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Broadband Quantum Noise Reduction in Advanced Virgo Plus - Eleonora Polini

Broadband Quantum Noise Reduction in Advanced Virgo Plus

From Frequency-Dependent Squeezing Implementation to Detection Losses and Stray Light Mitigation

(Autor)

Buch | Hardcover
XXI, 248 Seiten
2025
Springer International Publishing (Verlag)
978-3-031-95142-8 (ISBN)
CHF 224,65 inkl. MwSt
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This book presents the first implementation of frequency-dependent squeezing in the Virgo gravitational wave detector, a technique that reduces quantum noise across the entire detection band. By lowering noise, it enhances Virgo's ability to observe the universe.

It provides a detailed account of the experimental optical system-spanning hundreds of meters-and the measurement campaign that led to the first observation of frequency-dependent squeezing, with ellipse rotation occurring at the target frequency of a few tens of Hz. Additionally, the book covers the characterization and commissioning of a new Output Mode Cleaner cavity in Virgo to minimize optical losses on squeezed states. Finally, it examines the impact of stray light noise at low frequencies and explores mitigation strategies to improve detector sensitivity.

Eleonora Polini is a physicist specializing in quantum noise reduction for gravitational wave detectors. She earned her Bachelor s and Master s degrees in Physics from La Sapienza University of Rome, where she received the Enrico Persico and Tito Maiani Prizes for academic excellence.

She completed her PhD at the Laboratoire d Annecy de Physique des Particules and Université Savoie Mont Blanc, focusing on frequency-dependent squeezing in the Virgo detector. Her work included upgrading the Output Mode Cleaner cavity and investigating stray light noise, earning her the Virgo Award (2022) and GWIC Braccini Prize (2023).

She later conducted postdoctoral research at MIT, working on scattered light analysis for LIGO Hanford, assembling Output Mode Cleaner cavities at Caltech, and developing fiber interferometers for entangled-state gravitational measurements.

Currently, she is a Research Scientist at CNRS in the ARTEMIS laboratory at the Observatoire de la Côte d'Azur, focusing on gravitational wave detectors (current and future) and fundamental physics experiments.

 Gravitational waves.- Ground based gravitational waves detectors.- Theory of quantum light in gravitational waves detectors.- Quantum noise reduction system overview in Advanced Virgo Plus.- Quantum noise reduction system commissioning.- Stray light in gravitational waves detectors.- Ghost beams study and mitigation.- Active control of scattered light on the FDS system.- Matching of the squeezing beam to the ITF.- New high finesse Output Mode Cleaner for Advanced Virgo Plus.

Erscheinungsdatum
Reihe/Serie Springer Theses
Zusatzinfo XXI, 248 p. 150 illus., 145 illus. in color.
Verlagsort Cham
Sprache englisch
Maße 155 x 235 mm
Themenwelt Naturwissenschaften Physik / Astronomie Theoretische Physik
Schlagworte Advanced Virgo+ interferometer • Frequency-dependent squeezing in laser interferometers • Gravitational wave detection • Optical cavities in interferometry • Output mode cleaner cavity in interferometers • Quantum noise in gravitational wave detectors • Stray and scattered light effects • Suspended optical benches
ISBN-10 3-031-95142-5 / 3031951425
ISBN-13 978-3-031-95142-8 / 9783031951428
Zustand Neuware
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