Strong lensing of high-energy neutrinos

被引：2
作者：
Taak, Yoon Chan [1 ]
Treu, Tommaso [1 ]
Inoue, Yoshiyuki [2 ,3 ,4 ]
Kusenko, Alexander [1 ,4 ,5 ]
机构：
[1] Univ Calif Los Angeles, Phys & Astron Dept, Los Angeles, CA 90095 USA
[2] Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, 1-1 Machikaneyama, Toyonaka, Osaka 5600043, Japan
[3] RIKEN, Interdisciplinary Theoret & Math Sci Program iTHE, 2-1 Hirosawa, Saitama 3510198, Japan
[4] Univ Tokyo, Inst Adv Study, Kavli Inst Phys & Math Universe WPI, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan
[5] CERN, Theoret Phys Dept, CH-1211 Geneva 23, Switzerland
来源：
PHYSICAL REVIEW D | 2023年 / 107卷 / 02期
基金：
日本学术振兴会; 新加坡国家研究基金会;
关键词：
MASS; GALAXY; AGN;
D O I：
10.1103/PhysRevD.107.023011
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We consider the effects of strong gravitational lensing by galaxy-scale deflectors on the observations of multiple imaging is similar to 10-3, implying that while we do not expect any multiply imaged HENs with present samples, next-generation experiments should be able to detect the first such event. We then present the distribution of expected time delays to aid in the identification of such events, in combination with directional and energy information. In order to assist in the evaluation of HEN production mechanisms, we illustrate how lensing affects the observed number counts for a variety of intrinsic luminosity functions of the source population. Finally, we see that the lensing effects on the cosmic neutrino background flux calculation would be negligible by taking kiloparsec-scale jets as an example.
引用
收藏
页数：9
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