Simulation analysis with rock muons from atmospheric neutrino interactions in the ICAL detector at the India-based Neutrino Observatory

被引:0
|
作者
Kanishka, R. [1 ]
Indumathi, D. [2 ,3 ]
Mohan, Lakshmi S. [4 ]
Bhatnagar, V. [5 ]
机构
[1] Chandigarh Univ, Dept Phys, Gharuan 140413, Mohali, India
[2] Inst Math Sci, CIT Campus, Chennai 600113, India
[3] Homi Bhabha Natl Inst, Training Sch Complex, Anushaktinagar, Mumbai 400094, India
[4] Natl Ctr Nucl Res, 7 Pasteura Str, PL-02093 Warsaw, Poland
[5] Panjab Univ, Phys Dept, Sect 14, Chandigarh 160014, India
来源
EUROPEAN PHYSICAL JOURNAL C | 2023年 / 83卷 / 11期
关键词
FLUX; OSCILLATION; MODEL;
D O I
10.1140/epjc/s10052-023-12133-2
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
The proposed magnetized Iron CALorimeter detector (ICAL) to be built in the India-based Neutrino Observatory (INO) laboratory aims to study atmospheric neutrinos and its properties such as precision measurements of oscillation parameters and the neutrino mass hierarchy. High energy charged current (CC) interactions of atmospheric neutrinos with the rock surrounding the detector produce so-called "rock muons" along with hadrons. While the hadron component of these events are absorbed in the rock itself, the rock muons traverse the rock and are detected in the detector. These rock muon events can be distinguished from cosmic muons only in the upward direction and can provide an independent measurement of the oscillation parameters. A simulation study of these events at the ICAL detector shows that, although reduced in significance compared to muons produced in direct CC neutrino interactions with the detector, these events are indeed sensitive to the oscillation parameters, achieving a possible 1 sigma precision of 10% and 27% in determining Delta m(32)(2) and sin(2)theta(23), respectively. Hence a combination of the standard atmospheric neutrino analysis which is the main goal of ICAL, with these rock muon events, will improve the precision reach of ICAL for these parameters.
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页数:23
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