학술논문
The US Program in Ground-Based Gravitational Wave Science: Contribution from the LIGO Laboratory
Document Type
Working Paper
Author
Reitze, David; Abbott, Rich; Adams, Carl; Adhikari, Rana; Aggarwal, Nancy; Anand, Shreya; Ananyeva, Alena; Anderson, Stuart; Appert, Stephen; Arai, Koji; Araya, Melody; Aston, Stuart; Barayoga, Juan; Barish, Barry; Barker, David; Barsotti, Lisa; Bartlett, Jeffrey; Betzwieser, Joseph; Billingsley, GariLynn; Biscans, Sebastien; Biscoveanu, Sylvia; Blackburn, Kent; Blair, Carl; Blair, Ryan; Bockelman, Brian; Bork, Rolf; Bramley, Alyssa; Brooks, Aidan; Brunett, Sharon; Buikema, Aaron; Cahillane, Craig; Callister, Thomas; Carruthers, Tom; Clara, Filiberto; Corban, Paul; Coughlin, Michael; Couvares, Peter; Cowart, Matthew; Coyne, Dennis; Demos, Nicholas; Donovan, Fred; Driggers, Jenne; Dwyer, Sheila; Effler, Anamaria; Eisenstein, Robert; Etzel, Todd; Evans, Matthew; Evans, Tom; Feicht, Jon; Fernandez-Galiana, Alvaro; Fritschel, Peter; Frolov, Valery; Fyffe, Michael; Gateley, Bubba; Giaime, Joe; Giardina, Dwayne; Goetz, Evan; Gossan, Sarah; Gras, Slawomir; Grassia, Philippe; Gray, Corey; Gupta, Anchal; Gustafson, Eric; Guthman, Les; Hall, Evan; Hanks, Jonathan; Hanson, Joe; Hasskew, Raine; Haster, Carl-Johan; Heintze, Matthew; Hernandez, Edgar; Holt, Kathy; Huang, Yiwen; Huynh-Dinh, Tien; Isi, Max; Jones, Jeff; Kamai, Brittany; Kanner, Jonah; Kasprzack, Marie; Katsavounidis, Erik; Katzman, William; Kawabe, Keita; King, Peter; Kissel, Jeffrey; Kondrashov, Veronica; Korth, William; Kozak, Dan; Kumar, Rahul; Landry, Michael; Lane, Benjamin; Lanza, Robert; Laxen, Michael; Lazzarini, Albert; Lecoeuche, Yannick; Libbrecht, Ken; Lo, Ka-Lok; London, Lionel; Lormand, Marc; MacInnis, Myron; Mansell, Georgia; Markowitz, Aaron; Maros, Ed; Marx, Jay; Mason, Ken; Massinger, Thomas; Matichard, Fabrice; Mavalvala, Nergis; McCarthy, Richard; McCormick, Scott; McCuller, Lee; McIver, Jessica; Mendell, Gregory; Merilh, Edmond; Meshkov, Syd; Mittleman, Richard; Moraru, Dan; Moreno, Gerardo; Mullavey, Adam; Nelson, Timothy; Ng, Kwan-Yeung; Noh, Minkyun; O'Reilly, Brian; Oberling, Jason; Oram, Richard; Osthelder, Charles; Overmier, Harry; Parker, William; Pedraza, Mike; Pele, Arnaud; Perez, Carlos; Petterson, Danielle; Pirello, Marc; Raab, Fred; Radkins, Hugh; Mohapatra, Satyanarayan Ray Pitambar; Richardson, Jonathan; Robertson, Norna; Rollins, Jameson; Romel, Chandra; Romie, Janeen; Ryan, Kyle; Sadecki, Travis; Sanchez, Eduardo; Sanchez, Luis; Savage, Richard; Schaetzl, Dean; Sellers, Danny; Shaffer, Thomas; Shoemaker, David; Sigg, Daniel; Strunk, Amber; Sudhir, Vivishek; Sun, Ling; Tao, Duo; Taylor, Robert; Thomas, Michael; Thomas, Patrick; Thorne, Keith; Torrie, Calum; Traylor, Gary; Trudeau, Randy; Tse, Maggie; Vajente, Gabriele; Vass, Steve; Venugopalan, Gautam; Vitale, Salvatore; Vorvick, Cheryl; Wade, Andrew; Wallace, Larry; Warner, Jim; Weaver, Betsy; Weinstein, Alan; Weiss, Rainer; Whitcomb, Stan; Whittle, Chris; Willis, Joshua; Wipf, Christopher; Xiao, Sophia; Yamamoto, Hiro; Yu, Hang; Yu, Haocun; Zhang, Liyuan; Zucker, Michael; Zweizig, John
Source
2019 BAAS 51(3) 141
Subject
Language
Abstract
Recent gravitational-wave observations from the LIGO and Virgo observatories have brought a sense of great excitement to scientists and citizens the world over. Since September 2015,10 binary black hole coalescences and one binary neutron star coalescence have been observed. They have provided remarkable, revolutionary insight into the "gravitational Universe" and have greatly extended the field of multi-messenger astronomy. At present, Advanced LIGO can see binary black hole coalescences out to redshift 0.6 and binary neutron star coalescences to redshift 0.05. This probes only a very small fraction of the volume of the observable Universe. However, current technologies can be extended to construct "$3^\mathrm{rd}$ Generation" (3G) gravitational-wave observatories that would extend our reach to the very edge of the observable Universe. The event rates over such a large volume would be in the hundreds of thousands per year (i.e.tens per hour). Such 3G detectors would have a 10-fold improvement in strain sensitivity over the current generation of instruments, yielding signal-to-noise ratios of 1000 for events like those already seen. Several concepts are being studied for which engineering studies and reliable cost estimates will be developed in the next 5 years.
Comment: For the 2020 Astro decadal
Comment: For the 2020 Astro decadal