Collaboration:
Laboratory: Collaboration sites
National Responsible: F. Vetrano (Urbino/Fi)
1. Goal of the experiment
Virgo R&D is an experiment constituted by many sub-projects aiming at insuring that projected sensitivity of Virgo detector (the gravitational antenna which has been built in Cascina, near Pisa) will be reached and preserved, or else to improve Virgo sensitivity by reducing the noise. From this point of view, Virgo R&D is presently the most powerful effort to improve the performances of ground-based interferometric gravitational detectors at short- and medium time.
2.
Activities during 2001
All other cited R&D activities have been projected for starting from next year (2003).
Milestones 2002
Data taking and PSD for thermal noise of the LFF tower | 30-06-2002 |
Completion of the hardware structure for monocristalline suspension | 31-07-2002 |
Set up on Cascina of the UVVV technique | 31-07-2002 |
3 INFN contribution to the experiment in terms of manpower
Manpower: 5 researchers (1.8 FTE), 4 technologists (1.3 FTE), 2 technicians (0.7 FTE)
4 - Number of publications in refereed journals: 3
5 Conferences talks: 3
6 Number of undergraduate and doctoral theses on the experiment: 6
7 Leadership role in the experiment
Spokesperson of the Virgo R&D Collaboration is Flavio Vetrano from Urbino University & Florence INFN Section. For each sub-project there are corresponding leading persons: A. Di Virgilio from Pisa for LFF; L. Gammaitoni from Perugia for LDSW; M. Tonelli from Pisa for Crystal; F. Strumia from Pisa for UVVV; F. Ricci from Roma1 for GRID; F. Barone from Napoli for ElPu e AOC.
8 Innovative instruments
9 Competing experiments
For LFF: TNI (Thermal Noise Interferometer) in Caltech