Hadron energy estimation from atmospheric neutrino events

Abstract

The iron calorimeter (ICAL) at India-based neutrino observatory (INO) is designed to mainly observe the muons produced in the charged current interactions of atmospheric muon neutrinos and antineutrinos. The track of the muon is reconstructed using the hits they produce in the detector. From this track, the charge, the energy and the direction of the muon are estimated, which are used to do oscillation physics analysis. In a large fraction of events, a number of hadrons are also produced in addition to the muons. The charged hadrons also leave hits in the detector which can be utilised to estimate the hadron energy. In this work, we generate atmospheric neutrino events using two different neutrino event generators: NUANCE and GENIE. The generated events are passed through the Geant4 simulator of ICAL. In each case, we study the relation between hadron hits, defined to be the difference between the total number of hits and the muon track hits, and the hadron energy. We find that a non-negligible number of baryons are produced in atmospheric neutrino interactions. For \({E}_\mathrm{had} < 5\) GeV, almost all the hadron energy is carried by these baryons. Finally, we formulate a procedure by which the hadron energy can be estimated from the number of hadron hits.

This is a preview of subscription content, access via your institution.

Fig. 1
Fig. 2
Fig. 3
Fig. 4
Fig. 5
Fig. 6
Fig. 7
Fig. 8
Fig. 9
Fig. 10
Fig. 11
Fig. 12

References

  1. 1.

    S Ahmad et al, Pramana – J. Phys. 88: 79 (2017)

    ADS  Article  Google Scholar 

  2. 2.

    A Ajmi et al, Improving the hierarchy sensitivity of ICAL using neural network, arxiv:1510.02350 [physics.ins-det]

  3. 3.

    T Thakore et al, J. High Energy Phys. 05, 058 (2013)

    ADS  Article  Google Scholar 

  4. 4.

    A Ghosh et al, J. High Energy Phys. 04, 009 (2013)

    ADS  Article  Google Scholar 

  5. 5.

    M M Devi et al, J. Instrum. 08, P11003 (2013)

    Article  Google Scholar 

  6. 6.

    S Seth et al, J. Instrum. 13, P09015 (2018)

    Article  Google Scholar 

  7. 7.

    L S Mohan et al, J. Instrum. 9, T09003 (2014)

    Article  Google Scholar 

  8. 8.

    M M Devi et al, J. High Energy Phys. 2014, 189 (2014)

    ADS  Article  Google Scholar 

  9. 9.

    T Thakore, Physics potential of the India-based neutrino observatory (INO), Ph.D. thesis (DHEP, TIFR, Mumbai 2014)

  10. 10.

    D Casper, Nucl. Phys. B - Proc. Suppl. 112, 161 (2002)

    ADS  Article  Google Scholar 

  11. 11.

    C Andreopoulos et al, Nucl. Instrum. Methods A 614, 87 (2010)

    ADS  Article  Google Scholar 

  12. 12.

    P V Vavilov, Sov. Phys. JETP 5, 749 (1957)

    Google Scholar 

Download references

Acknowledgements

The authors would like to thank Dr Ali Ajmi who provided valuable help in the initial stages of this work. They also thank Prof. Gobinda Majumder, Dr Susanta Seth, Prof. Prafulla Behera and Dr Jafar Sadiq for discussions at different times. Thanks are also due to Prof. Raj Gandhi and Prof. Amol Dighe who gave valuable feedback at various intermediate stages. Funding was provided by Department of Atomic Energy (IN).

Author information

Affiliations

Authors

Corresponding author

Correspondence to M Nizam.

Rights and permissions

Reprints and Permissions

About this article

Verify currency and authenticity via CrossMark

Cite this article

Nizam, M., Sankar, S.U. Hadron energy estimation from atmospheric neutrino events. Pramana - J Phys 94, 118 (2020). https://doi.org/10.1007/s12043-020-01986-x

Download citation

Keywords

  • Atmospheric neutrinos
  • energy of hadrons
  • energy of baryons

PACS Nos

  • 13.15.+g
  • 95.55.Vj