12,543 research outputs found

    The Origin of Gamma-Rays from Globular Clusters

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    Fermi has detected gamma-ray emission from eight globular clusters. We suggest that the gamma-ray emission from globular clusters may result from the inverse Compton scattering between relativistic electrons/positrons in the pulsar wind of MSPs in the globular clusters and background soft photons including cosmic microwave/relic photons, background star lights in the clusters, the galactic infrared photons and the galactic star lights. We show that the gamma-ray spectrum from 47 Tuc can be explained equally well by upward scattering of either the relic photons, the galactic infrared photons or the galactic star lights whereas the gamma-ray spectra from other seven globular clusters are best fitted by the upward scattering of either the galactic infrared photons or the galactic star lights. We also find that the observed gamma-ray luminosity is correlated better with the combined factor of the encounter rate and the background soft photon energy density. Therefore the inverse Compton scattering may also contribute to the observed gamma-ray emission from globular clusters detected by Fermi in addition to the standard curvature radiation process. Furthermore, we find that the emission region of high energy photons from globular cluster produced by inverse Compton scattering is substantially larger than the core of globular cluster with a radius >10pc. The diffuse radio and X-rays emitted from globular clusters can also be produced by synchrotron radiation and inverse Compton scattering respectively. We suggest that future observations including radio, X-rays, and gamma-rays with energy higher than 10 GeV and better angular resolution can provide better constraints for the models.Comment: Accepted by ApJ, Comments may send to Prof. K.S. Cheng: [email protected]

    The Fundamental Plane of Gamma-ray Globular Clusters

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    We have investigated the properties of a group of γ\gamma-ray emitting globular clusters (GCs) which have recently been uncovered in our Galaxy. By correlating the observed γ\gamma-ray luminosities LγL_{\gamma} with various cluster properties, we probe the origin of the high energy photons from these GCs. We report LγL_{\gamma} is positively correlated with the encounter rate Γc\Gamma_{c} and the metalicity [Fe/H]\left[{\rm Fe/H}\right] which place an intimate link between the gamma-ray emission and the millisecond pulsar population. We also find a tendency that LγL_{\gamma} increase with the energy densities of the soft photon at the cluster location. Furthermore, the two-dimensional regression analysis suggests that LγL_{\gamma}, soft photon densities, and Γc\Gamma_{c}/[Fe/H]\left[{\rm Fe/H}\right] possibly span fundamental planes which potentially provide better predictions for the γ\gamma-ray properties of GCs.Comment: 17 pages, 4 figures, 3 tables, published in Ap

    Correlation effects during liquid infiltration into hydrophobic nanoporous mediums

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    Correlation effects arising during liquid infiltration into hydrophobic porous medium are considered. On the basis of these effects a mechanism of energy absorption at filling porous medium by nonwetting liquid is suggested. In accordance with this mechanism, the absorption of mechanical energy is a result expenditure of energy for the formation of menisci in the pores on the shell of the infinite cluster and expenditure of energy for the formation of liquid-porous medium interface in the pores belonging to the infinite cluster of filled pores. It was found that in dependences on the porosity and, consequently, in dependences on the number of filled pores neighbors, the thermal effect of filling can be either positive or negative and the cycle of infiltration-defiltration can be closed with full outflow of liquid. It can occur under certain relation between percolation properties of porous medium and the energy characteristics of the liquid-porous medium interface and the liquid-gas interface. It is shown that a consecutive account of these correlation effects and percolation properties of the pores space during infiltration allow to describe all experimental data under discussion

    Growth of High-Mobility Bi2Te2Se Nanoplatelets on hBN Sheets by van der Waals Epitaxy

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    The electrical detection of the surface states of topological insulators is strongly impeded by the interference of bulk conduction, which commonly arises due to pronounced doping associated with the formation of lattice defects. As exemplified by the topological insulator Bi2Te2Se, we show that via van der Waals epitaxial growth on thin hBN substrates the structural quality of such nanoplatelets can be substantially improved. The surface state carrier mobility of nanoplatelets on hBN is increased by a factor of about 3 compared to platelets on conventional Si/SiOx substrates, which enables the observation of well-developed Shubnikov-de Haas oscillations. We furthermore demonstrate the possibility to effectively tune the Fermi level position in the films with the aid of a back gate

    Magnetic fluctuations and superconducting properties of CaKFe4As4 studied by 75As NMR

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    We report 75^{75}As nuclear magnetic resonance (NMR) studies on a new iron-based superconductor CaKFe4_4As4_4 with TcT_{\rm c} = 35 K. 75^{75}As NMR spectra show two distinct lines corresponding to the As(1) and As(2) sites close to the K and Ca layers, respectively, revealing that K and Ca layers are well ordered without site inversions. We found that nuclear quadrupole frequencies νQ\nu_{\rm Q} of the As(1) and As(2) sites show an opposite temperature (TT) dependence. Nearly TT independent behavior of the Knight shifts KK are observed in the normal state, and a sudden decrease in KK in the superconducting (SC) state clearly evidences spin-singlet Cooper pairs. 75^{75}As spin-lattice relaxation rates 1/T1T_1 show a power law TT dependence with different exponents for the two As sites. The isotropic antiferromagnetic spin fluctuations characterized by the wavevector q{\bf q} = (π\pi, 0) or (0, π\pi) in the single-iron Brillouin zone notation are revealed by 1/T1TT_1T and KK measurements. Such magnetic fluctuations are necessary to explain the observed temperature dependence of the 75^{75}As quadrupole frequencies, as evidenced by our first-principles calculations. In the SC state, 1/T1T_1 shows a rapid decrease below TcT_{\rm c} without a Hebel-Slichter peak and decreases exponentially at low TT, consistent with an s±s^{\pm} nodeless two-gap superconductor.Comment: 9 pages, 6 figures, accepted for publication in Phys.Rev.

    Open-closed field algebras

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    We introduce the notions of open-closed field algebra and open-closed field algebra over a vertex operator algebra V. In the case that V satisfies certain finiteness and reductivity conditions, we show that an open-closed field algebra over V canonically gives an algebra over a \C-extension of the Swiss-cheese partial operad. We also give a tensor categorical formulation and categorical constructions of open-closed field algebras over V.Comment: 55 pages, largely revised, an old subsection is deleted, a few references are adde

    Multiband model for tunneling in MgB2 junctions

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    A theoretical model for quasiparticle and Josephson tunneling in multiband superconductors is developed and applied to MgB2-based junctions. The gap functions in different bands in MgB2 are obtained from an extended Eliashberg formalism, using the results of band structure calculations. The temperature and angle dependencies of MgB2 tunneling spectra and the Josephson critical current are calculated. The conditions for observing one or two gaps are given. We argue that the model may help to settle the current debate concerning two-band superconductivity in MgB2.Comment: minor corrections, published in Phys. Rev. B 65, 180517(R) (2002

    Performance and modeling of superconducting ring resonators at millimeter-wave frequencies

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    Microstrip ring resonators operating at 35 GHz were fabricated from laser ablated YBCO thin films deposited on lanthanum aluminate substrates. They were measured over a range of temperatures and their performance compared to identical resonators made of evaporated gold. Below 60 Kelvin the superconducting strip performed better than the gold, reaching an unloaded Q approximately 1.5 times that of gold at 25 K. A shift in the resonant frequency follows the form predicted by the London equations. The Phenomenological Loss Equivalence Method is applied to the ring resonator and the theoretically calculated Q values are compared to the experimental results
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