28 research outputs found

    Vortex lattices in strong type-II superconducting two-dimensional strips

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    We show how to calculate semi-analytically the dense vortex state in strong type-II superconducting nanostructures. For the specific case of a strip, we find vortex lattice solutions which also incorporate surface superconductivity. We calculate the energy cost to displace individual vortex rows parallel to the surfaces and find that this energy oscillates with the magnetic field. Remarkably, we also find that, at a critical field H∗H^* below Hc2H_{c2}, this ''shear'' energy becomes strictly zero for the surface rows due to an unexpected mismatch with the bulk lattice.Comment: Title, abstract, and some text paragraphs have been rewritte

    Bremsstrahlung Suppression due to the LPM and Dielectric Effects in a Variety of Materials

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    The cross section for bremsstrahlung from highly relativistic particles is suppressed due to interference caused by multiple scattering in dense media, and due to photon interactions with the electrons in all materials. We present here a detailed study of bremsstrahlung production of 200 keV to 500 MeV photons from 8 and 25 GeV electrons traversing a variety of target materials. For most targets, we observe the expected suppressions to a good accuracy. We observe that finite thickness effects are important for thin targets.Comment: 52 pages, 13 figures (incorporated in the revtex LaTeX file

    The ac magnetic response of mesoscopic type II superconductors

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    The response of mesoscopic superconductors to an ac magnetic field is numerically investigated on the basis of the time-dependent Ginzburg-Landau equations (TDGL). We study the dependence with frequency ω\omega and dc magnetic field HdcH_{dc} of the linear ac susceptibility χ(Hdc,ω)\chi(H_{dc}, \omega) in square samples with dimensions of the order of the London penetration depth. At Hdc=0H_{dc}=0 the behavior of χ\chi as a function of ω\omega agrees very well with the two fluid model, and the imaginary part of the ac susceptibility, χ"(ω)\chi"(\omega), shows a dissipative a maximum at the frequency Îœo=c2/(4πσλ2)\nu_o=c^2/(4\pi \sigma\lambda^2). In the presence of a magnetic field a second dissipation maximum appears at a frequency ωpâ‰ȘÎœ0\omega_p\ll\nu_0. The most interesting behavior of mesoscopic superconductors can be observed in the χ(Hdc)\chi(H_{dc}) curves obtained at a fixed frequency. At a fixed number of vortices, χ"(Hdc)\chi"(H_{dc}) continuously increases with increasing HdcH_{dc}. We observe that the dissipation reaches a maximum for magnetic fields right below the vortex penetration fields. Then, after each vortex penetration event, there is a sudden suppression of the ac losses, showing discontinuities in χ"(Hdc)\chi"(H_{dc}) at several values of HdcH_{dc}. We show that these discontinuities are typical of the mesoscopic scale and disappear in macroscopic samples, which have a continuos behavior of χ(Hdc)\chi(H_{dc}). We argue that these discontinuities in χ(Hdc)\chi(H_{dc}) are due to the effect of {\it nascent vortices} which cause a large variation of the amplitude of the order parameter near the surface before the entrance of vortices.Comment: 12 pages, 9 figures, RevTex

    The theory of the Landau, Pomeranchuk, Migdal effect

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    Bremsstrahlung of photons from highly relativistic electrons is investigated. The cross section of the processes, which is suppressed due to a multiple scattering of an emitting electron in dense media (LPM effect) and due to photon interaction with electrons of a medium, is calculated with an accuracy up to "next to leading logarithm" and with the Coulomb corrections taken into account. Making allowances for a multiple scattering and a polarization of a medium an analysis of radiation on a target boundary is carried out. The method of consideration of radiation in a thin target under influence of the LPM effect is developed. Interrelation with the recent experiment is discussed.Comment: 36 pages, LaTeX, 3 eps figure

    The Flux-Line Lattice in Superconductors

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    Magnetic flux can penetrate a type-II superconductor in form of Abrikosov vortices. These tend to arrange in a triangular flux-line lattice (FLL) which is more or less perturbed by material inhomogeneities that pin the flux lines, and in high-TcT_c supercon- ductors (HTSC's) also by thermal fluctuations. Many properties of the FLL are well described by the phenomenological Ginzburg-Landau theory or by the electromagnetic London theory, which treats the vortex core as a singularity. In Nb alloys and HTSC's the FLL is very soft mainly because of the large magnetic penetration depth: The shear modulus of the FLL is thus small and the tilt modulus is dispersive and becomes very small for short distortion wavelength. This softness of the FLL is enhanced further by the pronounced anisotropy and layered structure of HTSC's, which strongly increases the penetration depth for currents along the c-axis of these uniaxial crystals and may even cause a decoupling of two-dimensional vortex lattices in the Cu-O layers. Thermal fluctuations and softening may melt the FLL and cause thermally activated depinning of the flux lines or of the 2D pancake vortices in the layers. Various phase transitions are predicted for the FLL in layered HTSC's. The linear and nonlinear magnetic response of HTSC's gives rise to interesting effects which strongly depend on the geometry of the experiment.Comment: Review paper for Rep.Prog.Phys., 124 narrow pages. The 30 figures do not exist as postscript file

    On the macroscopic formation length for GeV photons

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    Experimental results for the radiative energy loss of 206 and 234 GeV electrons in 5–10 ÎŒm thin Ta targets are presented. An increase in radiation emission probability at low photon energies compared to a 100 ÎŒm thick target is observed. This increase is due to the formation length of the GeV photons exceeding the thickness of the thin foils, the so-called Ternovskii–Shul'ga–Fomin (TSF) effect. The formation length of GeV photons from a multi-hundred GeV projectile is through the TSF effect shown directly to be a factor 1010 longer than their wavelength
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