Enhancing Events in Neutrino Telescopes through Deep Learning-Driven Super-Resolution
- URL: http://arxiv.org/abs/2408.08474v1
- Date: Fri, 16 Aug 2024 01:20:27 GMT
- Title: Enhancing Events in Neutrino Telescopes through Deep Learning-Driven Super-Resolution
- Authors: Felix J. Yu, Nicholas Kamp, Carlos A. Argüelles,
- Abstract summary: We propose a novel technique that learns photon transport through the detector medium through the use of deep learning-driven super-resolution of data events.
Our strategy arranges additional virtual'' optical modules within an existing detector geometry and trains a convolutional neural network to predict the hits on these virtual optical modules.
- Score: 0.0
- License: http://creativecommons.org/licenses/by/4.0/
- Abstract: Recent discoveries by neutrino telescopes, such as the IceCube Neutrino Observatory, relied extensively on machine learning (ML) tools to infer physical quantities from the raw photon hits detected. Neutrino telescope reconstruction algorithms are limited by the sparse sampling of photons by the optical modules due to the relatively large spacing ($10-100\,{\rm m})$ between them. In this letter, we propose a novel technique that learns photon transport through the detector medium through the use of deep learning-driven super-resolution of data events. These ``improved'' events can then be reconstructed using traditional or ML techniques, resulting in improved resolution. Our strategy arranges additional ``virtual'' optical modules within an existing detector geometry and trains a convolutional neural network to predict the hits on these virtual optical modules. We show that this technique improves the angular reconstruction of muons in a generic ice-based neutrino telescope. Our results readily extend to water-based neutrino telescopes and other event morphologies.
Related papers
- Learning Efficient Representations of Neutrino Telescope Events [0.0]
Neutrino telescopes detect rare interactions of particles produced in some of the most extreme environments in the Universe.
Given their size and the high frequency of background interactions, these telescopes amass an enormous quantity of large variance, high-dimensional data.
We present a novel approach, called om2vec, that employs transformer-based variational autoencoders to efficiently represent neutrino telescope events by learning compact and latent representations.
arXiv Detail & Related papers (2024-10-17T02:07:54Z) - Preliminary Report on Mantis Shrimp: a Multi-Survey Computer Vision
Photometric Redshift Model [0.431625343223275]
Photometric redshift estimation is a well-established subfield of astronomy.
Mantis Shrimp is a computer vision model for photometric redshift estimation that fuses ultra-violet (GALEX), optical (PanSTARRS), and infrared (UnWISE) imagery.
arXiv Detail & Related papers (2024-02-05T21:44:19Z) - Trigger-Level Event Reconstruction for Neutrino Telescopes Using Sparse
Submanifold Convolutional Neural Networks [0.0]
Convolutional neural networks (CNNs) have seen extensive applications in scientific data analysis, including in neutrino telescopes.
We propose sparse submanifold convolutions (SSCNNs) as a solution to these issues.
We show that the SSCNN event reconstruction performance is comparable to or better than traditional and machine learning algorithms.
arXiv Detail & Related papers (2023-03-15T17:59:01Z) - Interpretable Joint Event-Particle Reconstruction for Neutrino Physics
at NOvA with Sparse CNNs and Transformers [124.29621071934693]
We present a novel neural network architecture that combines the spatial learning enabled by convolutions with the contextual learning enabled by attention.
TransformerCVN simultaneously classifies each event and reconstructs every individual particle's identity.
This architecture enables us to perform several interpretability studies which provide insights into the network's predictions.
arXiv Detail & Related papers (2023-03-10T20:36:23Z) - Supernova Light Curves Approximation based on Neural Network Models [53.180678723280145]
Photometric data-driven classification of supernovae becomes a challenge due to the appearance of real-time processing of big data in astronomy.
Recent studies have demonstrated the superior quality of solutions based on various machine learning models.
We study the application of multilayer perceptron (MLP), bayesian neural network (BNN), and normalizing flows (NF) to approximate observations for a single light curve.
arXiv Detail & Related papers (2022-06-27T13:46:51Z) - Processing Images from Multiple IACTs in the TAIGA Experiment with
Convolutional Neural Networks [62.997667081978825]
We use convolutional neural networks (CNNs) to analyze Monte Carlo-simulated images from the TAIGA experiment.
The analysis includes selection of the images corresponding to the showers caused by gamma rays and estimating the energy of the gamma rays.
arXiv Detail & Related papers (2021-12-31T10:49:11Z) - Deep learning with photosensor timing information as a background
rejection method for the Cherenkov Telescope Array [0.0]
New deep learning techniques present promising new analysis methods for Imaging Atmospheric Cherenkov Telescopes (IACTs)
CNNs could provide a direct event classification method that uses the entire information contained within the Cherenkov shower image.
arXiv Detail & Related papers (2021-03-10T13:54:43Z) - Rapid characterisation of linear-optical networks via PhaseLift [51.03305009278831]
Integrated photonics offers great phase-stability and can rely on the large scale manufacturability provided by the semiconductor industry.
New devices, based on such optical circuits, hold the promise of faster and energy-efficient computations in machine learning applications.
We present a novel technique to reconstruct the transfer matrix of linear optical networks.
arXiv Detail & Related papers (2020-10-01T16:04:22Z) - Spatial Mode Correction of Single Photons using Machine Learning [1.8086378019947618]
We exploit the self-learning and self-evolving features of artificial neural networks to correct the complex spatial profile of distorted Laguerre-Gaussian modes at the single-photon level.
Our results have important implications for real-time turbulence correction of structured photons and single-photon images.
arXiv Detail & Related papers (2020-06-14T01:25:17Z) - Quantum metamaterial for nondestructive microwave photon counting [52.77024349608834]
We introduce a single-photon detector design operating in the microwave domain based on a weakly nonlinear metamaterial.
We show that the single-photon detection fidelity increases with the length of the metamaterial to approach one at experimentally realistic lengths.
In stark contrast to conventional photon detectors operating in the optical domain, the photon is not destroyed by the detection and the photon wavepacket is minimally disturbed.
arXiv Detail & Related papers (2020-05-13T18:00:03Z) - Deep Photon Mapping [59.41146655216394]
In this paper, we develop the first deep learning-based method for particle-based rendering.
We train a novel deep neural network to predict a kernel function to aggregate photon contributions at shading points.
Our network encodes individual photons into per-photon features, aggregates them in the neighborhood of a shading point, and infers a kernel function from the per-photon and photon local context features.
arXiv Detail & Related papers (2020-04-25T06:59:10Z)
This list is automatically generated from the titles and abstracts of the papers in this site.
This site does not guarantee the quality of this site (including all information) and is not responsible for any consequences.