Laser Interferometer Space Antenna

By M. Hewitson. 2012

2,006 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/17095bbeee08cac58f183c578dfad9eb4bed358e

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1. V. Cardoso
2. Paolo Pani
3. R. Cai
4. Emanuele Berti
5. E. Belgacem
6. Juan García-Bellido
7. R. Brito
8. E. Barausse

Citations in the corpus

• Galactic binary science with the new LISA design (2017, background): “The analytic fits to the confusion noise have the functional form Sc(f) = Af −7/3 e α+βf sin(κf) [1 + tanh(γ(fk − f))] Hz (3) The overall f−7/3 slope is the theoretical prediction for the power spectrum of a population of quasi-circular binaries evolving due to gravitational wave emission.”
• Theoretical Physics Implications of the Binary Black-Hole Mergers GW150914 and GW151226 (2016, background): “Another theoretical implication that could be derived from a coincident GW/electromagnetic observation is a severe constraint on gravitational parity violation [139, 141, 282].”
• New physics from the polarized light of the cosmic microwave background (2022, background): “The upcoming ESA Laser Interferometer Space Antenna ( LISA 177 ) mission is sensitive to λ ≃ a few hundred million km (10 − 3 Hz), comparable to astronomical units.”
• Science case for the Einstein telescope (2019, methodology): “If Einstein Telescope will be operational during the same period as LISA, joint LISA-ET observations of the same source will then be of great value [92].”
• Detecting high-frequency gravitational waves with microwave cavities (2021, background): “These include future ground-based [3–5] and space-based [6, 7] laser interferometers, atom interferometers [8–10], pulsar timing arrays [11, 12], and CMB observations [13, 14], as well as new types of astrophysical signatures [15].”
• Solar-mass primordial black holes explain NANOGrav hint of gravitational waves (2020, methodology): “Future prospects of various GW observations are also shown: SKA [51], LISA [93], TianQin [94, 95], BBO [96], DECIGO [97], AION [98], AEDGE [99], Advanced LIGO Hanford and Livingston [100] combined with Advanced Virgo [101] as well as LIGO India [102, 103] and KAGRA [104, 105] (HLVIK), and Einstein T”
• Tests for the existence of black holes through gravitational wave echoes (2017, methodology): “For γecho = 20%, we estimate that the planned space mission LISA [53] will see at least one event per year, even for the most pessimistic population synthesis models used to estimate the rates [52].”
• Phase transitions in an expanding universe: stochastic gravitational waves in standard and non-standard histories (2020, unknown): “J C A P 0 1 ( 2 0 2 1 ) 0 0 1 10-4 10-3 10-2 10-1 1 10-20 10-18 10-16 10-14 10-12 10-10 10-8 Ta iji T ian Qi n BBO LISA DECIGO Asymptotic Figure 19.”