Mon Oct 13, F. Flechtner
• Sorted by Date • Sorted by Last Name of First Author •
Sesana, A., Weber, W. J., Killow, C. J., Perreur-Lloyd, M., Robertson, D. I., Ward, H., Fitzsimons, E. D., Bryant, J., Cruise, A. M., Dixon, G., Hoyland, D., Smith, D., Bogenstahl, J., McNamara, P. W., Gerndt, R., Flatscher, R., Hechenblaikner, G., Hewitson, M., Gerberding, O., Barke, S., Brause, N., Bykov, I., Danzmann, K., Enggaard, A., Gianolio, A., Vendt Hansen, T., Heinzel, G., Hornstrup, A., Jennrich, O., Kullmann, J., Møller-Pedersen, S., Rasmussen, T., Reiche, J., Sodnik, Z., Suess, M., Armano, M., Sumner, T., Bender, P. L., Akutsu, T., and Sathyaprakash, B. S., 2014. Space-based detectors. General Relativity and Gravitation, 46:1793, doi:10.1007/s10714-014-1793-0.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2014GReGr..46.1793S,
author = {{Sesana}, A. and {Weber}, W.~J. and {Killow}, C.~J. and {Perreur-Lloyd}, M. and {Robertson}, D.~I. and {Ward}, H. and {Fitzsimons}, E.~D. and {Bryant}, J. and {Cruise}, A.~M. and {Dixon}, G. and {Hoyland}, D. and {Smith}, D. and {Bogenstahl}, J. and {McNamara}, P.~W. and {Gerndt}, R. and {Flatscher}, R. and {Hechenblaikner}, G. and {Hewitson}, M. and {Gerberding}, O. and {Barke}, S. and {Brause}, N. and {Bykov}, I. and {Danzmann}, K. and {Enggaard}, A. and {Gianolio}, A. and {Vendt Hansen}, T. and {Heinzel}, G. and {Hornstrup}, A. and {Jennrich}, O. and {Kullmann}, J. and {M{\o}ller-Pedersen}, S. and {Rasmussen}, T. and {Reiche}, J. and {Sodnik}, Z. and {Suess}, M. and {Armano}, M. and {Sumner}, T. and {Bender}, P.~L. and {Akutsu}, T. and {Sathyaprakash}, B.~S.},
title = "{Space-based detectors}",
journal = {General Relativity and Gravitation},
keywords = {LISA Pathfinder, Optical bench Interferometer, Spaceborne precision metrology, Interferometry, Phasemeter, Gravitational waves},
year = 2014,
month = dec,
volume = {46},
eid = {1793},
pages = {1793},
abstract = "{The parallel session C5 on Space-Based Detectors gave a broad overview
over the planned space missions related to gravitational wave
detection. Overviews of the revolutionary science to be expected
from LISA was given by Alberto Sesana and Sasha Buchman. The
launch of LISA Pathfinder (LPF) is planned for 2015. This
mission and its payload ``LISA Technology Package'' will
demonstrate key technologies for LISA. In this context,
reference masses in free fall for LISA, and gravitational
physics in general, was described by William Weber, laser
interferometry at the pico-metre level and the optical bench of
LPF was presented by Christian Killow and the performance of the
LPF optical metrology system by Paul McNamara. While LPF will
not yet be sensitive to gravitational waves, it may nevertheless
be used to explore fundamental physics questions, which was
discussed by Michele Armano. Some parts of the LISA technology
that are not going to be demonstrated by LPF, but under
intensive development at the moment, were presented by Oliver
Jennrich and Oliver Gerberding. Looking into the future, Japan
is studying the design of a mid-frequency detector called
DECIGO, which was discussed by Tomotada Akutsu. Using atom
interferometry for gravitational wave detection has also been
recently proposed, and it was critically reviewed by Peter
Bender. In the nearer future, the launch of GRACE Follow-On (for
Earth gravity observation) is scheduled for 2017, and it will
include a Laser Ranging Interferometer as technology
demonstrator. This will be the first inter-spacecraft laser
interferometer and has many aspects in common with the LISA long
arm, as discussed by Andrew Sutton.}",
doi = {10.1007/s10714-014-1793-0},
adsurl = {https://ui.adsabs.harvard.edu/abs/2014GReGr..46.1793S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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