'Laser noise' diaporamas de présentation

A look at interferometer topologies that use reflection gratings

A look at interferometer topologies that use reflection gratings. Peter Beyersdorf Stanford University. Spring 2005 LSC meeting G050171-00-Z. Outline. Motivation for considering reflection gratings Configurations that use gratings Reflective RSE

548 views • 43 slides

Synthetic LISA simulating time-delay interferometry in a model LISA

Synthetic LISA simulating time-delay interferometry in a model LISA. (presenting) Michele Vallisneri (in absentia) John W. Armstrong LISA Science Office, Jet Propulsion Laboratory 12/17/2003. lisa.jpl.nasa.gov. Why Synthetic LISA?.

509 views • 31 slides

Laser synchronization and RF transmission over stabilized fibers

Laser synchronization and RF transmission over stabilized fibers. Russell Wilcox John Staples Larry Doolittle LCLS meeting Mar 10, 2006. Two combs can be synched by comparing two lines of each. ?? m. ?? m. master clock. frequency. transmitted frequencies. ?? m - ?? s. ?? m - ?? s.

258 views • 25 slides

Laser Noise, Decoherence &Observations in the Optimal Control of Quantum Dynamics

Laser Noise, Decoherence &Observations in the Optimal Control of Quantum Dynamics. ? ?. Department of Chemistry, Princeton University. Frontiers of Bond-Selective Chemistry. Rabitz Group in Princeton. Effect of environments on control of Quantum Dynamics: Fighting & Cooperating

242 views • 24 slides

Abstract

Abstract.

223 views • 16 slides

Entanglement between test masses

227 views • 12 slides

Effects of laser linewidth on the back-action cooling of optomechanical resonators.

Effects of laser linewidth on the back-action cooling of optomechanical resonators. Gregory A. Phelps This work is sponsored by: UA NASA Space Grant, NSF, ARO, ONR. Introduction. Gravitational Wave Detection (LIGO) 4 kilometer interferometer. (Hartle, 339-342).

264 views • 10 slides

Effects of laser linewidth on the back-action cooling of optomechanical resonators.

Effects of laser linewidth on the back-action cooling of optomechanical resonators. Gregory A. Phelps This work is sponsored by: UA NASA Space Grant, NSF, ARO, ONR. Introduction. Gravitational Wave Detection (LIGO) 4 kilometer interferometer. (Hartle, 339-342).

207 views • 10 slides