Observational cosmology with Artificial Neural Networks
arXiv:2112.12645 · doi:10.3390/universe8020120
Abstract
In cosmology, the analysis of observational evidence is very important to test theoretical models of the Universe. Artificial neural networks are powerful and versatile computational tools for data modelling and are recently being considered in the analysis of cosmological data. The main goal of this paper is to provide an introduction to artificial neural networks and to describe some applications to cosmology. We present an overview on the fundamentals of neural networks and their technical details. Throughout three examples, we show their capabilities in modelling cosmological data, saving computational time in numerical tasks, and classifying stellar objects. Artificial neural networks offer interesting qualities that make them a viable alternative method for data analysis in cosmological research.
arXiv comment17 pages, 13 figures; matches the version published in Universe
References in corpus (24)
- Artificial Neural Networks for Solving Ordinary and Partial Differential Equations
- Rotation-invariant convolutional neural networks for galaxy morphology prediction
- Why does deep and cheap learning work so well?
- Real-time gravitational-wave science with neural posterior estimation
- Fast likelihood-free cosmology with neural density estimators and active learning
- Learning to Predict the Cosmological Structure Formation
- Neural networks and separation of Cosmic Microwave Background and astrophysical signals in sky maps
- A deep learning approach to cosmological dark energy models
- Fast cosmic web simulations with generative adversarial networks
- A Deep Learning Approach to Galaxy Cluster X-ray Masses
- Fast cosmological parameter estimation using neural networks
- What can Machine Learning tell us about the background expansion of the Universe?
- Distinguishing standard and modified gravity cosmologies with machine learning
- Deep learning Approach for Classifying, Detecting and Predicting Photometric Redshifts of Quasars in the Sloan Digital Sky Survey Stripe 82
- Cosmological parameter inference with Bayesian statistics
- Neural Network Reconstruction of Late-Time Cosmology and Null Tests
- Testing the Mutual Consistency of the Pantheon and SDSS/eBOSS BAO Data Sets with Gaussian Processes
- The GCE in a New Light: Disentangling the -ray Sky with Bayesian Graph Convolutional Neural Networks
- Full-sky Cosmic Microwave Background Foreground Cleaning Using Machine Learning
- Machine Learning the Cosmic Curvature in a Model-independent Way
- Accelerated Bayesian inference using deep learning
- Bayesian model selection on Scalar -Field Dark Energy
- Self-interacting Scalar Field Trapped in a Randall-Sundrum Braneworld: The Dynamical Systems Perspective
- Classification algorithms applied to structure formation simulations
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- Reconstruction of full sky CMB and modes spectra removing -to- leakage from partial sky using deep learning
- In Search of Global 21-cm Signal using Artificial Neural Network in light of ARCADE 2
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