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\textit{Euclid}: From Galaxies to Gravitational Waves -- Forecasting Stochastic Gravitational Wave Background Anisotropies and Their Cross-Correlation
K. Z. Yang, G. Cusin, V. Mandic +141
We estimate the amplitude and spatial anisotropy in the stochastic gravitational wave background (SGWB) energy density due to compact binary coalescence (CBC) events: binary black…
Aberration of gravitational waveforms by peculiar velocity
Camille Bonvin, Giulia Cusin, Cyril Pitrou +3
One key prediction of General Relativity is that gravitational waves are emitted with a pure spin-2 polarisation. Any extra polarisation mode, spin-1 or spin-0, is consequently con…
Space tests of the strong equivalence principle: BepiColombo and the Sun-Earth Lagrangian points opportunity
Fabrizio De Marchi, Giuseppe Congedo
The validity of General Relativity, after 100 years, is supported by solid experimental evidence. However, there is a lot of interest in pushing the limits of precision by other ex…
Detection principle of gravitational wave detectors
Giuseppe Congedo
With the first two detections in late 2015, astrophysics has officially entered into the new era of gravitational wave observations. Since then, much has been going on in the field…
Testing the Strong Equivalence Principle with spacecraft ranging towards the nearby Lagrangian points
Giuseppe Congedo, Fabrizio De Marchi
General relativity is supported by great experimental evidence. Yet there is a lot of interest in precisely setting its limits with on going and future experiments. A question to a…
Derivative of the light frequency shift as a measure of spacetime curvature for gravitational wave detection
Giuseppe Congedo
The measurement of frequency shifts for light beams exchanged between two test masses nearly in free fall is at the heart of gravitational wave detection. It is envisaged that the…