Master in Physics at University of Pisa, Italy (1997), and doctorate in Physics from Scuola Normale Superiore di Pisa, Italy (2000). Has experience in Physics, focusing on Gravitational Wave Physics. Post-docs: U. fo Helsinki (Finland) 9/01 -- 8/03, U. of Geneva (Switzerland) 10/03 -- 10/08, U. of Urbino (Italy) 11/08 -- 11/12, Young Investigator at IFT (UNESP, São Paulo) 3/13--9/16, Researcher at International Institute of Physics (Natal) between 10/16 and 2/22. Since March 2022 Researcher at IFT-UNESP and ICTP-SAIFR. (Source: Lattes Curriculum)
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Gravitational waves are propagating ripples in space-time geometry, produced bythe accelerated motion of massive astrophysical objects or by cosmologicalsources, and they have been first observed by the Advanced Laser Interferometer Gravitational Observatory (LIGO) in September 2015, when the signal from a pairof coalescing black holes were detected. Since then, during the observationrun …
The gravitational wave astronomy era will start in a few years time, with the most likely candidate source for repeated detection being coalescing binaries made of compact objects like neutron stars and stellar mass black holes. However, for earth-based detectors like LIGO and Virgo the signals are buried deeply within the instrumental noise, thus a detailed knowledge of the signal itself…
Gravitational waves (GW) were predicted by Einstein as a consequence of his theory of general relativity. They are produced when mass and energy distributions change their configuration; they present themselves as wave- like distortions of the space-time metric. Only extreme cosmological and astrophysical events may produce GWs at a detectable leveI. This includes the early universe, supe…
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