Quantum Optics and Macroscopic Quantum Measurement LIGO Laboratory, MIT
What we are about Precision interferometry (for gravitational wave detection) beyond the quantum limit Manipulating macroscopic objects such as the mirrors of the interferometer using the quantum properties of light Measuring quantum state of macroscopic objects
The LIGO group at MIT is ~25 people Who we are... The LIGO group at MIT is ~25 people 5 faculty and senior research scientists ~10 scientists, post-docs and engineering staff ~10 graduate students The Quantum Measurement group Corbitt, Goda, Wipf, Pelc, Zaheer Innerhofer, Mikhailov Nergis Lab visit/tour Friday 10am in NW17
The ‘Standard Quantum Limit’ How precisely can we measure the position of a particle using light? Quantum fluctuations on the light (shot noise) Use N photons in the measurement Get sqrt(N) uncertainty Back action (radiation pressure noise) Photon impart momentum to the particle Fluctuations in photon number gives uncertainty in position of the particle
Some (sub-)quantum states of light Analogous to the phasor diagram Stick dc term Ball fluctuations Common states Coherent state Vacuum state Amplitude squeezed state Phase squeezed state McKenzie
Radiation-pressure-induced Squeezing
The principle A “tabletop” interferometer that generates squeezed light Use radiation pressure as the squeezing mechanism Intensity fluctuations of the light push on the mirror Mirror motion imprinted on phase of the light Amplitude and phase correlations squeezing Relies on intrinsic quantum physics of optical field-mechanical oscillator correlations Quantum radiation pressure squeezing sub-SQL
The Ponderomotive Interferometer
High circulating laser power High-finesse cavities Key ingredients High circulating laser power 10 kW High-finesse cavities 15000 Light, low-noise mechanical oscillator mirror 1 gm with 1 Hz resonant frequency Optical spring Detuned arm cavities
Noise budget
Why is this interesting/important? First ever (?) demonstration of radiation-pressure induced squeezing Probes quantum mechanics of optical field-mechanical oscillator coupling at 1 g mass scales Test of low noise optical spring Suppression of thermal noise Simulations and techniques useful for precision interferometry (e.g. GW interferometers) Quantum optical simulation package Michelson detuning Role of feedback control in these quantum systems Quantum decoherence tests