Fighting Newtonian Noise with Gradient-Based Optimization at the Einstein Telescope
Patrick Schillings, Johannes Erdmann

TL;DR
This paper introduces a gradient-based optimization method to determine optimal seismometer placements around the Einstein Telescope to mitigate Newtonian noise, outperforming traditional metaheuristics in efficiency and effectiveness.
Contribution
It reformulates the seismometer placement problem as a differentiable optimization, enabling efficient gradient-based solutions for Newtonian noise reduction in gravitational wave detectors.
Findings
Gradient-based optimization matches metaheuristics for small seismometer arrays.
It outperforms metaheuristics in larger arrays by a factor of 2.25 in noise reduction.
Gradient methods are more computationally efficient than metaheuristics.
Abstract
Newtonian noise in gravitational wave detectors originates from density fluctuations in the adjacency of the interferometer mirrors. At the Einstein Telescope, this noise source is expected to be dominant for low frequencies. Its impact is proposed to be reduced with the help of an array of seismometers that will be placed around the interferometer endpoints. We reformulate and implement the problem of finding the optimal seismometer positions in a differentiable way. We then explore the use of first-order gradient-based optimization for the design of the seismometer array for 1 Hz and 10 Hz and compare its performance and computational cost to two metaheuristic algorithms. For 1 Hz, we introduce a constraint term to prevent unphysical optimization results in the gradient-based method. In general, we find that it is an efficient strategy to initialize the gradient-based optimizer with a…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Adaptive optics and wavefront sensing · Cosmology and Gravitation Theories
