Detection of Black Holes
Schwarzschild Radius and Event Horizon
Space-Time Curvature and the General Theory of Relativity
The Principle of Superposition and the Gravitational Field
Gravitation Between Spherically Symmetric Masses
Gravitational Potential Energy for Extended Objects
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The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
Published on: August 12, 2013
Liu Tao1, Mohak Bhattacharya1, Peter Carney1
1University of California, Riverside, Department of Physics & Astronomy, Riverside, California 92521 USA.
New adaptive optics technology enhances gravitational-wave observatories by reducing noise and increasing detection range. This advancement improves sensitivity to spacetime strain, enabling observations of distant cosmic events.
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