Signatures of discrete time-crystallinity in transport through quantum dot arrays

Discrete time-crystals are periodically driven quantum many-body systems with broken discrete-time translational symmetry. Measurements of time-crystallinity are currently limited to optical experiments due to the conception that the presence of an environment destroys the time-crystal behavior. We demonstrate that a periodically driven quantum dot array attached to electrodes exhibits both stable and meta-stable discrete time-crystal and quasi-crystal behaviors. These behaviors are manifested in spin-current measurable in transport set-up. The present-day availability of quantum dot arrays with electrically controllable sites makes our findings experimentally verifiable.Comment: Submitted for publication, comments are welcom

An Updated Study of Potential Targets for Ariel

Ariel has been selected as ESA's M4 mission for launch in 2028 and is designed for the characterisation of a large and diverse population of exoplanetary atmospheres to provide insights into planetary formation and evolution within our Galaxy. Here we present a study of Ariel's capability to observe currently-known exoplanets and predicted TESS discoveries. We use the Ariel Radiometric model (ArielRad) to simulate the instrument performance and find that ~2000 of these planets have atmospheric signals which could be characterised by Ariel. This list of potential planets contains a diverse range of planetary and stellar parameters. From these we select an example Mission Reference Sample (MRS), comprised of 1000 diverse planets to be completed within the primary mission life, which is consistent with previous studies. We also explore the mission capability to perform an in-depth survey into the atmospheres of smaller planets, which may be enriched or secondary. Earth-sized planets and Super-Earths with atmospheres heavier than H/He will be more challenging to observe spectroscopically. However, by studying the time required to observe ~110 Earth-sized/Super-Earths, we find that Ariel could have substantial capability for providing in-depth observations of smaller planets. Trade-offs between the number and type of planets observed will form a key part of the selection process and this list of planets will continually evolve with new exoplanet discoveries replacing predicted detections. The Ariel target list will be constantly updated and the MRS re-selected to ensure maximum diversity in the population of planets studied during the primary mission life

The DRAKE mission: finding the frequency of life in the Cosmos

In the search for life in the Universe, exoplanets represent numerous natural experiments in planet formation, evolution, and the emergence of life. This raises the fascinating prospect of evaluating cosmic life on a statistical basis. One key statistic is the occurrence rate of life-bearing worlds, fL, the ‘frequency of life’ term in the famous Drake Equation. Measuring fL would give profound insight into how common life is and may help to constrain origin-of-life theories. I propose fL as the goal for the DRAKE mission (Dedicated Research for Advancing Knowledge of Exobiology): a transit spectroscopy survey of M-dwarf habitable zone terrestrial planets. I investigate how the uncertainty on the observed value of fL scales with sample size. I determine that sampling error dominates over observational error and that the uncertainty is a function of the observed fL value. I show that even small sample sizes can provide significant constraints on fL, boding well for the transit spectroscopy approach. I perform a feasibility study of the DRAKE mission using a nominal instrument design and mission plan. Due to low observing efficiencies, DRAKE may need to be incorporated into a wider-ranging deep-space or lunar observatory. A 50-planet survey could constrain fL to ≤ 0.06 (at 95% confidence) if the sample fL = 0, or 0.03-0.2 if the sample fL = 0.1. This can be achieved (on average) in 10 years using a 17-m telescope with an unrestricted field-of-regard. DRAKE is a viable approach to attempting the first experimental measurement of fL