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
Fabian Brau 2004 J. Phys. A: Math. Gen. 37 6687
U De Angelis et al 1980 J. Phys. C: Solid State Phys. 13 3649
R Witt (for the STAR Collaboration) 2007 J. Phys. G: Nucl. Part. Phys. 34 S921
Diederik Aerts and Marek Czachor 2007 J. Phys. A: Math. Theor. 40 F259
V S Manko and E Ruiz 2004 Class. Quantum Grav. 21 5849
H S Domingos 2004 J. Phys.: Condens. Matter 16 9083
T Stauber and A Mielke 2003 J. Phys. A: Math. Gen. 36 2707
M Vos et al 1999 J. Phys.: Condens. Matter 11 3645
E A Carlen et al 2009 Nonlinearity 22 2919