Bereiche | Tage | Auswahl | Suche | Downloads | Hilfe

Q: Fachverband Quantenoptik und Photonik

Q 3: Präzisionsmessungen und Metrologie I

Q 3.4: Gruppenbericht

Montag, 10. März 2008, 15:30–16:00, 3D

LISA: Laser interferometry for the spaceborne gravitational wave detection — •Antonio Francisco Garcia Marin¹, Felipe Guzman Cervantes¹, Frank Steier¹, Simon Barke¹, Christian Diekmann¹, Roland Fleddermann¹, Benjamin Sheard¹, Michael Tröbs¹, Juan Jose Esteban Delgado¹, Iouri Bykov¹, Jens Reiche¹, Oliver Jennrich², Gerhard Heinzel¹, and Karsten Danzmann¹ — ¹Albert-Einstein-Institut Hannover, Max-Planck-Institut für Gravitationsphysik and Universität Hannover, Germany — ²ESA ESTEC, Noordwijk, The Netherlands

The Laser Interferometer Space Antenna (LISA) is a joint ESA-NASA mission designed to observe gravitational waves in the frequency range between 0.1 to 100 mHz, where ground-based detectors are limited by terrestrial noise. Sources in this frequency range include supermassive black holes and galactic binary stars. LISA consists of three identical spacecraft separated by 5 million kilometers carrying a total of six free flying test masses in heliocentric drag-free orbit. The fluctuations in separation between two of these test masses located in different satellites will be measured by laser interferometry with picometre precision. I will present a brief overview of the LISA mission with special emphasis on the laser interferometry, the research field at the Albert Einstein Institute.