面向 Mini-EUSO 中核子态的观测
高能天体物理现象
2022-01-05 v1 天体物理仪器与方法
高能物理 - 实验
摘要
Mini-EUSO 是一台小型轨道望远镜，视场为 ，主要在 320–420 nm 波段观测夜间地球。其时间分辨率从微秒（触发）到毫秒（未触发）不等，覆盖地面超过 km，已使其记录到数千颗流星。此类探测使该望远镜成为搜寻假想重致密物体的合适工具，后者会因高密度和高速在大气中留下光迹。最典型的例子是核子态（nuclearites）——假想的奇异夸克物质团块，可能比核物质更稳定、更致密。本文中，我们给出了基于 42 小时观测数据得到的核子态通量潜在限制。
引用
@article{arxiv.2201.01114,
title = {Towards observations of nuclearites in Mini-EUSO},
author = {L. W. Piotrowski and D. Barghini and M. Battisti and A. Belov and M. Bertaina and F. Bisconti and C. Blaksley and K. Bolmgren and F. Cafagna and G. Cambiè and F. Capel and M. Casolino and T. Ebisuzaki and F. Fenu and A. Franceschi and C. Fuglesang and A. Golzio and P. Gorodetzki and F. Kajino and H. Kasuga and P. Klimov and V. Kungel and M. Manfrin and L. Marcelli and W. Marszał and H. Miyamoto and M. Mignone and T. Napolitano and G. Osteria and E. Parizot and P. Picozza and Z. Plebaniak and G. Prévôt and E. Reali and M. Ricci and N. Sakaki and K. Shinozaki and J. Szabelski and Y. Takizawa and S. Wada and L. Wiencke},
journal= {arXiv preprint arXiv:2201.01114},
year = {2022}
}
备注
To be published in the Proceedings of the 37th International Cosmic Ray Conference (ICRC 2021), Berlin, 12 -23 July 2021