Linear Approximation in Time Domain
Area Computation by the Alternative Coordinate Method
Rectangular and Triangular Pulse Function
Convolution Properties I
Fast Fourier Transform
Linear Approximation in Frequency Domain
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An Experimental Protocol for Femtosecond NIR/UV - XUV Pump-Probe Experiments with Free-Electron Lasers
Published on: October 23, 2018
Neha Anil Kumar1, Marc Kamionkowski1
1William H. Miller III Department of Physics and Astronomy, <a href="https://ror.org/00za53h95">Johns Hopkins University</a>, 3400 North Charles Street, Baltimore, Maryland 21218, USA.
Pulsar timing arrays detect gravitational waves (GWs) using correlation functions. This study presents a general formula for these functions, accounting for arbitrary polarization and anisotropy in GW backgrounds.
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