This code is a basic computer implementation of the quadrupole formalism of general relativity applied to point-mass binary systems in circular orbits.
The code was written with the aim to efficiently generate large amounts of parameter-dependent gravitational waveform time-series used for the incipient development of neural networks dedicated to the detection and classification of gravitational waves. The variable source parameters considered are the binary mass ratio, orbital inclination, distance to source and antenna pattern coefficients. The generated gravitational waveforms are either "clean" or distorted with adjustable additive random noise.
Besides gravitational waveforms, the code also computes the parameter-dependent time-evolution of the main physical quantities in the quadrupole formalism (orbital separation, gravitational waves frequency, amplitude and phase).
An updated version of the code, with enhanced functionalities, will soon be available on MathWorks File Exchange.
引用格式
Developed by Traian Popescu for the LISA ISS-Sci team.
MATLAB 版本兼容性
创建方式
R2022a
兼容任何版本
平台兼容性
Windows macOS Linux标签
Community Treasure Hunt
Find the treasures in MATLAB Central and discover how the community can help you!
Start Hunting!