Direct observations of thermal fluctuations at sub-shot noise levels

Similar documents
Quantum Mechanical Noises in Gravitational Wave Detectors

Phys 531 Lecture 27 6 December 2005

UNIVERSITY OF SOUTHAMPTON

Quantum enhanced magnetometer and squeezed state of light tunable filter

Enhancing sensitivity of gravitational wave antennas, such as LIGO, via light-atom interaction

Chapter 2 Correlation Force Spectroscopy

Squeezed Light for Gravitational Wave Interferometers

X-ray Intensity Fluctuation Spectroscopy. Mark Sutton McGill University

Squeezing manipulation with atoms

Single Emitter Detection with Fluorescence and Extinction Spectroscopy

File name: Supplementary Information Description: Supplementary Figures, Supplementary Notes and Supplementary References

Study of a quantum nondemolition interferometer using ponderomotive squeezing

A Guide to Experiments in Quantum Optics

Digital Holographic Measurement of Nanometric Optical Excitation on Soft Matter by Optical Pressure and Photothermal Interactions

Quantum optics and squeezed states of light

Two-Stage Chirped-Beam SASE-FEL for High Power Femtosecond X-Ray Pulse Generation

Frequency dependent squeezing for quantum noise reduction in second generation Gravitational Wave detectors. Eleonora Capocasa

Survey on Laser Spectroscopic Techniques for Condensed Matter

Quantum Noise in Mirror-Field Systems: Beating the Standard Quantum IARD2010 Limit 1 / 23

Temperature ( o C)

Lecture 9. PMTs and Laser Noise. Lecture 9. Photon Counting. Photomultiplier Tubes (PMTs) Laser Phase Noise. Relative Intensity

Decoherence and the Classical Limit

A classical corpuscular approach to optical noise Philippe Gallion Abstract

Astronomy 203 practice final examination

PART 2 : BALANCED HOMODYNE DETECTION

Optical Frequency Comb Fourier Transform Spectroscopy with Resolution beyond the Path Difference Limit

Let us consider a typical Michelson interferometer, where a broadband source is used for illumination (Fig. 1a).

Optical Coatings and Thermal Noise in Precision Measurements

Squeezed states of light - generation and applications

Two-electron systems

Interference- Michelson Interferometer. Interference lecture by Dr. T.Vishwam

The Hanbury Brown Twiss effect for matter waves. Chris Westbrook Laboratoire Charles Fabry, Palaiseau Workshop on HBT interferometry 12 may 2014

Interferometric. Gravitational Wav. Detectors. \p World Scientific. Fundamentals of. Peter R. Sawlson. Syracuse University, USA.

Thermal Emission in the Near Field from Polar Semiconductors and the Prospects for Energy Conversion

Efficient Generation of Second Harmonic Wave with Periodically. Poled MgO:LiNbO 3

Laboratory 3&4: Confocal Microscopy Imaging of Single-Emitter Fluorescence and Hanbury Brown and Twiss setup for Photon Antibunching

The Truth about diffusion (in liquids)

Relic Gravitons, Dominant Energy Condition and Bulk Viscous Stresses

The structure of laser pulses

CORRELATION BETWEEN PHOTONS IN TWO COHERENT BEAMS OF LIGHT

QND for advanced GW detectors

PHY 481/581. Some classical/quantum physics for the nanometer length scale.

Measurement of liquid surface properties by laser-induced surface deformation spectroscopy

Problem Set: TT Quantum Information

Anti-Bunching from a Quantum Dot

Fourier Transform Infrared Spectrometry

Interference. Reminder: Exam 2 and Review quiz, more details on the course website

Expressions for f r (T ) and Q i (T ) from Mattis-Bardeen theory

Effect of Liquid Viscosity on Sloshing in A Rectangular Tank

Recent progress in SR interferometer

Optics, Light and Lasers

Lecture 9: Introduction to QM: Review and Examples

EUV Reflectivity measurements on Acktar Sample Magic Black

LIGO s Thermal Noise Interferometer: Progress and Status

Confocal Microscopy Imaging of Single Emitter Fluorescence and Hanbury Brown and Twiss Photon Antibunching Setup

College Physics 10th edition

Laser Dissociation of Protonated PAHs

Note the diverse scales of eddy motion and self-similar appearance at different lengthscales of the turbulence in this water jet. Only eddies of size

II Relationship of Classical Theory to Quantum Theory A Quantum mean occupation number

Lasers & Holography. Ulrich Heintz Brown University. 4/5/2016 Ulrich Heintz - PHYS 1560 Lecture 10 1

Corrections to A Guide to Experiments in Quantum Optics

Lab 3-4 : Confocal Microscope Imaging of Single-Emitter Fluorescence and Hanbury-Brown and Twiss Set Up, Photon Antibunching

Constructive vs. destructive interference; Coherent vs. incoherent interference

MODERN OPTICS. P47 Optics: Unit 9

Optics.

High-Resolution Imagers

Michelson Interferometer

Where are the Fringes? (in a real system) Div. of Amplitude - Wedged Plates. Fringe Localisation Double Slit. Fringe Localisation Grating

SUPPLEMENTARY INFORMATION

4 Classical Coherence Theory

How can x-ray intensity fluctuation spectroscopy push the frontiers of Materials Science. Mark Sutton McGill University

Homework 1. Property LASER Incandescent Bulb

Supplementary Figures

Lecture 2: Open quantum systems

Verification of conditional quantum state in GW detectors. LSC-VIRGO Meeting, QND workshop Hannover, October 26, 2006

Status and Prospects for LIGO

IMPROVED QUANTUM MAGNETOMETRY

3. Excitation and Detection of Fluorescence

GRAVITATIONAL WAVE SOURCES AND RATES FOR LISA

Labs 3-4: Single-photon Source

LONG-LIVED QUANTUM MEMORY USING NUCLEAR SPINS

SWOrRD. For direct detection of specific materials in a complex environment

Low-coherence heterodyne photon correlation spectroscopy

Advanced Virgo and LIGO: today and tomorrow

Quantum Optics in Wavelength Scale Structures

The Hanbury Brown and Twiss effect: from stars to cold atoms

Michelson Interferometer. crucial role in Einstein s development of the Special Theory of Relativity.

Noise in voltage-biased scaled semiconductor laser diodes

The gravitational wave detector VIRGO

One- and two-particle microrheology in solutions of actin, fd-virus and inorganic rods

Fiber Gratings p. 1 Basic Concepts p. 1 Bragg Diffraction p. 2 Photosensitivity p. 3 Fabrication Techniques p. 4 Single-Beam Internal Technique p.

Advanced Workshop on Nanomechanics September Quantum Measurement in an Optomechanical System

The Large Amplitude Oscillatory Strain Response of Aqueous Foam: Strain Localization and Full Stress Fourier Spectrum

Solution structure and dynamics of biopolymers

New directions for terrestrial detectors

Simple strategy for enhancing terahertz emission from coherent longitudinal optical phonons using undoped GaAs/n-type GaAs epitaxial layer structures

X-Ray Scattering Studies of Thin Polymer Films

DIGITAL CORRELATION OF FIRST ORDER SPACE TIME IN A FLUCTUATING MEDIUM

Correlation functions in optics; classical and quantum 2. TUW, Vienna, Austria, April 2018 Luis A. Orozco

Supplementary Information: Three-dimensional quantum photonic elements based on single nitrogen vacancy-centres in laser-written microstructures

Transcription:

Direct observations of thermal fluctuations at sub-shot noise levels 2012 T. Mitsui, K.A., Phys. Rev. E 80, 020602(R)-1 4 (2009) Phys. Rev. E 86, 011602 (2012) arxiv:1206.3828

Contents 1. Thermal fluctuations 2. Liquid surface fluctuations and their properties 3. Shot noise 4. Noise reduction 5. Surface height fluctuation measurements 6. Surface inclination fluctuation measurements 7. Discussion 1

Thermal fluctuations Thermal fluctuation phenomena: surfaces, Brownian motion, liquid surfaces, solid Thermal fluctuations are ubiquitous! Directly observe thermal fluctuations of common materials in an everyday environment. Fluctuations are small! noise! Measure at hitherto unseen low noise levels Test theory to previously unachieved precision. Observe new phenomena. 2

Liquid surface fluctuations Ripplons Typical thermal fluctuation phenomena which is relatively well understood. Liquid surfaces fluctuate thermally. (von Schmoluchowski, 1908; Mandelstam, 1913) Experimentally observed effectively as gratings. (Katyl, Ingard, 1967) Will not work for viscous liquids Size of fluctuations atomic scale z 2 k BT 4πσ log σ (0.4 nm)2 (σ gρl2 : surface tension, l: molecular scale) 3

Properties of thermal surface fluctuations Surface fluctuation properties determined from hydrodynamics. Interesting fundamental physics. Thermal fluctuation spectral properties known. Important test! Spectral function: (Bouchiat, Meunier, 1971) Analytic, but behavior not simple. (ρ: density, σ: surface tension, η: viscosity) P (k, ω) = k BT πω kτ 2 0 ρ Im [ (1 + s) 2 + y 1 + 2s ] 1 s iωτ 0, τ 0 ρ σρ 2ηk2, y 4η 2 k 4

P(k,2πf) [m 4 /Hz] 10-30 10-35 10-40 10-45 10-50 10 3 10 4 10 5 10 6 10 7 10 8 k [m -1 ] Low dissipation η 3 ω/(ρσ 2 ) < 1/(8 2) Compare with simple analytic behavior (black, dotted) 2 regions. Peak behavior disappears for higher ω Viscous f = 10 3, 10 5, 10 7 [s 1 ] P (k, ω) k BT π ) 1/3 ( 4ηk 3 ρω 2 k < 2 1/6 k ρ 2 ω 4 R (ω), k R (ω) σ 2η k > 2 1/6 k σ 2 k 3 R (ω) 5

P(k,2πf) [m 4 /Hz] 10-32 10-34 10-36 10-38 10-40 10-42 10-44 10-46 10-48 10-50 10 3 10 4 10 5 10 6 10 7 10 8 k [m -1 ] Highly dissipative case η 3 ω/(ρσ 2 ) > 1/(8 2) No peaks viscous Leading order behavior 3 regions, simple. f = 10 3, 10 5, 10 7 [s 1 ] P 0 (k, ω) = k BT π 4ηk 3 ρω k < 2 1/4 ρ 2 ω 4 2η 1 ρω 2 1/4 2ηkω 2 2η < k < 2ηω σ 6 2η σ 2 k 3 k > 2ηω σ

Measure surface fluctuations directly. Characterize the fluctuations spectra. Fluctuations too small to examine precisely. Noise, esp. shot noise 7

Shot noise Essentially quantum noise. Randomness of photon arrival times. Photoconversion noise in current ( I) 2 = 2eI f White noise (f independent). Unavoidable in photoconversion (cf. gravitational wave detection). quantum non- Reduce shot noise Squeezed light ( 1/2 so far), demolition(?). 8

Noise reduction A measurement: D 1 = S + N 1, S: signal, N 1 : noise S has no known periodicity ( eg. thermal fluctuations). Power spectrum: ( D 1 Fourier transform of D 1 ) D 1 2 = S 2 + Ñ1 2 Impossible to separate S, N 1 even in theory 9

Noise reduction A measurement: D 1 = S + N 1, S: signal, N 1 : noise S has no known periodicity ( eg. thermal fluctuations). Power spectrum: ( D 1 Fourier transform of D 1 ) D 1 2 = S 2 + Ñ1 2 Impossible to separate S, N 1 even in theory Make multiple measurements: D 1,2 = S + N 1,2 D 1 D2 S 2, N relative error 1/ N Uncorrelated noise statistically reduced. 9

Comments on the noise reduction method Simple! at least in theory Principle not limited to optical or surface measurements. Noise needs to be uncorrelated. crucial Any uncorrelated noise eliminated: Shot noise, AM noise, amplification noise, FM noise, directional fluctuations,. In practice, 10 3 reduction achieved. 10

Practical limitations of the noise reduction method Always applicable, but efficacy depends on the properties of the signal. Noise elimination statistical. Reltative reduction: 1/ N. Given f (frequency resolution), N = ft. (T : total measurement time). f = 1 MHz, noise reduction factor 10 3 T = 1 s. Roughly speaking, need many periods of the wave component for the method to be effective. 11

Surface height fluctuation measurements Basic setup Michelson interferometer, except for photodetection and data processing. applicable to any Michelson measurement Laser: 532 nm wavelength, 0.5 mw at sample, reference. Sample size: 0.96 µ m. 2.2 mm, beam diameter: Sample surface reflectivity few %. (water: 2 %, oil: 4 %) 12

Observed spectrum (summed over k, b: beam diameter): S(f) = 2 ã 0 (ω) 2 = 2 0 dk ke b2 k 2 /8 P (k, 2πf), a 0 : average height Uniquely determined, given the liquid properties (ρ, σ, η) and b. Sample size: long distance cutoff. Beam size: short distance cutoff (averages within the beam spot). 13

10-22 10-23 water surface spectrum S h [m 2 /Hz] (water) 10-23 10-24 10-25 10-26 10-27 10-28 10-29 10-30 ethanol water shot noise level (theory) 10 3 10 4 10 5 10 6 10 7 f [Hz] 10-24 10-25 10-26 10-27 10-28 10-29 10-30 10-31 S h [m 2 /Hz] (ethanol) ethanol surface spectrum Single signal shot noise Theoretical prediction! Theoretical shot noise level Good agreement, some lens aberration effects. 10 3 below shot noise level! Perfect agreement for water. Almost perfect for ethanol, very slight deviations at high frequencies. 14

S h [m 2 /Hz] 10-23 10-24 10-25 10-26 10-27 10-28 10-29 10-30 10 3 10 4 10 5 10 6 10 7 f [Hz] δα 0.105 0.1 0.095 0.09 0.085 0.08 0.075 0.07 0.065 0.06 0.055 290 300 310 320 330 340 350 Oil surface fluctuations: T = 21, 30, 59, 74 C. Good agreement, slight deviation at high frequencies. Mismatch larger for smaller T. Deviation: S h (f) f α, δα = C exp(u/k B T ), U = 7 kj/mol latent heat. T [K] 15

Quantum Optics Single light source: Classically, difficult to imagine uncorrelated noise from a single source. Photon arrival times are random in the coherent state. Photons partitioned at the mirror shot noise in the 2 detectors uncorrelated. Will not work with squeezed light (shot noise in two measurements correlated). 16

Surface inclination fluctuation measurements Basic concept: Surface = optical lever. Measure the fluctuation spectrum of the inclination. Dual PD for an inclination measurement. 2 Dual PD for correlation measurement Noise reduction Observed spectrum: S(f) = 0 dk k 3 e b2 k 2 /8 P (k, 2πf) 17

P(2πf) [rad 2 /Hz] 10-11 10-12 10-13 10-14 10-15 10-16 10-17 10-18 10-19 f -2 f -1 α 1000 10000 100000 f [Hz] 2 1.8 1.6 1.4 1.2 1 1 10 100 1000 t [min] Time dependent spectra Epoxy adhesive example. Gradually hardens Spectra S(f) f α, α: time dep. α : 2 1 f 2 : Viscous liquid surface f 1 : Solid surface Why? α(t)? 18

Discussion Directly measured surface thermal fluctuation spectra of ordinary materials at ordinary temperatures (simple liquids, biological materials, complex fluids, polymers, ) Modification to standard measurements minimal broad area of application Noise reduction: not limited to optical, surfaces, thermal fluctuations. Achieved 10 3 reduction or more. Small power 0.5 mw, small sample size few µm, short measurement time few sec. wide applicability 19

To do: Understand surface fluctuation properties of various materials. Applications in other areas, other than optical, surfaces measurements. More to come 20