Observation of ordered phases of fullerenes in carbon nanotubes

Physical Review Letters 92 (2004) 245507 4pp

Authors:

AN Khlobystov, DA Britz, A Ardavan, GAD Briggs

Experimental demonstration of a new radiation mechanism: emission by an oscillating, accelerated, superluminal polarization current

(2004)

Authors:

A Ardavan, J Singleton, H Ardavan, J Fopma, D Halliday, W Hayes

Angle-dependent magnetoresistance of the layered organic superconductor κ-(ET)2Cu(NCS)2: Simulation and experiment

Physical Review B - Condensed Matter and Materials Physics 69:17 (2004)

Authors:

PA Goddard, SJ Blundell, J Singleton, RD McDonald, A Ardavan, A Narduzzo, JA Schlueter, AM Kini, T Sasaki

Abstract:

The angle dependences of the magnetoresistance of two different isotopic substitutions (deuterated and undeuterated) of the layered organic superconductor κ-(ET)2Cu(NCS)2 are presented (where ET is the organic molecule bis(ethylenedithio)-tetrathiafulvalene). The angle-dependent magnetoresistance oscillations (AMRO) arising from the quasi-one-dimensional and quasi-two-dimensional Fermi surfaces in this material are easily confused. By using the Boltzmann transport equation extensive simulations of the AMRO are made that reveal the subtle differences between the different species of oscillation. No significant differences are observed in the electronic parameters derived from quantum oscillations and AMRO for the two isotopic substitutions. The interlayer transfer integrals are determined for both isotopic substitutions and a slight difference is observed which may account for the negative isotope effect previously reported. The success of the semiclassical simulations suggests that non-Fermi liquid effects are not required to explain the interlayer transport in this system.

Landau levels, molecular orbitals, and the Hofstadter butterfly in finite systems

American Journal of Physics 72:5 (2004) 613-618

Authors:

JG Analytis, SJ Blundell, A Ardavan

Abstract:

The Hofstadter butterfly is the energy spectrum of an infinite square lattice, plotted as a function of the magnetic field. We illustrate a method of calculating similar spectra for finite lattices in a magnetic field, using methods that consider the appropriate molecular orbitals, and find that the spectra resemble the Hofstadter butterfly. We relate the bonding and antibonding orbitals used to describe small systems to the Landau levels of the infinite system. This approach provides an unusual, but instructive, method of introducing the physics of Landau levels from the basic quantum mechanics of small systems. © 2004 American Association of Physics Teachers.

Spectral and polarization characteristics of the nonspherically decaying radiation generated by polarization currents with superluminally rotating distribution patterns.

J Opt Soc Am A Opt Image Sci Vis 21:5 (2004) 858-872

Authors:

Houshang Ardavan, Arzhang Ardavan, John Singleton

Abstract:

We present a theoretical study of the emission from a superluminal polarization current whose distribution pattern rotates (with an angular frequency omega) and oscillates (with a frequency Omega) at the same time and that comprises both poloidal and toroidal components. This type of polarization current is found in recent practical machines designed to investigate superluminal emission. We find that the superluminal motion of the distribution pattern of the emitting current generates localized electromagnetic waves that do not decay spherically, i.e., that do not have an intensity diminishing as RP(-2) with the distance RP from their source. The nonspherical decay of the focused wave packets that are emitted by the polarization currents does not contravene conservation of energy: The constructive interference of the constituent waves of such propagating caustics takes place within different solid angles on spheres of different radii (RP) centered on the source. For a polarization current whose longitudinal distribution (over an azimuthal interval of length 2pi) consists of m cycles of a sinusoidal wave train, the nonspherically decaying part of the emitted radiation contains the frequencies Omega +/- momega; i.e., it contains only the frequencies involved in the creation and implementation of the source. This is in contrast to recent studies of the spherically decaying emission, which was shown to contain much higher frequencies. The polarization of the emitted radiation is found to be linear for most configurations of the source.