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Niels Bohr Institute Copenhagen University Eugene PolzikLECTURE 3
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Einstein-Podolsky-Rosen (EPR) entanglement Experimental techniques for observing quantum noise and entanglement Light Photon statistics – dc measurements Entanglement in the spectral modes of light – ac measurements Atoms Addition of magnetic field – ac measurements with atoms Generation of Entangled state of two distant Atomic Objects
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Einstein-Podolsky-Rosen paradox – entanglement; 1935 2 particles entangled in position/momentum L Simon (2000); Duan, Giedke, Cirac, Zoller (2000) Necessary and sufficient condition for entanglement
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2 particles entangled in position/momentum L What does it mean in practice? 1.Prepare many identical pairs of particles 2.Measure X 1 - X 2 on some of those pairs 3.Measure P 1 +P 2 on others 4.Plot statistical distributions of the results 5.Measure the width of these distributions L X 1 - X 2 0 P 1 + P 2 (X 1 - X 2 ) (P 1 + P 2 )
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Why does it make sense? Two independent particles Minimal symmetric uncertainties 0 P 1 + P 2 (P 1 + P 2 )= L X 1 - X 2 (X 1 - X 2 )= < Entangled state
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Position – momentum uncertainty The best optical interferometry measurement: Macroscopic object – a mirror Assume M=1mg
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Instead of two EPR particles we use Two beams of light 1998 Two atomic ensembles 2001
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Coherent state of light. Poissonian photon statistics. Delta-correlated noise. Probability of counting n photons Variance: Compare to For coherent state
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(vacuum units) Strong field A(t) Polarizing cube Polarizing cube 45 0 /-45 0 0 X coherent state 1 -1
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Phase squeezed Amplitude squeezed Quadrature operators. Squeezed light
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Single photon state
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x Polarization beamsplitter Spectral measurements of Quadrature Operators Homodyne detector RF spectrum analyzer
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x Polarization beamsplitter Spectral measurements on vacuum state (coherent state) Homodyne detector RF spectrum analyzer vacuum Delta correlated noise Flat spectrum of noise
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In real world Flat spectrum of noise Technical (classical) noise Quantum noise n > n > n > n
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Spectral measurements of Quadrature Operators Spectrum analyzer Advantage: getting rid of technical noise Same for sine modes 1 MHz
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Optical Spectrum of the strong field and the quantum field
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0,00,20,40,60,81,01,21,41,61,82,0 0,0 0,2 0,4 0,6 0,8 1,0 1,2 1,4 1,6 1,8 2,0 2,2 2,4 Atomic Quantum Noise Atomic noise power [arb. units] Atomic density [arb. units] y z Measuring rotating spin states
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300000310000320000330000340000 0,0000 0,0002 0,0004 0,0006 0,0008 Shot noise level Noise power [arb. units] Frequency (Hz) Density [arb. units] ---------------------------------- 1.00±0.02 0.56±0.01 0.21±0.01, Probe polarization noise spectrum Larmor frequency 320kHz Detecting quantum projections of the spin in rotating frame Atomic density (a.u.) 1.0 0.5 0.2 RF frequency z B probe y
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Einstein-Podolsky-Rosen paradox – entanglement; 1935 2 particles entangled in position/momentum L Simon (2000); Duan, Giedke, Cirac, Zoller (2000) Necessary and sufficient condition for entanglement
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10 12 spins in each ensemble yz x yz x Spins which are “more parallel” than that are entangled Experimental long-lived entanglement of two macroscopic objects. B. Julsgaard, A. Kozhekin and EP, Nature, 413, 400 (2001)
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X Z or Y 2nd 1st If the two macroscopic spins are collinear they must be entangled: Compare
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Stern-Gerlach projection on any axis to x: 1 21+2 JJ J Along y,z: ideally no misbalance between heads and tails of the two ensembles, or, at least, less than random misbalance
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10 12 atoms in each ensemble 2 gas samples 6S 1/2 Cesium )3,...,3( m 4 3
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Total z and y components of two ensembles with equal and opposite macroscopic spins can be determined simultaneously with arbitrary accuracy xx y z z Therefore entangled state with Can be created by a measurement Top view: Parallel spins must be entangled
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How to measure the total spin projections? Send off-resonant light through two atomic samples Measure polarization state of light Duan, Cirac, Zoller, EP 2000
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pump pump Y Z Z Y Entangling beam Polarization detection Entangled state of 2 macroscopic objects J1J1 J2J2 B B
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Establishing the entanglement bound Two independent ensembles Minimal symmetric uncertainties 0 Jy 1 + Jy 2 0 Jz 1 + Jz 2
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S p e c t r a l v a r i a n c e o f t h e p r o b e p u l s e Collective spin of the atomic sample J x [10 ] 0246 0 10 20 30 40 12 CSS Entanglement criterion: =
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0 Jy 1 + Jy 2 0 Jz 1 + Jz 2 Entangled state < Proving the entanglement condition:
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B-field PBS Time Verifying pulse Entangling pulse 0.5 ms m=4 700MHz 6S 6P Entangling and verifying beams S Entangling and verifying pulses F=3 F=4 = 325kHz m=4 1/2 3/2 y out x2 Optical pumping Pumping beams J x1 + J - 0,00,20,40,60,81,01,21,41,61,82,0 0,0 0,2 0,4 0,6 Atomic density [arb. units]
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Entangled spin states Create entangled state and measure the state variance Julsgaard, Kozhekin, EP Nature 413, 400 (2001).
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Material objects deterministically entangled at 0.5 m distance Niels Bohr Institute December 2003 0246810121416 0,70 0,75 0,80 0,85 0,90 0,95 1,00 10-12- 2003/noise.opj Atom/shot(comp) / PN Mean Faraday angle [deg] Quantum uncertainty
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Decoherence issues only collective spin states are entangled particles are indistinguishable - high symmetry of the system – - robustness against losses. This is not a Schrodinger’s cat made of 10 12 atoms! no free lunch: limited capabilities compared to ideal maximal entanglement Sources of decoherence: stray magnetic fields decoherence time 3 milliseconds collisions decoherence time 1-2 milliseconds
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Realism – two noncommuting spin components cannot be measured – therefore do not exist? But can be entangled Non-locality – two entangled macroscopic objects can be used to violate Bell-type inequalities via distillation All entangled Gaussian two-mode states are distillable (Giedke et al)
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