在皮埃尔·奥格天文台寻找超高能量光子

T. P. A. C. P. Abreu, M. Aglietta, I. Allekotte, K. A. Cheminant, A. Almela, J. Alvarez-Muñiz, J. A. Yebra, G. A. Anastasi, L. Anchordoqui, B. Andrada, S. Andringa, C. Aramo, P. Ferreira, E. Arnone, J. C. A. Vel'azquez, Hernán Asorey, P. Assis, G. Avila, E. Avocone, A. Badescu, A. Bakalová, A. Bălăceanu, F. Barbato, J. Bellido, C. Bérat, M. Bertaina, G. Bhatta, P. Biermann, V. Binet, K. Bismark, T. Bister, J. Biteau, J. Blazek, C. Bleve, J. Blumer, M. Boh'avcov'a, D. Boncioli, C. Bonifazi, L. Arbeletche, N. Borodai, J. Brack, T. Bretz, P. G. B. Orchera, F. Briechle, P. Buchholz, A. Bueno, S. Buitink, M. Buscemi, M. Busken, A. Bwembya, K. Caballero-Mora, L. Caccianiga, I. Caracas, R. Caruso, A. Castellina, F. Catalani, G. Cataldi, L. Cazon, M. Cerda, J. Chinellato, J. Chudoba, L. Chytka, R. Clay, A. Cerutti, R. Colalillo, A. Coleman, M. Coluccia, R. Conceiccao, A. Condorelli, G. Consolati, F. Contreras, F. Convenga, D. D. Santos, C. Covault, M. Cristinziani, S. Dasso, K. Daumiller, B. Dawson, R. M. Almeida
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引用次数: 6

摘要

天体粒子物理学的关键挑战之一是确定最高能量(高于10^18电子伏特)的宇宙射线的来源。在这种情况下,寻找超高能量光子是非常有趣的。观测这种能量的光子将影响天体物理学和粒子物理学以及基础物理学,并将对多信使天文学作出重要贡献。位于阿根廷马拉格附近的皮埃尔·奥格天文台是最大的用于探测超高能量宇宙射线的气阵雨实验。它由大约1660个水切伦科夫探测器组成,排列在一个三角形网格上,覆盖面积超过3000平方公里。在四个地点的27个荧光望远镜俯瞰探测器阵列,为气淋探测提供了一种独立和互补的方法。在论文中,将介绍皮埃尔·奥格天文台在寻找超高能量光子方面的各种活动,并对目前的结果进行总结。
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Searches for ultra-high-energy photons at the Pierre Auger Observatory
One of the key challenges in astroparticle physics is identifying the sources of cosmic rays at the highest energies (above 10^18 eV). In this context, the search for ultra-high energy photons is of high interest. Observing photons of such energies would impact astrophysics and particle physics as well as fundamental physics and would be an important contribution to multimessenger astronomy. The Pierre Auger Observatory near Malargue, Argentina, is the largest air-shower experiment for the detection of ultra-high energy cosmic rays. It consists of an array of about 1660 water Cherenkov detectors arranged on a triangular grid which covers an area of more than 3000 km^2. 27 fluorescence telescopes at four sites overlooking the detector array provide an independent and complementary method for air-shower detection. In the contribution, the various activities at the Pierre Auger Observatory concerning searches for ultra-high energy photons will be presented and the current results will be summarized.
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