Accedi

2nd ET GENERAL WORKSHOP

14–16 ott 2009
Ettore Majorana Foundation
Europe/Rome fuso orario

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16. Welcome talk(s)
14/10/09, 14:00
oral presentation
Workshop opening session
17. Status of the current and advanced GW detectors
Dr. Harald Lueck (AEI Hannover (MPI f. gravitational Physics / Inst. f. Grav.physics Leibniz Uni Hannover))
14/10/09, 14:10
18. ET project status and evolution
Michele Punturo (PG)
14/10/09, 14:30
0. Core-Collapse Supernova and Long-Soft GRB Science Goals with ET
Dr. Christian Ott (Caltech and Niels Bohr Institute)
14/10/09, 15:00
WP4: Astrophysics
WG4 - Astrophysics - 1
3. Exploring intermediate and massive black-hole binaries with IMRI sources
Dr. Jonathan Gair (University of Cambridge)
14/10/09, 15:20
1. Testing star formation models with ET
Dr. Christian Van Den Broeck (Nikhef)
14/10/09, 15:40
WP4: Astrophysics
WG4 - Astrophysics - 1
30. Multi-messengers in ET
Dr. Martin Hendry
14/10/09, 16:00
4. Accurate SNR and parameter estimation calculations for ET
Dr. Eliu Huerta (IoA, Cambridge)
14/10/09, 17:00
WP4: Astrophysics
WG4 - Astrophysics - 2
5. Stochastic backgrounds and the early universe the Einstein Telescope
Dr. Thomas Dent (Cardiff University)
14/10/09, 17:20
19. Parametrized tests of post mewtonian Theory with ET
Dr. Chandrakant Misra
14/10/09, 17:40
6. Testing GR with ET
Dr. Walter Del Pozzo (University of Birmingham)
14/10/09, 18:00
7. Computing infrastructure for ET
Dr. Leone Battista Bosi (INFN Perugia)
14/10/09, 18:20
9. Thermal Noise Modeling
Paola Puppo (RM1)
15/10/09, 08:30
10. Thermal Noise and Material Issues for ET
Dr. Ronny Nawrodt
15/10/09, 08:50
41. Cryogenic Si-Si Bond Strength Testing
Dr. Nicola Beverigde
15/10/09, 09:10
11. Mirror thermal noise and its implication on the mirror design
Sig.na Janyce FRANC (CNRS)
15/10/09, 09:30
12. Measurements of superattenuator performance on the VIRGO itf:a comparison with ET requirements
Dr. Stefano BRACCINI
15/10/09, 09:50
13. the superattenuator upgrades and the SAFE project
Franco Frasconi (PI)
15/10/09, 10:10
14. Sensor and actuators for ET
Ettore Majorana (RM1)
15/10/09, 10:50
15. Cooling issues
Fulvio Ricci (RM1)
15/10/09, 11:10
WP1: Site and Infrastructures
WG2 - Suspensions and thermal noise 2
20. Squeezed light integration at GEO 600 and beyond
Sig. Alexander Khalaidovski
15/10/09, 15:00
21. Squeezed light generation at 1064 nm and 1550 nm
Dr. Tobias Eberle
15/10/09, 15:15
22. Absorption measurements on silicon
Dr. Sebastian Steinlechner
15/10/09, 15:30
23. Parametric instability of a cavity of ET
Dr. Kazuhiro Yamamoto
15/10/09, 15:50
25. Thermal Noise Reduction through LG modes
Dr. Janyce FRANC
15/10/09, 16:10
26. LG Mode Generation
Dr. Keiko Kokeyama
15/10/09, 16:25
24. Displacement Noise Free Interferometry
Dr. Sergey Tarabrin
15/10/09, 17:20
27. xylophone topologies
Dr. stefan hild
15/10/09, 17:40
28. Topology comparison RSE vs. Sagnac using GWINC
Dr. Simon chelkowski
15/10/09, 18:05
29. Next steps: from technology reviews to detector design
Dr. Andreas Freise
15/10/09, 18:30
31. Status plans for ET WG1
Prof. Jo van den Brand (Nikhef - VU)
16/10/09, 09:20
32. Suspension an Mirror Cooling : impact on the infrastructure
Fulvio Ricci (RM1)
16/10/09, 09:40
33. Cultural Noise Measurements for Particle Accelerator Site selection
Dr. Heiko Ehrlichmann
16/10/09, 09:55
34. Plans for IliasNext
Alessio Rocchi (RM2)
16/10/09, 10:15
35. Possible candidates for the site of ET
Dr. Istvan Racz
16/10/09, 10:30
36. Gravity gradient noise: estimates and reduction strategies
Giancarlo Cella (PI)
16/10/09, 11:30
37. GGN subtraction in homogeneous media
Dr. Jan Harms
16/10/09, 11:50
39. FEA of GGN for subterranean gravitational wave detectors
Dr. Mark beker
16/10/09, 12:10
38. Sensing and subtraction of GGN
Dr. David Rabeling
16/10/09, 12:25
40. Aspects of seismic noise detection for GGN suppression
Dr. Riccardo DeSalvo
16/10/09, 12:40
42. Conclusive remarks
Dr. Harald Lueck (AEI Hannover (MPI f. gravitational Physics / Inst. f. Grav.physics Leibniz Uni Hannover))
16/10/09, 13:00
8. Grid computing for ET
Dr. Gergely Debreczeni (MTA KFKI RMKI)
2. IMBH binaries and ET
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