ignore
Aspen2003
ignore
general information
program
registration
participants
announcements
presentations
contact us
Program (02.08.2003)
 printable version

Monday, February 3
AM: Why and How to Go Beyond 2KHz and Below 10Hz I

Convenors: E. Coccia, S. Finn
08:00 S. Meshkov (CIT)
J. Kelly (ACP)
Welcome
08:10 S. Finn (Penn State) Between and Beyond: Sources and Science
08:35 Discussion
08:40 V. Kalogera (NWU) NS-WD Event Rates Relevant to GW Frequencies Below 10 Hz
09:05 Discussion
09:10 Break
09:40 F. Rasio (NWU) NS-WD Mergers In-between Interferometer and LISA Bands; NS-NS Mergers with f~2 kHz
10:05 Discussion
10:10 C. Miller (U of MD) Intermediate-Mass BH and Gravitational Radiation
10:35 Discussion
10:40 D. Shoemaker (MIT) Status of Advanced LIGO
10:55 Discussion
11:00 Adjourn

Monday
PM: Why and How to Go Beyond 2KHz and Below 10Hz II

Convenors: E. Coccia, S. Finn
04:30 E. Coccia (U of Rome) Introduction
04:40 Discussion
04:45 M. Cerdonio (Padova U) Dual Detector
05:10 Discussion
05:20 A. de Waard (Leiden U) MiniGRAIL
05:45 Discussion
05:55 Break
06:20 A. Rüduger (Garching) ASTROD
06:45 Discussion
06:55 N. Seto (Osaka U) DECIGO
07:20 Discussion
07:30 Adjourn

Tuesday, February 4
AM: Strategies for Extensions to Low Frequencies I

Convenors: R. DeSalvo, N. Robertson
08:00 G. Cella (U of Pisa) Going Underground to Reduce Newtonian Noise
08:25 Discussion
08:30 S. Sato (NAOJ) Noise Experience of the 20m Run 1 km Underground in the Kamioka Mine
08:55 Discussion
09:00 Break
09:30 S. Rowan (Stanford/Glasgow U) Improving Future Interferometer Sensitivities at Low Frequencies Using Cooled Silicon
09:55 Discussion
10:00 T. Uchiyama (ICRR) Present Status of LCGT
10:25 Discussion
10:30 A. Giazotto (INFN) Some Ideas on a 4K Cryogenic Detector
10:55 Discussion
11:00 C. Hardham (Stanford) The Hydraulic External PreIsolator (HEPI)
11:25 Discussion
11:30 Adjourn

Tuesday
PM: Strategies for Extensions to Low Frequencies II

Convenors: R. DeSalvo, N. Robertson
04:30 D. Ottaway (MIT) QND
04:55 Discussion
05:00 A. Bertolini (U of Pisa) Accelerometers for Gravity Gradient Subtraction
05:25 Discussion
05:30 Break
06:00 R. DeSalvo (CIT)
K. Numata (Tokyo U)
S. Penn (Syracuse U)
Fused Silica Mirror Possibilities
06:25 Discussion
06:30 R. DeSalvo (CIT) Glassy Metal Mirror Suspensions
06:55 Discussion
07:00 W. Hua (Stanford) 3 Axis Active Suppression of Microseismic Peak
07:25 Discussion
07:30 Adjourn

Wednesday, February 5
AM: Strategies for Extensions to High Frequencies I

Convenor: F. Fidecaro
08:00 F. Fidecaro (U of Pisa) Overview
08:25 Discussion
08:30 M. Fejer (Stanford) Diffractive Optics
08:55 Discussion
09:00 Break
09:20 R. Schnabel (U of Hanover) Squeezed Light, Entanglement, and Teleportation
09:45 Discussion
09:50 W. Kells (CIT) Thermal Lensing in LIGO
10:15 Discussion
10:20 A. Melissinos (Rochester U) Search for High Frequency Signals at the Hanford 4K IFO
10:35 Discussion
10:40 G. Sanders (CIT) What Should Drive the Rest of Workshop
11:05 Discussion
11:15 Adjourn

Wednesday
PM: Strategies for Extensions to High Frequencies II

Convenor: F. Fidecaro
04:30 B. Schutz (U of Potsdam) TBA
04:55 Discussion
05:05 B. Berger (NSF) The View from NSF
05:30 Discussion
05:40 F. Menzinger (EGO) The View from EGO
05:50 Discussion
06:00 Adjourn
Public lecture, Wheeler Opera House
Chair: S. Meshkov
08:00 S. Finn Gravitational Waves: From Black Holes to Light Waves to a New Astronomy

Thursday, February 6
AM: Lowering the Sensitivity Floor I

Convenor: TBD
08:00 T. Tomaru (KEK) Cooling System in a Cryogenic Interferometer
08:25 Discussion
08:30 J.-M. Courty (Lab Kastler Brossel) Improvement of Interferometer Sensitivity by Quantum Locking of Mirrors
08:55 Discussion
09:00 Break
09:30 S. Wise (U of FL) Inclusion of a Line-Broadening Element in Fabry-Perot Cavities
09:55 Discussion
10:00 G. Billingsley (CIT) TBD
10:25 Discussion
10:30 R. Schnabel (U of Hanover) Squeezed Light Enhanced Michelson Interferometers
10:55 Discussion
11:00 Adjourn

Thursday
PM: Advances in Critical Areas I

Convenor: A. Rüdiger
04:30 M. Tinto (JPL) Optimal Time-Delay Interferometry for LISA
04:55 Discussion
05:00 A. Krolak (JPL) On LISA Signal Resolution
05:25 Discussion
05:30 Break
06:00 J. Camp (GSFC) LISA R&D
06:25 Discussion
06:30 M. te Plate (ERA/ESTEC) LISA Technology Package
06:55 Discussion
07:00 A. Kuhnert (JPL) Progress on the ST7 Interferometer
07:25 Discussion
07:30 Adjourn

Friday, February 7
AM: Lowering then Sensitivity Floor II

Convenor: J. Hough
08:00 S. Penn (Syracuse U) Achieving Low Thermal Noise in Fused Silica: New advances and New Challenges
08:25 Discussion
08:30 P. Sneddon (Glasgow U) Mechanical Loss Measurements Relevant to Present and Future Detectors
08:55 Discussion
09:00 Break
09:25 K. Yamamoto (Tokyo U) Coating Q Factors vs Temperature
09:50 Discussion
09:55 K. Numata (Tokyo U) Observation of the Thermal and Thermoelastic Noise Floor in BK7 and Fluorite Mirrors
10:20 Discussion
10:25 A. Gretarsson (LLO) Monitoring Excess Noise in Suspension Fibres
10:50 Discussion
10:55 K. Numata (Tokyo U) Frequency Behaviour of Mechanical Q Factor of GWI Mirrors
11:20 Discussion
11:25 Adjourn

Friday
PM: Advances in Critical Areas II

Convenor: TBD
04:30 A. Takamori (Tokyo U) Seismic Attenuation/Suspension Experiment
04:55 Discussion
05:00 G. Gemme (U of Genoa) Parametric Frequency Converter for GW Detection
05:25 Discussion
05:30 Break
06:00 M. Benacquista (MT St U) Sources in the Medium Frequency Band
06:25 Discussion
06:30 R. Matzner (U of TX) TBA
06:55 Discussion
07:00 H. Cuesta (Brazilian Centre for Physics) Bursts of GW from Neutrino Oscillations
07:25 Discussion
07:30 Adjourn

Saturday, February 8
AM: Summary

Convenor: TBD
08:00 R. DeSalvo (CIT) Round Table: Mirrors and Mirror Suspensions
08:25 Discussion
08:35 TBD TBA
09:00 Discussion
09:10 Break
09:40 J. Hough (Glasgow U) Conference Summary
10:10 Conference Adjourns

ignore
LIGO home


webmaster
02.11.2003
© California Institute of Technology