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Common-red-signal analysis with 24-yr high-precision timing of the European Pulsar Timing Array: Inferences in the stochastic gravitational-wave background search
S. Chen, R. N. Caballero, Y. J. Guo +49
We present results from the search for a stochastic gravitational-wave background (GWB) as predicted by the theory of General Relativity using six radio millisecond pulsars from th…
QSNET, a network of clocks for measuring the stability of fundamental constants
G. Barontini, V. Boyer, X. Calmet +19
The QSNET consortium is building a UK network of next-generation atomic and molecular clocks that will achieve unprecedented sensitivity in testing variations of the fine structure…
Ultra-low frequency gravitational waves from cosmological and astrophysical processes
Christopher J. Moore, Alberto Vecchio
Gravitational waves (GWs) at ultra-low frequencies () are key to understanding the assembly and evolution of astrophysical black hole (BH) binaries wi…
High mass but low spin: an exclusion region to rule out hierarchical black-hole mergers as a mechanism to populate the pair-instability mass gap
Davide Gerosa, Nicola Giacobbo, Alberto Vecchio
The occurrence of pair-instability supernovae is predicted to prevent the formation of black holes with masses . Recent gravitational-wave detections in this ma…