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Precision Interferometry in a New Shape - Higher-order Laguerre-Gauss Modes for Gravitational Wave Detection (Hardcover, 2014 ed.)
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Precision Interferometry in a New Shape - Higher-order Laguerre-Gauss Modes for Gravitational Wave Detection (Hardcover, 2014 ed.)
Series: Springer Theses
Expected to ship within 12 - 17 working days
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With his Ph.D. thesis, presented here in the format of a "Springer
Theses", Paul Fulda won the 2012 GWIC thesis prize awarded by the
Gravitational Wave International Committee. The impact of thermal
noise on future gravitational wave detectors depends on the size
and shape of the interrogating laser beam. It had been known since
2006 that, in theory, higher-order Laguerre-Gauss modes could
reduce thermal noise. Paul Fulda's research brings Laguerre-Gauss
modes an enormous step forward. His work includes analytical,
numerical and experimental work on table-top setups as well as
experiments at the Glasgow 10m prototype interferometer. Using
numerical simulations the LG33 mode was selected as the optical
mode to be tested. Further research by Paul and his colleagues
since then concentrated on this mode. Paul has developed and
demonstrated simple and effective methods to create this mode with
diffractive optics and successfully demonstrated its compatibility
with the essential building blocks of gravitational wave detectors,
namely, optical cavities, Michelson interferometers and
opto-electronic sensing and control systems. Through this work,
Laguerre-Gauss modes for interferometers have been transformed from
an essentially unknown entity to a well understood option with an
experimental basis.
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