425 research outputs found
On-Chip Microwave Quantum Hall Circulator
Circulators are non-reciprocal circuit elements integral to technologies
including radar systems, microwave communication transceivers, and the readout
of quantum information devices. Their non-reciprocity arises from the
interference of microwaves over the centimetre-scale of the signal wavelength
in the presence of bulky magnetic media that break time-reversal symmetry. Here
we realize a completely passive on-chip microwave circulator with size
one-thousandth the wavelength by exploiting the chiral, slow-light response of
a 2-dimensional electron gas (2DEG) in the quantum Hall regime. For an
integrated GaAs device with 330 um diameter and 1 GHz centre frequency, a
non-reciprocity of 25 dB is observed over a 50 MHz bandwidth. Furthermore, the
direction of circulation can be selected dynamically by varying the magnetic
field, an aspect that may enable reconfigurable passive routing of microwave
signals on-chip
Galaxy-Quasar correlations between APM galaxies and Hamburg-ESO QSOs
We detect angular galaxy-QSO cross-correlations between the APM Galaxy
Catalogue and a preliminary release (consisting of roughly half of the
anticipated final catalogue) of the Hamburg-ESO Catalogue of Bright QSOs as a
function of source QSO redshift using multiple cross-correlation estimators.
Each of the estimators yield very similar results, implying that the APM
catalogue and the Hamburg-ESO survey are both fair samples of the respective
true galaxy and QSO populations. Though the signal matches the expectations of
gravitational lensing qualitatively, the strength of the measured
cross-correlation signal is significantly greater than the CDM models of
lensing by large scale structure would suggest. This same disagreement between
models and observation has been found in several earlier studies. We estimate
our confidence in the correlation detections versus redshift by generating 1000
random realizations of the Hamburg-ESO QSO survey: We detect physical
associations between galaxies and low-redshift QSOs at 99% confidence and
detect lensing associations at roughly 95% confidence for QSOs with redshifts
between 0.6 and 1. Control cross-correlations between Galactic stars and QSOs
show no signal. Finally, the overdensities (underdensities) of galaxies near
QSO positions relative to those lying roughly 135 - 150 arcmin away are
uncorrelated with differences in Galactic extinction between the two regions,
implying that Galactic dust is not significantly affecting the QSO sample.Comment: 35 pages total, including 9 figures. Accepted by the Astrophysical
Journa
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