1,274 research outputs found

    Optical Hall Effect in the Integer Quantum Hall Regime

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    Optical Hall conductivity σxy(ω)\sigma_{xy}(\omega) is measured from the Faraday rotation for a GaAs/AlGaAs heterojunction quantum Hall system in the terahertz frequency regime. The Faraday rotation angle (\sim fine structure constant \sim mrad) is found to significantly deviate from the Drude-like behavior to exhibit a plateau-like structure around the Landau-level filling ν=2\nu=2. The result, which fits with the behavior expected from the carrier localization effect in the ac regime, indicates that the plateau structure, although not quantized, still exists in the terahertz regime.Comment: 4 pages, 4 figure

    Sub-wavelength imaging at infrared frequencies using an array of metallic nanorods

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    We demonstrate that an array of metallic nanorods enables sub-wavelength (near-field) imaging at infrared frequencies. Using an homogenization approach, it is theoretically proved that under certain conditions the incoming radiation can be transmitted by the array of nanorods over a significant distance with fairly low attenuation. The propagation mechanism does not involve a resonance of material parameters and thus the resolution is not strongly affected by material losses and has wide bandwidth. The sub-wavelength imaging with λ/10\lambda/10 resolution by silver rods at 30 THz is demonstrated numerically using full-wave electromagnetic simulator.Comment: 12 pages, 16 figures, submitted to PR

    Frequency-Dependent Squeezing for Advanced LIGO

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    The first detection of gravitational waves by the Laser Interferometer Gravitational-wave Observatory (LIGO) in 2015 launched the era of gravitational wave astronomy. The quest for gravitational wave signals from objects that are fainter or farther away impels technological advances to realize ever more sensitive detectors. Since 2019, one advanced technique, the injection of squeezed states of light is being used to improve the shot noise limit to the sensitivity of the Advanced LIGO detectors, at frequencies above 50\sim 50 Hz. Below this frequency, quantum back action, in the form of radiation pressure induced motion of the mirrors, degrades the sensitivity. To simultaneously reduce shot noise at high frequencies and quantum radiation pressure noise at low frequencies requires a quantum noise filter cavity with low optical losses to rotate the squeezed quadrature as a function of frequency. We report on the observation of frequency-dependent squeezed quadrature rotation with rotation frequency of 30Hz, using a 16m long filter cavity. A novel control scheme is developed for this frequency-dependent squeezed vacuum source, and the results presented here demonstrate that a low-loss filter cavity can achieve the squeezed quadrature rotation necessary for the next planned upgrade to Advanced LIGO, known as "A+."Comment: 6 pages, 2 figures, to be published in Phys. Rev. Let

    Metallic Carbon Nanotube Quantum Dots with Broken Symmetries as a Platform for Tunable Terahertz Detection

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    Quantum dots (QD) in metallic single-walled carbon nanotubes (SWNT) have shown great potential to build sensitive terahertz (THz) detection devices usually based on photon-assisted tunneling. A recently reported mechanism based on a combination of resonant QD transitions and asymmetries in the tunneling barriers results in narrow linewidth photocurrent response with a large signal to noise ratio under weak THz radiation. However in such devices, due to metallic SWNTs linear dispersion relation, the detection range is intrinsically limited to allowed energy transitions between equidistant quantized states set by the QD length. Here, we show that simultaneously breaking translational, rotational and mirror symmetries in metallic SWNT QDs leads to a quantized spectrum with non-equidistant energy levels. This result stems from tight-binding and first-principle simulations of a defect-induced metallic zigzag SWNT QD and is validated experimentally by scanning tunneling spectroscopy studies. Importantly, we show that breaking symmetries in metallic SWNT QDs of arbitrary chirality strongly relaxes the selection rules in the electric dipole approximation, leading to a richer set of allowed optical transitions spanning frequencies from as low as 1 THz up to several tens of THz for a \sim10 nm QD. Such findings make metallic carbon nanotube QDs with broken symmetries a promising platform to design tunable THz detectors operating above liquid helium temperatures. In this context, we propose a device design based on a metallic SWNT QD engineered with artificially created defects.Comment: 20 pages, 15 figure

    Properties of metastable alkaline-earth-metal atoms calculated using an accurate effective core potential

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    The first three electronically excited states in the alkaline-earth-metal atoms magnesium, calcium, and strontium comprise the (nsnp) triplet P^o_J (J=0,1,2) fine-structure manifold. All three states are metastable and are of interest for optical atomic clocks as well as for cold-collision physics. An efficient technique--based on a physically motivated potential that models the presence of the ionic core--is employed to solve the Schroedinger equation for the two-electron valence shell. In this way, radiative lifetimes, laser-induced clock shifts, and long-range interaction parameters are calculated for metastable Mg, Ca, and Sr.Comment: 13 pages, 9 table

    Long-range behavior of the optical potential for the elastic scattering of charged composite particles

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    The asymptotic behavior of the optical potential, describing elastic scattering of a charged particle α\alpha off a bound state of two charged, or one charged and one neutral, particles at small momentum transfer Δα\Delta_{\alpha} or equivalently at large intercluster distance ρα\rho_{\alpha}, is investigated within the framework of the exact three-body theory. For the three-charged-particle Green function that occurs in the exact expression for the optical potential, a recently derived expression, which is appropriate for the asymptotic region under consideration, is used. We find that for arbitrary values of the energy parameter the non-static part of the optical potential behaves for Δα0\Delta_{\alpha} \rightarrow 0 as C1Δα+o(Δα)C_{1}\Delta_{\alpha} + o\,(\Delta_{\alpha}). From this we derive for the Fourier transform of its on-shell restriction for ρα\rho_{\alpha} \rightarrow \infty the behavior a/2ρα4+o(1/ρα4)-a/2\rho_{\alpha}^4 + o\,(1/\rho_{\alpha}^4), i.e., dipole or quadrupole terms do not occur in the coordinate-space asymptotics. This result corroborates the standard one, which is obtained by perturbative methods. The general, energy-dependent expression for the dynamic polarisability C1C_{1} is derived; on the energy shell it reduces to the conventional polarisability aa which is independent of the energy. We emphasize that the present derivation is {\em non-perturbative}, i.e., it does not make use of adiabatic or similar approximations, and is valid for energies {\em below as well as above the three-body dissociation threshold}.Comment: 35 pages, no figures, revte

    Testing Lorentz and CPT symmetry with hydrogen masers

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    We present details from a recent test of Lorentz and CPT symmetry using hydrogen masers. We have placed a new limit on Lorentz and CPT violation of the proton in terms of a recent standard model extension by placing a bound on sidereal variation of the F = 1 Zeeman frequency in hydrogen. Here, the theoretical standard model extension is reviewed. The operating principles of the maser and the double resonance technique used to measure the Zeeman frequency are discussed. The characterization of systematic effects is described, and the method of data analysis is presented. We compare our result to other recent experiments, and discuss potential steps to improve our measurement.Comment: 26 pages, 16 figure

    A constraint on antigravity of antimatter from precision spectroscopy of simple atoms

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    Consideration of antigravity for antiparticles is an attractive target for various experimental projects. There are a number of theoretical arguments against it but it is not quite clear what kind of experimental data and theoretical suggestions are involved. In this paper we present straightforward arguments against a possibility of antigravity based on a few simple theoretical suggestions and some experimental data. The data are: astrophysical data on rotation of the Solar System in respect to the center of our galaxy and precision spectroscopy data on hydrogen and positronium. The theoretical suggestions for the case of absence of the gravitational field are: equality of electron and positron mass and equality of proton and positron charge. We also assume that QED is correct at the level of accuracy where it is clearly confirmed experimentally
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