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29 November 2021 to 3 December 2021
Virtual and IBS Science Culture Center, Daejeon, South Korea
Asia/Seoul timezone

Identifying mass composition of ultra high energy cosmic rays using deep learning

contribution ID 553
Not scheduled
20m
Apple (Gather.Town)

Apple

Gather.Town

Poster Track 2: Data Analysis - Algorithms and Tools Posters: Apple

Speaker

Ivan Kharuk (INR RAS)

Description

We introduce a novel method for identifying fractions of primary air shower particles in an ensemble of events using deep learning. The suggested approach is developed for the Monte-Carlo simulated data for the Telescope Array experiment. For a given hadronic model, the error of identifying individual fractions of primary particles in an ensemble is less than 7%. We show that the developed method is sensitive to the underlying hadronic model and study the corresponding systematic error.

References

https://www.youtube.com/watch?v=MLnLlDe8OYA&list=PLQKlHTdtNqvifTuKIFnEM1IdMMN_9pfrx&index=5
and soon paper on arXiv.

Significance

In many physical experiments detectors readings are subject to high variance. This fact complicates the usage of standard machine learning techniques as they yield low accuracy under such conditions. We show how one can overcome this problem on the example of Telescope Array data. The main ingredients of the method are: 1) switching to predictions for an ensemble of events and 2) using the chain of two neural networks, one for individual events and one for ensembles of events, to get best accuracy.

Speaker time zone Compatible with Europe

Primary authors

Grigory Rubtsov (Institute for Nuclear Research of Russina Academy of Scinces) Ivan Kharuk (INR RAS) Mikhail Kuznetsov (Service de Physique Theorique, Universite Libre de Bruxelles)

Presentation materials