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A cryogenic silicon interferometer for gravitational-wave detection
Classical and Quantum Gravity ( IF 3.6 ) Pub Date : 2020-07-29 , DOI: 10.1088/1361-6382/ab9143 R X Adhikari 1 , K Arai 1 , A F Brooks 1 , C Wipf 1 , O Aguiar 2 , P Altin 3 , B Barr 4 , L Barsotti 5 , R Bassiri 6 , A Bell 4 , G Billingsley 1 , R Birney 7 , D Blair 8 , E Bonilla 6 , J Briggs 4 , D D Brown 9 , R Byer 6 , H Cao 9 , M Constancio 2 , S Cooper 10 , T Corbitt 11 , D Coyne 1 , A Cumming 4 , E Daw 12 , R deRosa 13 , G Eddolls 4 , J Eichholz 3 , M Evans 5 , M Fejer 6 , E C Ferreira 2 , A Freise 10 , V V Frolov 13 , S Gras 5 , A Green 14 , H Grote 15 , E Gustafson 1 , E D Hall 5 , G Hammond 4 , J Harms 16 , G Harry 17 , K Haughian 4 , D Heinert 18 , M Heintze 13 , F Hellman 19 , J Hennig 20 , M Hennig 20 , S Hild 21 , J Hough 4 , W Johnson 11 , B Kamai 1 , D Kapasi 3 , K Komori 5 , D Koptsov 22 , M Korobko 23 , W Z Korth 1 , K Kuns 5 , B Lantz 6 , S Leavey 20 , F Magana-Sandoval 14 , G Mansell 5 , A Markosyan 6 , A Markowitz 1 , I Martin 4 , R Martin 24 , D Martynov 10 , D E McClelland 3 , G McGhee 4 , T McRae 3 , J Mills 15 , V Mitrofanov 22 , M Molina-Ruiz 19 , C Mow-Lowry 10 , J Munch 9 , P Murray 4 , S Ng 9 , M A Okada 2 , D J Ottaway 9 , L Prokhorov 10 , V Quetschke 25 , S Reid 26 , D Reitze 1 , J Richardson 1 , R Robie 1 , I Romero-Shaw 27 , R Route 6 , S Rowan 4 , R Schnabel 23 , M Schneewind 20 , F Seifert 28 , D Shaddock 3 , B Shapiro 6 , D Shoemaker 5 , A S Silva 2 , B Slagmolen 3 , J Smith 29 , N Smith 1 , J Steinlechner 21 , K Strain 4 , D Taira 2 , S Tait 4 , D Tanner 14 , Z Tornasi 4 , C Torrie 1 , M Van Veggel 4 , J Vanheijningen 8 , P Veitch 9 , A Wade 3 , G Wallace 26 , R Ward 3 , R Weiss 5 , P Wessels 20 , B Willke 20 , H Yamamoto 1 , M J Yap 3 , C Zhao 8
Classical and Quantum Gravity ( IF 3.6 ) Pub Date : 2020-07-29 , DOI: 10.1088/1361-6382/ab9143 R X Adhikari 1 , K Arai 1 , A F Brooks 1 , C Wipf 1 , O Aguiar 2 , P Altin 3 , B Barr 4 , L Barsotti 5 , R Bassiri 6 , A Bell 4 , G Billingsley 1 , R Birney 7 , D Blair 8 , E Bonilla 6 , J Briggs 4 , D D Brown 9 , R Byer 6 , H Cao 9 , M Constancio 2 , S Cooper 10 , T Corbitt 11 , D Coyne 1 , A Cumming 4 , E Daw 12 , R deRosa 13 , G Eddolls 4 , J Eichholz 3 , M Evans 5 , M Fejer 6 , E C Ferreira 2 , A Freise 10 , V V Frolov 13 , S Gras 5 , A Green 14 , H Grote 15 , E Gustafson 1 , E D Hall 5 , G Hammond 4 , J Harms 16 , G Harry 17 , K Haughian 4 , D Heinert 18 , M Heintze 13 , F Hellman 19 , J Hennig 20 , M Hennig 20 , S Hild 21 , J Hough 4 , W Johnson 11 , B Kamai 1 , D Kapasi 3 , K Komori 5 , D Koptsov 22 , M Korobko 23 , W Z Korth 1 , K Kuns 5 , B Lantz 6 , S Leavey 20 , F Magana-Sandoval 14 , G Mansell 5 , A Markosyan 6 , A Markowitz 1 , I Martin 4 , R Martin 24 , D Martynov 10 , D E McClelland 3 , G McGhee 4 , T McRae 3 , J Mills 15 , V Mitrofanov 22 , M Molina-Ruiz 19 , C Mow-Lowry 10 , J Munch 9 , P Murray 4 , S Ng 9 , M A Okada 2 , D J Ottaway 9 , L Prokhorov 10 , V Quetschke 25 , S Reid 26 , D Reitze 1 , J Richardson 1 , R Robie 1 , I Romero-Shaw 27 , R Route 6 , S Rowan 4 , R Schnabel 23 , M Schneewind 20 , F Seifert 28 , D Shaddock 3 , B Shapiro 6 , D Shoemaker 5 , A S Silva 2 , B Slagmolen 3 , J Smith 29 , N Smith 1 , J Steinlechner 21 , K Strain 4 , D Taira 2 , S Tait 4 , D Tanner 14 , Z Tornasi 4 , C Torrie 1 , M Van Veggel 4 , J Vanheijningen 8 , P Veitch 9 , A Wade 3 , G Wallace 26 , R Ward 3 , R Weiss 5 , P Wessels 20 , B Willke 20 , H Yamamoto 1 , M J Yap 3 , C Zhao 8
Affiliation
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravitational wave astronomy, revealing a previously hidden side of the cosmos. To maximize the reach of the existing LIGO observatory facilities, we have designed a new instrument that will have 5 times the range of Advanced LIGO, or greater than 100 times the event rate. Observations with this new instrument will make possible dramatic steps toward understanding the physics of the nearby universe, as well as observing the universe out to cosmological distances by the detection of binary black hole coalescences. This article presents the instrument design and a quantitative analysis of the anticipated noise floor.
中文翻译：
一种用于引力波探测的低温硅干涉仪
LIGO 探测到来自紧密双星并合的引力波，开启了引力波天文学的时代，揭示了宇宙先前隐藏的一面。为了最大限度地扩大现有 LIGO 天文台设施的覆盖范围，我们设计了一种新仪器，其范围是 Advanced LIGO 的 5 倍，或事件率的 100 倍以上。使用这种新仪器进行观测将使了解附近宇宙的物理学以及通过检测双黑洞合并来观测宇宙到宇宙学距离方面迈出戏剧性的一步。本文介绍了仪器设计和预期本底噪声的定量分析。
更新日期：2020-07-29
中文翻译：
一种用于引力波探测的低温硅干涉仪
LIGO 探测到来自紧密双星并合的引力波，开启了引力波天文学的时代，揭示了宇宙先前隐藏的一面。为了最大限度地扩大现有 LIGO 天文台设施的覆盖范围，我们设计了一种新仪器，其范围是 Advanced LIGO 的 5 倍，或事件率的 100 倍以上。使用这种新仪器进行观测将使了解附近宇宙的物理学以及通过检测双黑洞合并来观测宇宙到宇宙学距离方面迈出戏剧性的一步。本文介绍了仪器设计和预期本底噪声的定量分析。
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