Detection of Gravitational Waves Using Bayesian Neural Networks
- URL: http://arxiv.org/abs/2007.04176v2
- Date: Tue, 19 Jan 2021 01:09:15 GMT
- Title: Detection of Gravitational Waves Using Bayesian Neural Networks
- Authors: Yu-Chiung Lin, Jiun-Huei Proty Wu
- Abstract summary: We propose a new model of Bayesian Neural Networks to detect the events of compact binary coalescence in observational data of gravitational waves (GW)
Our model successfully detects all seven BBH events in the LIGO Livingston O2 data, with the periods of their GW waveforms correctly labeled.
This makes our model possible for nearly real-time detection and for forecasting the coalescence events when assisted with deeper training on a larger dataset using the state-of-art HPCs.
- Score: 0.0
- License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
- Abstract: We propose a new model of Bayesian Neural Networks to not only detect the
events of compact binary coalescence in the observational data of gravitational
waves (GW) but also identify the full length of the event duration including
the inspiral stage. This is achieved by incorporating the Bayesian approach
into the CLDNN classifier, which integrates together the Convolutional Neural
Network (CNN) and the Long Short-Term Memory Recurrent Neural Network (LSTM).
Our model successfully detect all seven BBH events in the LIGO Livingston O2
data, with the periods of their GW waveforms correctly labeled. The ability of
a Bayesian approach for uncertainty estimation enables a newly defined
`awareness' state for recognizing the possible presence of signals of unknown
types, which is otherwise rejected in a non-Bayesian model. Such data chunks
labeled with the awareness state can then be further investigated rather than
overlooked. Performance tests with 40,960 training samples against 512 chunks
of 8-second real noise mixed with mock signals of various optimal
signal-to-noise ratio $0 \leq \rho_\text{opt} \leq 18$ show that our model
recognizes 90% of the events when $\rho_\text{opt} >7$ (100% when
$\rho_\text{opt} >8.5$) and successfully labels more than 95% of the waveform
periods when $\rho_\text{opt} >8$. The latency between the arrival of peak
signal and generating an alert with the associated waveform period labeled is
only about 20 seconds for an unoptimized code on a moderate GPU-equipped
personal computer. This makes our model possible for nearly real-time detection
and for forecasting the coalescence events when assisted with deeper training
on a larger dataset using the state-of-art HPCs.
Related papers
- Continuous time recurrent neural networks: overview and application to
forecasting blood glucose in the intensive care unit [56.801856519460465]
Continuous time autoregressive recurrent neural networks (CTRNNs) are a deep learning model that account for irregular observations.
We demonstrate the application of these models to probabilistic forecasting of blood glucose in a critical care setting.
arXiv Detail & Related papers (2023-04-14T09:39:06Z) - LSTM and CNN application for core-collapse supernova search in
gravitational wave real data [0.0]
Core-collapse supernovae (CCSNe) are expected to emit gravitational wave signals that could be detected by interferometers within the Milky Way and nearby galaxies.
We show potential of machine learning (ML) for multi-label classification of different CCSNe simulated signals and noise transients using real data.
arXiv Detail & Related papers (2023-01-23T12:12:33Z) - A quantum algorithm for training wide and deep classical neural networks [72.2614468437919]
We show that conditions amenable to classical trainability via gradient descent coincide with those necessary for efficiently solving quantum linear systems.
We numerically demonstrate that the MNIST image dataset satisfies such conditions.
We provide empirical evidence for $O(log n)$ training of a convolutional neural network with pooling.
arXiv Detail & Related papers (2021-07-19T23:41:03Z) - Real-time gravitational-wave science with neural posterior estimation [64.67121167063696]
We demonstrate unprecedented accuracy for rapid gravitational-wave parameter estimation with deep learning.
We analyze eight gravitational-wave events from the first LIGO-Virgo Gravitational-Wave Transient Catalog.
We find very close quantitative agreement with standard inference codes, but with inference times reduced from O(day) to a minute per event.
arXiv Detail & Related papers (2021-06-23T18:00:05Z) - Training Strategies for Deep Learning Gravitational-Wave Searches [43.55994393060723]
We restrict our analysis to signals from non-spinning binary black holes.
We systematically test different strategies by which training data is presented to the networks.
We find that the deep learning algorithms can generalize low signal-to-noise ratio (SNR) signals to high SNR ones but not vice versa.
arXiv Detail & Related papers (2021-06-07T16:04:29Z) - Towards a method to anticipate dark matter signals with deep learning at
the LHC [58.720142291102135]
We study several simplified dark matter (DM) models and their signatures at the LHC using neural networks.
We focus on the usual monojet plus missing transverse energy channel, but to train the algorithms we organize the data in 2D histograms instead of event-by-event arrays.
This results in a large performance boost to distinguish between standard model (SM) only and SM plus new physics signals.
arXiv Detail & Related papers (2021-05-25T15:38:13Z) - Convolutional Neural Networks for Sleep Stage Scoring on a Two-Channel
EEG Signal [63.18666008322476]
Sleep problems are one of the major diseases all over the world.
Basic tool used by specialists is the Polysomnogram, which is a collection of different signals recorded during sleep.
Specialists have to score the different signals according to one of the standard guidelines.
arXiv Detail & Related papers (2021-03-30T09:59:56Z) - Deep learning for gravitational-wave data analysis: A resampling
white-box approach [62.997667081978825]
We apply Convolutional Neural Networks (CNNs) to detect gravitational wave (GW) signals of compact binary coalescences, using single-interferometer data from LIGO detectors.
CNNs were quite precise to detect noise but not sensitive enough to recall GW signals, meaning that CNNs are better for noise reduction than generation of GW triggers.
arXiv Detail & Related papers (2020-09-09T03:28:57Z) - Complete parameter inference for GW150914 using deep learning [0.0]
LIGO and Virgo gravitational-wave observatories have detected many exciting events over the past five years.
As the rate of detections grows with detector sensitivity, this poses a growing computational challenge for data analysis.
We apply deep learning techniques to perform fast likelihood-free Bayesian inference for gravitational waves.
arXiv Detail & Related papers (2020-08-07T18:00:02Z)
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.