用于重力波检测的低温硅干涉仪

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用于重力波检测的低温硅干涉仪

A Cryogenic Silicon Interferometer for Gravitational-wave Detection

论文作者

Adhikari, Rana X, Aguiar, Odylio, Arai, Koji, Barr, Bryan, Bassiri, Riccardo, Billingsley, Garilynn, Birney, Ross, Blair, David, Briggs, Joseph, Brooks, Aidan F, Brown, Daniel D, Cao, Huy-Tuong, Constancio, Marcio, Cooper, Sam, Corbitt, Thomas, Coyne, Dennis, Daw, Edward, Eichholz, Johannes, Fejer, Martin, Freise, Andreas, Frolov, Valery, Gras, Slawomir, Green, Anna, Grote, Hartmut, Gustafson, Eric K, Hall, Evan D, Hammond, Giles, Harms, Jan, Harry, Gregg, Haughian, Karen, Hellman, Frances, Hennig, Jan-Simon, Hennig, Margot, Hild, Stefan, Johnson, Warren, Kamai, Brittany, Kapasi, Disha, Komori, Kentaro, Korobko, Mikhail, Kuns, Kevin, Lantz, Brian, Leavey, Sean, Magana-Sandoval, Fabian, Markosyan, Ashot, Martin, Iain, Martin, Rodica, Martynov, Denis V, Mcclelland, David, Mcghee, Graeme, Mills, Joseph, Mitrofanov, Valery, Molina-Ruiz, Manel, Mow-Lowry, Conor, Murray, Peter, Ng, Sebastian, Prokhorov, Leonid, Quetschke, Volker, Reid, Stuart, Reitze, David, Richardson, Jonathan, Robie, Raymond, Romero-Shaw, Isobel, Rowan, Sheila, Schnabel, Roman, Schneewind, Merle, Shapiro, Brett, Shoemaker, David, Slagmolen, Bram, Smith, Joshua, Steinlechner, Jessica, Tait, Simon, Tanner, David, Torrie, Calum, Vanheijningen, Joris, Veitch, Peter, Wallace, Gavin, Wessels, Peter, Willke, Benno, Wipf, Christopher, Yamamoto, Hiro, Zhao, Chunnong, Barsotti, Lisa, Ward, Robert, Bell, Angus, Byer, Robert, Wade, Andrew, Korth, William Z, Seifert, Frank, Smith, Nicholas, Koptsov, Dimitry, Tornasi, Zeno, Markowitz, Aaron, Mansell, Georgia, Mcrae, Terry, Altin, Paul, Yap, Min J, Van Veggel, Marielle, Eddolls, Graeme, Bonilla, Edgard, Ferreira, Elvis C, Silva, Allan S, Okada, Marcos A, Taira, Diego, Heinert, Daniel, Hough, James, Strain, Ken, Cumming, Alan, Route, Roger, Shaddock, Daniel, Evans, Matthew, Weiss, Rainer

论文摘要

利戈（Ligo）从紧凑型二元合并中检测引力波已经打开了引力波天文学的时代，揭示了宇宙的先前隐藏的一侧。为了最大程度地提高现有的Ligo天文台设施的覆盖范围，我们设计了一种新仪器，其范围是高级LIGO范围的5倍，即事件速率的100倍以上。使用这种新仪器的观察将为理解附近宇宙的物理学做出巨大的步骤，并通过发现二进制黑洞合并的发现来观察宇宙到宇宙学的距离。本文介绍了仪器设计和对预期噪声的定量分析。

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.

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