Demonstrating the ability of IceCube DeepCore to probe Earth's interior with atmospheric neutrino oscillations
Sharmistha Chattopadhyay, Krishnamoorthi J, Anuj Kumar Upadhyay (For the IceCube Collaboration)

TL;DR
This paper shows how IceCube DeepCore can use atmospheric neutrino oscillations to investigate Earth's internal structure, including density distribution and mass, by analyzing 9.3 years of simulated data.
Contribution
It demonstrates the potential of IceCube DeepCore to probe Earth's interior through neutrino oscillation measurements, a novel application of neutrino astronomy.
Findings
DeepCore can detect Earth's matter effects on neutrino oscillations.
The study validates the non-homogeneous electron density distribution in Earth.
Potential to measure Earth's mass and layer densities using atmospheric neutrinos.
Abstract
The IceCube Neutrino Observatory is an optical Cherenkov detector instrumenting one cubic kilometer of ice at the South Pole. The Cherenkov photons emitted following a neutrino interaction are detected by digital optical modules deployed along vertical strings within the ice. The densely instrumented bottom central region of the IceCube detector, known as DeepCore, is optimized to detect GeV-scale atmospheric neutrinos. As upward-going atmospheric neutrinos pass through Earth, matter effects alter their oscillation probabilities due to coherent forward scattering with ambient electrons. These matter effects depend upon the energy of neutrinos and the density distribution of electrons they encounter during their propagation. Using simulated data at the IceCube Deepcore equivalent to its 9.3 years of observation, we demonstrate that atmospheric neutrinos can be used to probe the broad…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
