Detection of Black Holes
Difference from Background: Limit of Detection
The Principle of Superposition and the Gravitational Field
Space-Time Curvature and the General Theory of Relativity
Standing Electromagnetic Waves
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The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
Published on: August 12, 2013
Haowen Zhong1, Luca Reali2, Bei Zhou3,4
1University of Minnesota, School of Physics and Astronomy, Minneapolis, Minnesota 55455, USA.
Detecting primordial gravitational waves requires advanced methods to overcome astrophysical noise. This study introduces a novel framework to isolate cosmological signals from binary black hole and neutron star mergers using next-generation detectors.
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