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Quantum Hypothesis Testing for Exoplanet Detection
Physical Review Letters ( IF 8.1 ) Pub Date : 2021-09-23 , DOI: 10.1103/physrevlett.127.130502
Zixin Huang 1, 2 , Cosmo Lupo 2
Affiliation  

Detecting the faint emission of a secondary source in the proximity of the much brighter one has been the most severe obstacle for using direct imaging in searching for exoplanets. Using quantum state discrimination and quantum imaging techniques, we show that one can significantly reduce the probability of error for detecting the presence of a weak secondary source, especially when the two sources have small angular separations. If the weak source has intensity ε1 relative to the bright source, we find that the error exponent can be improved by a factor of 1/ε. We also find linear-optical measurements that are optimal in this regime. Our result serves as a complementary method in the toolbox of optical imaging, with applications ranging from astronomy to microscopy.

中文翻译:

用于系外行星探测的量子假设检验

在更亮的源附近检测到次要源的微弱发射一直是使用直接成像寻找系外行星的最严重障碍。使用量子态判别和量子成像技术,我们表明可以显着降低检测弱二次源存在的错误概率,尤其是当两个源具有小角度间隔时。如果弱源有强度ε1 相对于亮光源,我们发现误差指数可以提高一个因子 1/ε. 我们还发现在这种情况下最佳的线性光学测量。我们的结果作为光学成像工具箱中的一种补充方法,应用范围从天文学到显微镜。
更新日期:2021-09-23
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