Laboratory: EGO, Cascina
National Responsible: F. Vetrano (Urbino/Fi)
Home page of the experiment: http://www.virgo.infn.it/
1. Goal of the experiment
The scientific goal of the experiment, after the end of the construction and the commissioning of the interferometric gravitational antenna Virgo (a suspended Michelson interferometer, with 3 km Fabry-Pérot cavities as orthogonal arms), is to reach sensitivity enough, to take data, to develop analysis strategy, in order to be able to detect gravitational waves from astrophysical and/or cosmological sources, provided their amplitudes are those by currently accepted theoretical models.
2.
Activities during 2001
Virgo experiment is beginning its activity in 2002, but it was preceeded by a long Special Project (1994-2001), which was entirely devoted to the construction of the antenna with all related infrastructures. The construction and the commissioning of the Central Interferometer (a suspended 6 m Michelson interferometer without Fabry-Pérot cavities) are now approaching the end, and the commissioning of CITF has been a good fundamental learning for the way along with we will move towards Virgo-3km, showing fundamental characteristics of detector noise against which we are (and we will be) fighting.
Milestones 2002
Completion of the towers at the end of the interferometer | 31-05-2002 |
Debugging of the interferometer | 30-09-2002 |
Full planning of the interferometer Commissioning | 31-11-2002 |
Conclusion of the tests for distributed calculus on the FI/Urbino- PG-NA-Roma1 clusters for Virgo data analysis | 31-12-2002 |
3. INFN contribution to the experiment in terms of manpower
Manpower: 83 researchers (62.8 FTE), 19 technicians (8.5 FTE)
Budget for the Year 2002: 1108,5 kEuro
4. Publications in refereed journals (Year 2001): 8
5. Conference talks (Year 2001): 9
6. Number of undergraduate and doctoral theses on the experiment: 12
7. Leadership roles in the experiment
8. Innovative instruments
9. Competing experiments
LIGO (USA)