Broadband Quantum Noise Reduction in Advanced Virgo Plus: From Frequency-Dependent Squeezing Implementation to Detection Losses and Stray Light Mitiga
暫譯: 先進維爾戈加強版中的寬頻量子噪聲減少：從頻率依賴的擠壓實現到檢測損失與雜散光的減緩
Polini, Eleonora
- 出版商: Springer
- 出版日期: 2025-08-12
- 售價: $6,840
- 貴賓價: 9.8 折 $6,703
- 語言: 英文
- 頁數: 248
- 裝訂: Hardcover - also called cloth, retail trade, or trade
- ISBN: 3031951425
- ISBN-13: 9783031951428
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相關分類:
量子 Quantum
海外代購書籍(需單獨結帳)
相關主題
商品描述
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.
商品描述(中文翻譯)
本書介紹了在Virgo引力波探測器中首次實現的頻率依賴性擠壓（frequency-dependent squeezing），這是一種減少整個檢測頻帶量子噪聲的技術。透過降低噪聲，它增強了Virgo觀測宇宙的能力。
本書詳細描述了實驗光學系統，涵蓋數百米的範圍，以及導致首次觀測到頻率依賴性擠壓的測量活動，該擠壓在幾十赫茲的目標頻率下發生橢圓旋轉。此外，本書還涵蓋了在Virgo中對新輸出模式清潔器（Output Mode Cleaner）腔體的特性化和調試，以最小化擠壓態的光學損失。最後，本書探討了低頻下雜散光噪聲的影響，並研究了改善探測器靈敏度的減緩策略。
作者簡介
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.
作者簡介(中文翻譯)
埃莉諾拉·波利尼是一位專門研究重力波探測器量子噪聲減少的物理學家。她在羅馬薩賓納大學獲得物理學學士和碩士學位，並因學術優秀獲得恩里科·佩爾西科（Enrico Persico）和蒂托·馬亞尼（Tito Maiani）獎。
她在安納西粒子物理實驗室（Laboratoire d'Annecy de Physique des Particules）和薩瓦蒙特布朗大學（Université Savoie Mont Blanc）完成博士學位，研究重力波探測器維爾戈（Virgo）中的頻率依賴性擠壓。她的工作包括升級輸出模式清潔器（Output Mode Cleaner）腔體並調查雜散光噪聲，因而獲得維爾戈獎（Virgo Award，2022年）和GWIC-布拉奇尼獎（GWIC-Braccini Prize，2023年）。
之後，她在麻省理工學院（MIT）進行博士後研究，專注於LIGO漢福德（LIGO Hanford）的散射光分析，在加州理工學院（Caltech）組裝輸出模式清潔器腔體，並開發纖維干涉儀以進行糾纏態重力測量。
目前，她是法國國家科學研究中心（CNRS）ARTEMIS實驗室的研究科學家，專注於重力波探測器（目前和未來）及基礎物理實驗。
