D
D.O. Richstone
Researcher at University of Michigan
Publications - 2
Citations - 656
D.O. Richstone is an academic researcher from University of Michigan. The author has contributed to research in topics: Gravitational-wave observatory & Gravitational wave. The author has an hindex of 2, co-authored 2 publications receiving 651 citations.
Papers
More filters
Posted Content
Laser Interferometer Space Antenna
I. Ciufolini,Roland Schilling,Benjamin William Allen,Pierre Touboul,H. Ward,G. Schafer,Bangalore Suryanarayana Sathyaprakash,J.C. Ray,Craig J. Hogan,D.O. Richstone,Curt Cutler,W. Hiscock,H. Dittus,S.Buchman,Lee Samuel Finn,Walter Winkler,F. Fidecaro,Robin T. Stebbins,S. Shapiro,M.C.W. Sanford,O. Bales,B. Teegarden,K. A. Thorne,Massimo Tinto,Clive C. Speake,J. Y. Vinet,R.D. Newman,Karsten Danzmann,Rainer Weiss,Stefano Vitale,E.L. Turner,R. Reinhard +31 more
TL;DR: The LISA Consortium as discussed by the authors proposed a 4-year mission in response to ESA's call for missions for L3, which provides the closest ever view of the infant universe at TeV energy scales, has known sources in the form of verification binaries in the Milky Way, and can probe the entire universe, from its smallest scales near the horizons of black holes, all the way to cosmological scales.
Journal ArticleDOI
LISA and its in-flight test precursor SMART-2
Stefano Vitale,Peter L. Bender,A. Brillet,Saps Buchman,Antonella Cavalleri,Massimo Cerdonio,M. Cruise,Curt Cutler,Karsten Danzmann,Rita Dolesi,William M. Folkner,Alberto Gianolio,Y. Jafry,G. Hasinger,Gerhard Heinzel,Craig J. Hogan,Mauro Hueller,J. H. Hough,S. Phinney,T. A. Prince,D.O. Richstone,D. I. Robertson,M. Rodrigues,Albrecht Rüdiger,M. Sandford,Roland Schilling,D. H. Shoemaker,B. F. Schutz,Robin T. Stebbins,Christopher W. Stubbs,Tamara Sumner,Kip S. Thorne,M. Tinto,P. Touboul,H. Ward,W. J. Weber,Walter Winkler +36 more
TL;DR: The first space-home gravitational wave observatory, LISA, is scheduled to be launched in 2010-11 as discussed by the authors, where the principle of operation of LISA is based on laser ranging of test-masses under pure geodesic motion.