output
20022026
most citedEntanglement detection

2.4k citations

Showing 2021Show all

75 papers · 1 filter

astro-ph.EP202145 cited

High-resolution detection of neutral oxygen and non-LTE effects in the atmosphere of KELT-9b

Francesco Borsa, Luca Fossati, Tommi Koskinen +2

Oxygen is a constituent of many of the most abundant molecules detected in exoplanetary atmospheres and a key ingredient for tracking how and where a planet formed. In particular,…

astro-ph.EP202137 cited

The GAPS Programme at TNG. XXXII. The revealing non-detection of metastable HeI in the atmosphere of the hot Jupiter WASP-80b

L. Fossati, G. Guilluy, I. F. Shaikhislamov +38

The hot Jupiter WASP-80b has been identified as a possible excellent target for detecting and measuring HeI absorption in the upper atmosphere. We observed 4 primary transits of WA…

quant-ph202139 cited

Controlling long ion strings for quantum simulation and precision measurements

Florian Kranzl, Manoj K. Joshi, Christine Maier +4

Scaling a trapped-ion based quantum simulator to a large number of ions creates a fully-controllable quantum system that becomes inaccessible to numerical methods. When highly anis…

quant-ph202123 cited

Squeezing Quantum Many-Body Scars

Bennet Windt, Hannes Pichler

We develop an analytical approach for the description of quantum many-body scars in PXP models. We show that the scarred dynamics in the PXP model on a complete bipartite graph can…

astro-ph.EP2021

Atmospheric mass loss and stellar wind effects in young and old systems II: Is TOI-942 the past of TOI-421 system?

Daria Kubyshkina, Aline A. Vidotto, Carolina Villarreal D'Angelo +3

The two planetary systems TOI-942 and TOI-421 share many similar characteristics, apart from their ages (50~Myr and 9~Gyr). Each of the stars hosts two sub-Neptune-like planets at…

astro-ph.EP2021

Atmospheric mass loss and stellar wind effects in young and old systems I: comparative 3D study of TOI-942 and TOI-421 systems

Daria Kubyshkina, Aline A. Vidotto, Carolina Villarreal D'Angelo +3

At young ages, when radiation from the host star is high, and the planet is hot and inflated after formation, planetary atmospheric mass loss can be extremely strong compared to ol…