articleTop 10% cited
Laser interferometry for the Big Bang Observer
Classical and Quantum Gravity · 2006 · Vol. 23(15) · pp. 4887–4894
Gregory M Harry✉(Massachusetts Institute of Technology)P. Fritschel(Massachusetts Institute of Technology)D. A. Shaddock(Jet Propulsion Laboratory)W. M. Folkner(Jet Propulsion Laboratory)E. S. Phinney(California Institute of Technology)
Abstract
The Big Bang Observer is a proposed space-based gravitational-wave detector intended as a follow on mission to the Laser Interferometer Space Antenna (LISA). It is designed to detect the stochastic background of gravitational waves from the early universe. We discuss how the interferometry can be arranged between three spacecraft for this mission and what research and development on key technologies are necessary to realize this scheme.
Advanced Frequency and Time StandardsPulsars and Gravitational Waves ResearchCold Atom Physics and Bose-Einstein CondensatesPhysicsInterferometryGravitational waveObserver (physics)SpacecraftLaserAtom interferometerDetectorGravitational-wave observatorySpace (punctuation)
Funding
- National Aeronautics and Space Administration
Citations
418
FWCI
4.15
field-weighted impact
References
11
Percentile
94%
vs. same field & year
Citations per year
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References
Beyond LISA: Exploring future gravitational wave missions
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2005 · 656 citations
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