2024 (v1)
Publication
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Uploaded on: September 7, 2024
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Last name: ANDREA CHINCARINI
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Ta2O5 mechanical losses seem to be the main cause of mirror thermal noise, limiting current interferometric gravitational wave detectors sensitivity in the 50-300 Hz frequency range. Work is in progress for the identification of these relaxation processes probably related with lattice defects and impurities that are distributed both in the...