paul c. haljan university of michigan oct. 2003. i. laser cooling atoms magnets lasers

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Paul C. Haljan University of Michigan Oct. 2003

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Page 1: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Paul C. HaljanUniversity of MichiganOct. 2003

Page 2: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

I. Laser cooling atoms

Magnets

Lasers

Page 3: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

II. Quantum Tornadoes Near Absolute Zero

Courtesy NOAA

Page 4: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Cd+Cadmium quantum bits

Page 5: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

The world circa 1920’s

Air = molecules moving around!

Atomic constituents

Light

and radio waves …..

Page 6: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Fifth Solvay Conference 1927“Electrons and photons”

Quantum Theory – “Quantum Wave Mechanics” - takes flight

Page 7: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Everyday waves: Sound waves

Source Detector

time

Pressure

Wavelength ~ 30cmat 1000Hz frequency

Page 8: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Waves can add (constructive interference)

or cancel (destructive interference)

=

=

Louder

Silent

Page 9: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Interference – you can hear it!

Page 10: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

You can see interference too.

Laser

Light intensity

Light interference: Young’s double slit experiment

Wavelength

Electromagnetic waves

Page 11: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

How about a double slit experiment for particles (atoms)?

Beam of particles

Particle Detector

Page 12: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

How about a double slit experiment for particles (atoms)?

Beam of particles

Particle Detector

Distribution is built up from

single particle detections

Page 13: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

How about a double slit experiment for particles (atoms)?

Beam of particlesSorry!

Page 14: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

How about a double slit experiment for particles (atoms)?

Beam of particles

Intensity(both slits) =I1+I2

Page 15: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Double slit experiment for particles

Interference!!!!

electrons atoms

HitachiCarnal, Mlynek 1991

Page 16: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

If only one particle at a time passes through

the interferometer …..

an interference pattern still builds up!!!!

“click”

Intensity pattern shows upAfter many particles detected

Page 17: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

So what’s interfering?

LouisdeBroglie

= de Broglie wavelength

h = Planck’s constant (tiny)

m = mass

v = particle velocity

McEvoy & Zarate

h

mv

Page 18: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Schrödinger’s Equationfor quantum wave mechanics

McEvoy & Zarate

wavefunction

x,t2 probabilityof finding particleat position xat time t.

Page 19: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Particle interferometry with ever bigger, more complex objects!

• (Photons) 0• Electrons – 1950’s 0.0005• Neutrons 1975 1• Atoms 1991 10-100• Buckyballs and biomolecules 2003 >1000

C44H30N4 C60F48

h

mv

Mass / proton mass

de Broglie wavelength

Page 20: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Cold - the quantum frontier!

h

mvde Broglie wavelength

Temperature(random jiggling)

Thermal velocity

de Broglie wavelength

hot fastcold slow

Gas

BIG!

Page 21: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

How cold is cold?

Thermal velocity

de Broglie wvlen. (microns)

Temperature

Florida

Air liquifies

Triton

0 -460

100 -269

200 -99

300 +81

Absolute zero – all motion stops

Record low (Antartica)

Michigan winter

Outer space (3K)

Absolute (Kelvin)

Fahrenheit (degrees)

Temp.

300 K 300m/s 1x10-5

300 K 30cm/s 0.01300 nK 1cm/s 1

1nK=0.000 000 001 K

Rubidium atom

virus

E-coli

Page 22: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Lasers zap, burn, cut

How do they COOL atoms????

Page 23: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Pushing atoms with light

Rb

Acceleration 100 000 g’s!!!!

Page 24: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

It’s a bit harder than that …..An atom only absorbs specific colors.

(explained by quantum theory).

The laser for Rubidium atoms is a deep red. “Lowest A”

Atom is reallyspecific!!!A single key ona 26 million keypiano!!!!

Page 25: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Problem: How can we stop the fast atoms without speeding up the slow ones in a gas?

Solution: Doppler effect “The color the atom absorbs depends on its velocity!”

Atom moving towards the laser scatters photons

Stopped atom doesn’t scatter

Page 26: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Laser molasses

APPLET

Page 27: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

I. Laser cooling atoms

Lasers

Page 28: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

BEC intro II

JILA Mark III

Page 29: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

JILA Mark III

~1 billion atoms10-100uK

Page 30: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Atom Interferometry (AI):

Page 31: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Light interferometersWave interference can be used to measure

(changes in) path length difference:

mirror mirror

Beam

splitter

Detector

Page 32: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

LIGO pict

LIGO Gravitational wave detectorHanford WA

4km

A really BIG light interferometer!

Page 33: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

de Broglie Wave Interference

Neutron interference

MICHIGAN 1975

= h/mv

= de Broglie wavelength

Particle wavepacket

Atoms (v~1m/s):

Compare with light

waves:

Shorter wavelength a more sensitive ruler!

Page 34: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Atom Interferometer Force Sensors

Gravity/Accelerations

gravity

LONGER de Broglie wavelength

As atom climbs gravitational potential, velocity decreases and wavelength increases

(Rotations also sensed)

The quantum mechanical wave-like properties of atoms are used to sense inertial forces.

SHORTER de Brogliewavelength

Page 35: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Gravimetry

MASSIVEBLOB

Gravitational force ~ mass

(distance)2

Page 36: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Example: Light-Pulse AI Gravity Gradiometer

Mirror

Atoms

Atoms

L a s

e r

B

e a

m

Gradient measurements: Distinguish gravity induced accelerations from those due to platform motion.

– Simultaneously measure g at two locations with atom interferometer accelerometers

– Difference acceleration signal contains gradient information

G. McGuirk, M. Kasevich

Page 37: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Laboratory validation: Mass Detection

Pb bricks

Lower accelerometer

Sample number (1 sample/sec)

Gra

dien

t (ar

b. u

nits

)

Modulated acceleration signal due to 8 lead bricks near lower accelerometer.

Green o,+: upper/lower accelerometer outputs

Blue: Gradient signal

Successful laboratory demonstration of mass anomaly detection capabilities

G. McGuirk, M. Kasevich

Page 38: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Applications

• SSN/SSBN Navigation - Gravity assisted navigation (currently in use on subs, but need better)

• Underground structure detection (a.k.a. bunker detection)

• Oil and mineral exploration (e.g. kimberlite pipes in Utah –diamonds come from kimberlite, or salt domes in the Gulf of Mexico: oil)

• Space-based studies of Earth’s gravity field

LM UGM

Page 39: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

II. Quantum Tornadoes Near Absolute Zero

Courtesy NOAA

Plus ….what kind of thermometer measures the coldest places in the universe anyways?

Page 40: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers
Page 41: Paul C. Haljan University of Michigan Oct. 2003. I. Laser cooling atoms Magnets Lasers

Hot cloud

Images of clouds

How to make a thermometer for cold atoms

Let the gas expand

Cold cloud