RICERCA

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    The research activities of the Amaldi Research Center are organized into the following research areas:

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    The Third Generation Gravitational Wave Detector Laboratory (3G GW Lab) will play a key role in the development and construction of the 3G detectors that will observe the Universe up to its extreme border. An opto-cryogenic infrastructure will be built to house the prototypes made by the Quantum...

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    In the frequency zone where the sensitivity of interferometers for GW detection is higher, the limit of these detectors is due to the thermal noise of the mirrors, ultimately determined by the acoustic dissipation of the thin films that form the coatings and determine their high optical...
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    Quantum technologies are a promising resource...

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    Since 2013, the detection of a diffuse flux of high-energy neutrinos (0.1-10 PeV), in excess with respect to the atmospheric one, has opened a new window to the Universe, revealing the existence of extremely energetic astrophysical neutrino sources. Within the context of standard acceleration...

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    The Gravitational-Astronomy era has officially started on September 14, 2015, when the the worldwide LIGO-Virgo scientific collaboration has detected the first transient GW signal. After that date, several...

L' Università degli Studi di Roma "La Sapienza" - Piazzale Aldo Moro 5, 00185 Roma