Benjamin Lange 2001 Class. Quantum Grav. 18 4153 doi:10.1088/0264-9381/18/19/325
Benjamin Lange
Show affiliationsThe very low specific-force noise specification of the LISA mission requires a drag-free satellite for its realization. Not only is the lowest specific-force noise most likely to be achieved by a completely free-floating proof mass with a wide gap and no applied forces or torques, but the performance of such a system can be assured by prior drag-free satellite experience so that a technology demonstration mission for the drag-free specification would not be needed. Better performance can be achieved if it is possible to present a defined reflecting surface to the laser beam. This paper discusses the techniques of having a defined surface and other issues involved with spherical proof masses.
04.80.Nn Gravitational wave detectors and experiments
06.30.Bp Spatial dimensions (e.g., position, lengths, volume, angles, and displacements)
Issue 19 (7 October 2001)
Received 5 July 2001
Published 17 September 2001
Benjamin Lange 2001 Class. Quantum Grav. 18 4153
Cheng-Ying Chou et al 2007 Phys. Med. Biol. 52 1923
Alexander Sakhnovich 2006 Inverse Problems 22 2083
D V Ahluwalia-Khalilova 2005 Class. Quantum Grav. 22 1433
P. Español and P. Warren 1995 Europhys. Lett. 30 191
Luo Shao-kai et al 2001 Chinese Phys. 10 271
M D Karunanayake et al 2007 Meas. Sci. Technol. 18 1908
Maurice G Cox 2007 Metrologia 44 187
S E Alm and R Parviainen 2004 J. Phys. A: Math. Gen. 37 549
David T Burns et al 2007 Metrologia 44 L53