'Signal recycling' presentation slideshows

Kazuhiro Yamamoto Henning Kaufer, Tobias Westphal, Daniel Friedrich, Helge Mueller-Ebhardt,

Radiation Pressure Noise Experiment in Hannover. Kazuhiro Yamamoto Henning Kaufer, Tobias Westphal, Daniel Friedrich, Helge Mueller-Ebhardt, Stefan Gossler, Karsten Danzmann and Roman Schnabel Max-Planck-Institut fuer Gravitationsphysik (Albert-Einstein-Institut)

731 views • 60 slides

579 views • 47 slides

Title

568 views • 41 slides

Title

414 views • 41 slides

Experiences and lessons learned from interferometer simulations at GEO

GWADW, 22.05.2013. Experiences and lessons learned from interferometer simulations at GEO. Andreas Freise for Hartmut Grote, Holger Wittel and the rest of the GEO 600 team LIGO-G1300578. Quick + Dirty Simulations. Quick!. Quick means: You can do the simulation

524 views • 38 slides

GEO 600 STATUS

432 views • 33 slides

Beam shaping for thermal noise reduction

469 views • 32 slides

Opening the Gravitational Wave Window

417 views • 29 slides

Selim Shahriar, Northwestern University

LIGO G0900207. Design constraints and optimization for a white light cavity based GW interferometer including power and signal recycling. Selim Shahriar, Northwestern University. Laboratory of Atomic and Photonic Technologies. URL: http://lapt.ece.northwestern.edu.

407 views • 29 slides

Dual Recycling in GEO 600

395 views • 29 slides

Future LIGO Interferometers

Future LIGO Interferometers. Moriond 07 La Thuille, Italy. Rana Adhikari Caltech. Advanced LIGO. LIGO mission: detect gravitational waves and initiate GW astronomy Next detector Should have assured detectability of known sources

569 views • 26 slides

Homodyne readout of an interferometer with Signal Recycling

Homodyne readout of an interferometer with Signal Recycling. Stefan Hild for the GEO600 team October 2007 LSC-Virgo meeting Hannover. Motivation for DC-readout (1). Disadvantages. Increased coupling of laser power noise. Usually an output mode cleaner (OMC) is required.

355 views • 26 slides

Homodyne readout of an interferometer with Signal Recycling

Homodyne readout of an interferometer with Signal Recycling. Stefan Hild for the GEO600 team October 2007 LSC-Virgo meeting Hannover. Motivation for DC-readout (1). Disadvantages. Increased coupling of laser power noise. Usually an output mode cleaner (OMC) is required.

357 views • 26 slides

The GEO 600 Detector

The GEO 600 Detector. Andreas Freise and the GEO 600 Team University of Hannover May 20, 2002. GEO. LIGO. VIRGO. TAMA. ACIGA. Location of GEO 600. the gallery in the central building. the clean room. t he cen t ral area. North Arm 600 m. the trench with vacuum tube. East Arm

422 views • 23 slides

Setting the Stage Dave Reitze LIGO Laboratory

GWADW: Gravitational Wave Detectors for 2015, 2020, and 2025. Setting the Stage Dave Reitze LIGO Laboratory. http://surfing-place.blogspot.com/2011/06/hawaii.html. Ground- based Detectors-- Past, Present, & Future. 2010 -- First Generation Interferometers:

320 views • 14 slides

Advanced LIGO

348 views • 14 slides

Advanced LIGO

149 views • 14 slides