Laser interferometry for the Big Bang Observer
By Gregory M. Harry, P. Fritschel, D. Shaddock, William M. Folkner, E. Phinney. 2006
426 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics
View Paper: https://www.semanticscholar.org/paper/f27a1f61ed321962ed2d43cb0fcf62c51a08f915
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In Astronomy and Astrophysics
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Citations in the corpus
- Solar-mass primordial black holes explain NANOGrav hint of gravitational waves (2020, methodology): “Future prospects of various GW observations are also shown: SKA [61], LISA [103], TianQin [104, 105], BBO [106], DECIGO [107], AION [108], AEDGE [109], Advanced LIGO Hanford and Livingston [110] combined with Advanced Virgo [111] as well as LIGO India [112, 113] and KAGRA [114, 115] (HLVIK), and Ein”
- Semianalytic calculation of gravitational wave spectrum nonlinearly induced from primordial curvature perturbations (2018, methodology): “The observations are from SKA [58], eLISA [59], LISA [60], BBO [61], DECIGO [62], Einstein Telescope [63], Cosmic Explorer [64], and KAGRA [65].”
- The stochastic gravitational wave background from turbulence and magnetic fields generated by a first-order phase transition (2009, methodology): “LIGO Corr AGIS LISA BBO BBO Corr 10-4 0.01 1 100 10-27 10-25 10-23 10-21 10-19 f HHzL h Figure 16.”