasaturation densities in neutron stars (NSs) and thus may make the NS have a pure neutron matter core. This is in contrast to the fact that using the mass 2.01±0.04M2.01 \pm 0.04 M_\odot of PSR J0348+0432 as the NS maximum mass cannot rule out the supersoft high-density Esym(n)E_{\rm sym}(n). Furthermore, we find the stiffer high-density Esym(n)E_{\rm sym}(n) based on the existence of 2.14M2.14M_\odot NSs leads to a strong constraint of Λ1.434851+88\Lambda_{1.4} \ge 348^{+88}_{-51} for the dimensionless tidal deformability of the canonical 1.4M1.4M_\odot NS.Comment: 8 pages, 2 figures, 1 table. The updated 2.14 solar mass used, results updated and presentation improved. Accepted version to appear in Ap

    Holographic Mutual Information of Two Disjoint Spheres

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    We study quantum corrections to holographic mutual information for two disjoint spheres at a large separation by using the operator product expansion of the twist field. In the large separation limit, the holographic mutual information is vanishing at the semiclassical order, but receive quantum corrections from the fluctuations. We show that the leading contributions from the quantum fluctuations take universal forms as suggested from the boundary CFT. We find the universal behavior for the scalar, the vector, the tensor and the fermionic fields by treating these fields as free fields propagating in the fixed background and by using the 1/n prescription. In particular, for the fields with gauge symmetries, including the massless vector boson and massless graviton, we find that the gauge parts in the propagators play indispensable role in reading the leading order corrections to the bulk mutual information.Comment: 37 pages, 1 figure; significant revisions, corrected the discussions on the computations of the mutual information in CFT, conclusions unchange
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