using the fine structure constant to push on the...

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Lecture 5: Using the Fine Structure Constant to Push on the Standard Model The 64 th Compton Lecture Series Unsolved Mysteries of the Universe: Looking for Clues in Surprising Places THE ENRICO FERMI INSTITUTE Brian Odom http://kicp.uchicago.edu/~odom/compton.htm

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Lecture 5: Using the Fine Structure Constantto Push on the Standard Model

The 64th Compton Lecture Series

Unsolved Mysteries of the Universe:Looking for Clues in Surprising Places

THE ENRICO FERMI INSTITUTE

Brian Odom

http://kicp.uchicago.edu/~odom/compton.htm

Oct. 21, 2006 Brian Odom Compton Lecture 5

The Fine Structure Constant2e

cα =

2P

1S

2P

1S

Hydrogen Energy Levels

Predicted Emission Spectrum

If there were no fine structure

With fine structure

10.2 eV (121.6 nm)10.2 eV (121.6 nm)

4.5 x 10-5 eV

Oct. 21, 2006 Brian Odom Compton Lecture 5

Coupling Constants

The fine structure constant quantifies the strength of the coupling of light to matter, or the strength of electromagnetism.

We will talk only aboutthe low-energy limit

Oct. 21, 2006 Brian Odom Compton Lecture 5

What is its Value?

“It has been a mystery ever since it was discovered more than fifty years ago, and all good theoretical physicists put this number up on their wall and worry about it.”

- Richard Feynman

It is “one of the greatest damn mysteries of physics: a magic number that comes to us with no understanding by man."

- Richard Feynman

Despite many attempts, α remains one of the free parameters of the standard model. We cannot predict it; we must measure it.

Oct. 21, 2006 Brian Odom Compton Lecture 5

What is its Value?

1137

α ≈

…but not quite

1 137α − ≈or

1 137.035 999 710 (96)α − ≈Gabrielse, Hanneke, Kinoshita, Nio, and Odom, Phys Rev Lett 97, 030802 (2006)

Oct. 21, 2006 Brian Odom Compton Lecture 5

A Good Thing that it is Small1 1

137α ≈

1st order:

This allows us to use perturbation theory for calculations

2nd order:

3rd order:

+ +

+ …

Oct. 21, 2006 Brian Odom Compton Lecture 5

Old Quasar Light…Is it Really Constant?

Murphy, et. al. Mon. Not. R. Astron Soc. 345 (2003)

( figure from Chris Churchill )

Oct. 21, 2006 Brian Odom Compton Lecture 5

Old Quasar Light…Is it Really Constant?

figure from Chris Churchill

Srianand, et al. Phys. Rev. Lett.. 92, 12 (2004)

… systematics errors can be tricky

Oct. 21, 2006 Brian Odom Compton Lecture 5

Is it Really Constant?

α αΔzexperiment α α≈ (yr -1)

< 6 x 10-17< 6 x 10-70.4 – 2.3QSO absorp., Srianand et. al.64 (14) x 10-17

< 20 x 10-17< 0.5 x 10-17< 200 x 10-17

54 (12) x 10-70.5 – 3.5QSO absorp., Murphy et. al.

< 8 x 10-70.45Meteorite Re/Os abundance< 0.1 x 10-70.14Oklo nuclear phenomenon< 6 x 10-150Lab atomic transitions (Yb/Cs)

< 6 x 10-17< 6 x 10-70.4 – 2.3QSO absorp., Srianand et. al.64 (14) x 10-17

< 20 x 10-17< 0.5 x 10-17< 200 x 10-17

54 (12) x 10-70.5 – 3.5QSO absorp., Murphy et. al.

< 8 x 10-70.45Meteorite Re/Os abundance< 0.1 x 10-70.14Oklo nuclear phenomenon< 6 x 10-150Lab atomic transitions (Yb/Cs)

So far, there is no evidence that α varies with time. But, it does vary in some theories. …We keep looking.

(…but I heard yesterday that the lab results have improved substantially)

An interesting note: these experiments have fantastic sensitvity to variations of α, but they are not the best ways to measure its actual value

Oct. 21, 2006 Brian Odom Compton Lecture 5

Electron Magnetic Moment

If the electron is a point particle (has no size), the Standard Model allows precise prediction of the magnetic moment, provided we know α

0th order:

1st order: + …

Oct. 21, 2006 Brian Odom Compton Lecture 5

The g - Factor

Classical, non-relativistic

Dirac equation as single-particle wave equation

Quantum Electrodynamics (QED)

2.002 319 304g = ...

2g =

1g =

2q S

gm

μ⎛ ⎞

= ⎜ ⎟⎝ ⎠

Oct. 21, 2006 Brian Odom Compton Lecture 5

Why Measure the g - Factor?

• Determination of α, using QED calculations

• Precision test of QED

• Probe for electron sub-structure

• Precision test of Lorentz, CPT symmetry

• Complement to the muon g – factor measurement

(which is a great search for new particles)

• Prospects for improved proton to electron mass

ratio

Oct. 21, 2006 Brian Odom Compton Lecture 5

Does the Electron Have Size?

So far we have no reason to believe it has size… but we keep looking.

Oct. 21, 2006 Brian Odom Compton Lecture 5

Testing Quantum Electrodynamics

α-1137.03599 137.03600 137.03601

Δα / α (ppb)-100-50050100

muonium h.f. structure

electron g, UW 1987

quantum Hall effect

ac Josephson effect & γp,h

h / mn

h / mCs, optical trans- itions, mass ratios

electron g, Harvard 2006

h / mRb, mass ratios

Oct. 21, 2006 Brian Odom Compton Lecture 5

Different Levers for New Physics

α αΔzexperiment α α≈ (yr -1)

< 6 x 10-17< 6 x 10-70.4 – 2.3QSO absorp., Srianand et. al.64 (14) x 10-17

< 20 x 10-17< 0.5 x 10-17< 200 x 10-17

54 (12) x 10-70.5 – 3.5QSO absorp., Murphy et. al.

< 8 x 10-70.45Meteorite Re/Os abundance< 0.1 x 10-70.14Oklo nuclear phenomenon< 6 x 10-150Lab atomic transitions (Yb/Cs)

< 6 x 10-17< 6 x 10-70.4 – 2.3QSO absorp., Srianand et. al.64 (14) x 10-17

< 20 x 10-17< 0.5 x 10-17< 200 x 10-17

54 (12) x 10-70.5 – 3.5QSO absorp., Murphy et. al.

< 8 x 10-70.45Meteorite Re/Os abundance< 0.1 x 10-70.14Oklo nuclear phenomenon< 6 x 10-150Lab atomic transitions (Yb/Cs)

Some people use high precision over short times. Some people use enormous times and less precision.

(…but I heard yesterday that the lab results have improved substantially)

Oct. 21, 2006 Brian Odom Compton Lecture 5

Different Levers for New Physics

Higher energy means shorter wavelength—and the ability to look for even smaller structure

… or we can do precision measurements, like measurement of the g - factor

Oct. 21, 2006 Brian Odom Compton Lecture 5

g from the Standard Model2 3 4

1 2 3 41 ...2g C C C C non QEDα α α α

π π π π⎛ ⎞ ⎛ ⎞ ⎛ ⎞ ⎛ ⎞= + + + + + + −⎜ ⎟ ⎜ ⎟ ⎜ ⎟ ⎜ ⎟⎝ ⎠ ⎝ ⎠ ⎝ ⎠ ⎝ ⎠

Oct. 21, 2006 Brian Odom Compton Lecture 5

An Electron in a Penning Trap

B Field E Field magnetronmotion

axialmotion

cyclotronmotion

0.02 Hz7.2 K149.0 GHzcyclotron

10-17 Hz6.4 μK130 kHzmagnetron

10-12 Hz7.2 K149.2 GHzspin

1 Hz9.6 mK200 MHzaxial

dampinghυ/kbfrequencymotion

Oct. 21, 2006 Brian Odom Compton Lecture 5

Do a Frequency Measurement!

( )( ) ( )

2 1a z c 2

21 1c z c2 2

2=1

2 2g ω ω ω δ

ω δ ω ω δ− +

++ + +

s

c2g ω

ω=

g in free space:

g-2 in free space:

a

c

21 12 2g g ω

ω−= + = +

g-2 in a Penning trap:

[ Brown and Gabrielse. Rev. Mod. Phys. 58, 1 (1986) ](3 orders of magnitude for free)

2q S

gm

μ⎛ ⎞

= ⎜ ⎟⎝ ⎠

Definition:

Oct. 21, 2006 Brian Odom Compton Lecture 5

Cylindrical Penning Trap Construction

Oct. 21, 2006 Brian Odom Compton Lecture 5

Dilution Refrigerator and Magnet

10'1"

x10

Oct. 21, 2006 Brian Odom Compton Lecture 5

The Lab

Oct. 21, 2006 Brian Odom Compton Lecture 5

A tabletop experiment …if you have a high ceiling

Oct. 21, 2006 Brian Odom Compton Lecture 5

Detection of a Single Electron•The axial oscillator is coupled to a tuned-circuit amplifier

Signal Out

−20 −10 0 10 20

0.0

0.4

ampl

itude

(a. u

.)

−20 −10 0 10 20−0.5

0.0

0.5

frequency − νz (Hz)

•Axial motion is driven to increase signal

Oct. 21, 2006 Brian Odom Compton Lecture 5

Single Quantum Jumps

decay time (s)0 10 20 30 40 50 60

num

ber o

f n=1

to n

=0 d

ecay

s

0

10

20

30

time (s)0 100 200 300

axia

l fre

quen

cy s

hift

(Hz)

-3

0

3

6

9

12

15τ = 16 s

•In free space, cyclotron lifetime = 0.08 s

•In our cylindrical traps, we have

achieved a 16 s lifetime

[ Peil and Gabrielse. Phys. Rev. Lett. 83, 1287 (1999) ]

Oct. 21, 2006 Brian Odom Compton Lecture 5

Benefits of Cooling Down

Relativistic Corrections

•Eliminates relativistic errorfrom ωc uncertainty

Thermal Jumps4.2 K

012

3.2 K

012

2.0 K

012

1.6 K

012

.08 K

time (minutes)0 5 10 15 20 25 30 35 40 45 50

cycl

otro

n qu

antu

m n

umbe

r

012

[ Peil and Gabrielse. Phys. Rev. Lett. 83, 1287 (1999) ]

•Reducing thermal jumps permits single-quantum cyclotron spectroscopy

Oct. 21, 2006 Brian Odom Compton Lecture 5

T-Dependent Magnetism…BAD

An unpleasant surprise:

•We observed a huge shift of B-field vs. trap temperature

•Heat load changes are unavoidable as:

•Amplifier cycles on/off

•Anomaly drive is applied

•10 ppb / mK is far too much!

tem

pera

ture

(mK

)

707580859095

100105

time (hours)0 2 4 6 8 10

B fi

eld

shift

(ppb

)

-300-250-200-150-100

-500

Shift of -10 ppb / mK at 75 mK !!!

Oct. 21, 2006 Brian Odom Compton Lecture 5

It’s the Trap!

temperature (Kelvin)

0.0 0.5 1.0 1.5 2.0

mag

netic

fiel

d sh

ift (p

pb)

-100

0

100

200

300

400

500

600

700

temperature-1 (Kelvin-1)

0 5 10 15-100

0

100

200

300

400

500

600

700

•Nuclear paramagnetism makes standard Penning trap materials (copper, MACOR) incompatible with a stable B-field below 1 K

Oct. 21, 2006 Brian Odom Compton Lecture 5

New Silver Trap

Oct. 21, 2006 Brian Odom Compton Lecture 5

Prototype Silver Tripod

Oct. 21, 2006 Brian Odom Compton Lecture 5

Silver Trap Improvement

temperature (Kelvin)

0.0 0.5 1.0 1.5 2.0

mag

netic

fiel

d sh

ift (p

pb)

-100

0

100

200

300

400

500

600

700

copper trapsilver trap

temperature-1 (Kelvin-1)

0 5 10 15-100

0

100

200

300

400

500

600

700

copper trapsilver trap

0.0 0.5 1.0 1.5 2.0

expa

nded

200

x

-10

0

10

20

30

•New silver trap decreases T-dependence of the field by ~ 400•With the silver trap, sub-ppb field stability is easily achieved

Oct. 21, 2006 Brian Odom Compton Lecture 5

More Benefits of Cooling Down

frequency - 146 832 090.270 kHz-0.5 0.0 0.5 1.0 1.5

quan

tum

jum

p fr

actio

n

0.00

0.05

0.10

0.15

0.20

2 ppb

frequency - 146 832 090.270 kHz-4 -2 0 2 4 6 8

quan

tum

jum

p fr

actio

n

0.00

0.05

0.10

0.15

0.20

10 ppb

Harvard cyclotron line

[ Van Dyck et al., QED, Kinoshita, ed. 1990]

101500150B2 (T/m2)

200

0.6

Harvard

0.09

0.1

60υz (MHz)

6Tz (K)

U. Wash. H

UW

ΔΔ

H

UW0.09Δ

Δ =

Oct. 21, 2006 Brian Odom Compton Lecture 5

Scatter of Measurements

uWave power (a.u.)0 20 40 60 80

176

178

180

182

184

186

UW 1991

uWave power (a.u.)0 20 40 60 80

176

178

180

182

184

186

Harvard 2006UW 1987

Oct. 21, 2006 Brian Odom Compton Lecture 5

Cavity Shift Systematic

• Parametric response of large e- cloud maps cavity mode structure

• Modes coupling to centered single e- cloud are easily identified[ Tan and Gabrielse. App. Phys. Lett. 55, 2144 (1989) ]

TE1n1TM1n1

Oct. 21, 2006 Brian Odom Compton Lecture 5

Lifetime Shifts

Q = 6500E

Q = 1400M

• Perform single e- experiments between TE127 and TM143

• Cyclotron lifetime data shows qualitatively correct behavior

• Fixing mode ω s and fitting for Qs gives reasonable results

Oct. 21, 2006 Brian Odom Compton Lecture 5

Apparent g – Factor Shift

Oct. 21, 2006 Brian Odom Compton Lecture 5

And the Number is …Harvard g-factor measurement:• Fully quantum measurement eliminates relativistic shift

( 1 ppt per quantum level )

• Low temperature allows quantum spectroscopy and narrows lines

• Cylindrical trap allows first quantitative treatment of cavity shift

g / 2 = 1.001 159 652 180 85 (76)(0.76 ppt)

α = 137.035 999 710 (90) (32)137.035 999 710 (96)

(0.70 ppb)

-1

Results :

Oct. 21, 2006 Brian Odom Compton Lecture 5

New Value for α