Detecting High-Energy Neutrinos from Galactic Supernovae with ATLAS

被引:1
|
作者
Wen, Alex Y. [1 ,2 ]
Arguelles, Carlos A. [1 ,2 ]
Kheirandish, Ali [3 ,4 ]
Murase, Kohta [5 ,6 ,7 ,8 ]
机构
[1] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
[2] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA
[3] Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
[4] Univ Nevada, Nevada Ctr Astrophys, Las Vegas, NV 89154 USA
[5] Penn State Univ, Inst Gravitat & Cosmos, Dept Phys, Dept Astron & Astrophys, University Pk, PA 16802 USA
[6] Penn State Univ, Inst Gravitat & Cosmos, Ctr Multimessenger Astrophys, University Pk, PA 16802 USA
[7] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA
[8] Kyoto Univ, Ctr Gravitat Phys & Quantum Informat, Yukawa Inst Theoret Phys, Kyoto 16802, Japan
基金
加拿大自然科学与工程研究理事会; 美国国家科学基金会;
关键词
MUON RECONSTRUCTION; COLLISION DATA; GAMMA-RAY; PROGENITORS; PERFORMANCE; EVOLUTION; ERUPTION; ICECUBE; SEARCH; BURST;
D O I
10.1103/PhysRevLett.132.061001
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We show that ATLAS, a collider detector, can measure the flux of high-energy supernova neutrinos, which can be produced from days to months after the explosion. Using Monte Carlo simulations for predicted fluxes, we find at most O(0.1-1) starting events and O(10-100) throughgoing events from a supernova 10 kpc away. Possible Galactic supernovae from Betelgeuse and Eta Carinae are further analyzed as demonstrative examples. We argue that, even with limited statistics, ATLAS has the ability to discriminate among flavors and between neutrinos and antineutrinos, making it a unique neutrino observatory so far unmatched in this capability.
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收藏
页数:8
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