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D. Richardson

Publications and source records attributed to D. Richardson.

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Extraction of Effective Electromagnetic Material Properties for Rydberg Electrometer Vapor Cells from 10-300 MHz

Quantum sensors often consist of packaging, such as dielectric-based vapor cells and metallic electrodes, that reduces and spatially alters the locally observed electromagnetic fields. These effects have been well studied in the optical regime, and even in the RF regime over a few GHz. However, there have been few studies in the electrically small regime below 1 GHz. In order to account for or remove the effects of the packaging, more studies are needed across a broad range of frequencies. This paper reports on the complex permittivity and conductivity of several commercially available vapor cells used for Rydberg electric field sensing from 10-300 MHz. A new method using a stripline transmission measurement was performed and full wave electromagnetics modeling was used to extract the effective dielectric constitutive parameters from the vapor cells. Additionally, the field reduction inside the vapor cell is reported, and published atomic measurements of the electric field are used to further validate the results presented here. Several observations were made from the measurements, such as the frequency dependencies of the RF dispersion and absorption. Applications of this technique include making precise numerical field corrections or physically designing a more optimal vapor cell via coatings, material changes, or geometric changes to improve field strength and uniformity.

physics.atom-ph

Chang-Refsdal Microlensed Type Ia Supernova Light Curves

A description of the light curves of microlensed Type Ia supernovae (SNe Ia) as extended and expanding sources is presented. We give examples of what microlensing by stellar-mass Chang-Refsdal lenses can do to a small percentage of supernova light curves. We find that in addition to overall brightening, significant changes in light--curve shapes can also occur. Peaks can be distorted, plateaus can appear, and even secondary peaks can be formed. The effects of both the relative motion of the lens and the supernova and the expansion of the supernova are given and compared. The effects of relative motion are more pronounced when a distant supernova ($z_s \sim 1$) impacts well within the Einstein ring of a nearby microlens ($z_d \sim 0.05$) and are less important for more distant deflectors. We also find that the increase in shear that comes with increased deflector distance tends to reduce the time variability of microlensing. We briefly discuss the probability of observing these effects.

astro-ph

Cold atoms probe the magnetic field near a wire

A microscopic Ioffe-Pritchard trap is formed using a straight, current-carrying wire, together with suitable auxiliary magnetic fields. By measuring the distribution of cold rubidium atoms held in this trap, we detect a weak magnetic field component $ΔB_z$ parallel to the wire. This field is proportional to the current in the wire and is approximately periodic along the wire with period $λ=230 μ$m. We find that the decrease of this field with distance from the centre of the wire is well described by the Bessel function $K_1(2πy/λ)$, as one would expect for the far field of a transversely oscillating current within the wire.

cond-mat