'Test masses' diaporamas de présentation

Advanced LIGO Systems Requirements Review

Advanced LIGO Systems Requirements Review. 3 July 2001. Agenda. Systems requirements & design, 1 hr (Peter F) Optical layout, 20 min (Dennis C) Generic requirements & standards, 10 min (Dennis C) LIGO Observatory environments, 20 min (David S) Summary. Outline for systems design.

726 views • 60 slides

Atomic Clocks as Detectors of Gravitational Waves

Atomic Clocks as Detectors of Gravitational Waves. Sergei Kopeikin University of Missouri, USA. Plan of lecture:. Gravitational wave spectrum and detectors Accuracy and stability of clock oscillators Pulsar clock as GW detector Computation of GW signal

436 views • 43 slides

Advanced LIGO

Advanced LIGO. 5 July 2012. David Shoemaker For the LIGO Scientific Collaboration. Advanced LIGO. Goal: open the era of gravitational-wave astronomy through the direct detection of gravitational waves. Replaces the instruments at the Washington and Louisiana sites

580 views • 35 slides

The search for gravitational waves with the new generation of interferometers

The search for gravitational waves with the new generation of interferometers. Peter R. Saulson Syracuse University LIGO-G030345-00-Z. Outline. 1. Gravitational waves and how to detect them 2. The new generation of interferometric detectors 3. Sample of first results.

434 views • 34 slides

Gravitational Wave Detection #2: How detectors work

Gravitational Wave Detection #2: How detectors work. Peter Saulson Syracuse University. Outline. How does an interferometer respond to gravitational waves? How does a resonant bar respond to gravitational waves?

436 views • 28 slides

Anna Nobili (University of Pisa & INFN) for the GG/GGG collaboration FPS-06 , LNF March 21-23 2006

396 views • 26 slides

Ho Jung Paik University of Maryland GW Astronomy, Korea August, 2016

Terrestrial Tensor GW Detector Based on Superconducting Instrumentation. Ho Jung Paik University of Maryland GW Astronomy, Korea August, 2016. GW detector bandwidths. Missing frequency band.

223 views • 22 slides

San Andreas Fault

P-Wave. S-Wave. S-P time. Detection of transient earthquake gravity signals using superconducting gravity gradiometer. San Andreas Fault. Ho Jung Paik University of Maryland E-GRAAL January 10, 2018. Blind zones of EEWS. US West Coast earthquake hazard.

232 views • 21 slides

Searching for gravitational waves with lasers

Searching for gravitational waves with lasers. Rick Savage Caltech LIGO Hanford Observatory - Richland, WA. Black holes and time warps. Sept 1974 - transferred to UCLA in Physics Jan 1975 - started working for F. Chen and N. Luhmann as undergraduate lab assistant (with Doug Cook)

557 views • 20 slides

A particle monitor for LISA Pathfinder and Gravity Probe-B gyroscope charging in LEO

328 views • 16 slides

GSFC ? JPL

263 views • 15 slides

Non-contact mode excitation of small structures in air using ultrasound radiation force Acoustical Society of America Me

Non-contact mode excitation of small structures in air using ultrasound radiation force Acoustical Society of America Meeting: May 17, 2005. Thomas M. Huber, John Purdham Physics Department, Gustavus Adolphus College Mostafa Fatemi, Randy Kinnick, James Greenleaf

349 views • 14 slides

Overview of Advanced LIGO

Overview of Advanced LIGO. David Shoemaker PAC meeting, NSF Review 5 June 2003, 11 June 2003. Advanced LIGO. LIGO mission: detect gravitational waves and initiate GW astronomy Next detector Must be of significance for astrophysics

141 views • 14 slides

Ho Jung Paik University of Maryland GW Astronomy, Korea August, 2016

Mitigation of Newtonian Noise Using Superconducting Gravity Gradiometer. Ho Jung Paik University of Maryland GW Astronomy, Korea August, 2016. Newtonian gravity noise. Seismic and atmospheric density modulations cause Newtonian gravity gradient noise (NN) , which cannot be shielded.

134 views • 13 slides

Entanglement between test masses

227 views • 12 slides

Paul McNamara on behalf of the LISA Pathfinder Science Working Team

Paul McNamara on behalf of the LISA Pathfinder Science Working Team.

137 views • 1 slides