LISA technology - concept, status, prospects

By K. Danzmann, A. Rüdiger. 2003

306 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/b400a970fc50d09f91d2f09697a005828b58fdfc

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Citations in the corpus

Gravitational wave production by collisions: more bubbles (2008, background): “This result is especially interesting in the light of recent investigations [7, 8] that indicate that in the case of a first-order electroweak phase transition (obtained by a singlet sector [14, 15] or higher dimensional operators [16]–[18]) the peak frequency of the radiation produced is below the ”
Chern-Simons Modified General Relativity (2009, methodology): “[33] have proposed a GW test of non-dynamical CS modified with a generic CS scalar through the spaceborne GW detector LISA [156–160].”
Les Houches lectures on effective field theories and gravitational radiation (2007, background): “If we decompose the typical gravitational wave signal as h(t) = A(t) cosφ(t), (2.12) then interferometric detectors, such as LIGO/VIRGO and LISA, are particularly sensitive to the phaseφ(t) ∼ 2 ∫ t dτω(τ) of the gravitational wave.”
Physics, Astrophysics and Cosmology with Gravitational Waves (2009, unknown): “1 Hz for the first time [196, 144].”
Gravitational Radiation Detection with Laser Interferometry (2013, background): “NGO (previously LISA: the Laser Interferometer Space Antenna) is a proposed ESA mission (Danzmann and R¨udiger, 2003; Faller et al. , 1989; Prince and the LISA Science Team, 2009; Prince et al. , 2002) slated for launch in the early part of the 21 st century.”
Intersatellite laser ranging instrument for the GRACE follow-on mission (2012, background): “…and the Laser Interferometer Space Antenna (LISA), a space-based gravitational wave detector under development (Danzmann and the LISA Science Team 2003; Danzmann and Rüdiger 2003; Heinzel et al. 2006; Shaddock 2008), from which the proposed instrument derives a number of key technologies.”