MARATTO

article · The European Physical Journal C

Measurement of the atmospheric $$\nu _{\mu }$$ flux with six detection units of KM3NeT/ORCA

2025Open accessMohamed I University

Abstract

Abstract A measurement of the atmospheric $$\nu _{\mu }+\bar{\nu }_{\mu }$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>ν</mml:mi> <mml:mi>μ</mml:mi> </mml:msub> <mml:mo>+</mml:mo> <mml:msub> <mml:mover> <mml:mrow> <mml:mi>ν</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>¯</mml:mo> </mml:mrow> </mml:mover> <mml:mi>μ</mml:mi> </mml:msub> </mml:mrow> </mml:math> flux with energies between 1 and 100 GeV is presented. The measurement has been performed using data taken with the first six detection units of the KM3NeT/ORCA detector, referred to as ORCA6. The data were collected between January 2020 and November 2021 and correspond to 510 days of livetime, with a total exposure of 433 kton $$\cdot $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mo>·</mml:mo> </mml:math> years. Using machine learning classification, 3894 neutrino candidate events have been selected with an atmospheric muon contamination of less than 1 $$\%$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mo>%</mml:mo> </mml:math> . The atmospheric $$\nu _{\mu }+\bar{\nu }_{\mu }$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>ν</mml:mi> <mml:mi>μ</mml:mi> </mml:msub> <mml:mo>+</mml:mo> <mml:msub> <mml:mover> <mml:mrow> <mml:mi>ν</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>¯</mml:mo> </mml:mrow> </mml:mover> <mml:mi>μ</mml:mi> </mml:msub> </mml:mrow> </mml:math> energy spectrum is derived using an unfolding procedure and the impact of systematic uncertainties is estimated. The atmospheric $$\nu _{\mu }+\bar{\nu }_{\mu }$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msub> <mml:mi>ν</mml:mi> <mml:mi>μ</mml:mi> </mml:msub> <mml:mo>+</mml:mo> <mml:msub> <mml:mover> <mml:mrow> <mml:mi>ν</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>¯</mml:mo> </mml:mrow> </mml:mover> <mml:mi>μ</mml:mi> </mml:msub> </mml:mrow> </mml:math> flux measured using the ORCA6 configuration is in agreement with the values measured by other experiments.

Research topics

  • Atmospheric Ozone and Climate
  • Astrophysics and Cosmic Phenomena
  • Ionosphere and magnetosphere dynamics

Read the original research

This page summarises published work. The authoritative version sits with the publisher.

DOI: 10.1140/epjc/s10052-025-14513-2

Is something wrong with this record? Report it or request removal.

Discussion

Discuss this research

Have you built on this work, tried to replicate it, or seen it applied in practice? Share what you know. Verified researchers and MARATTO™ domain experts can open a discussion, and any member can reply. Contributions are reviewed before they appear.

No discussion yet. Open the first thread.