Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift...

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Lecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3 Last Time : eigenstates and energies for hydrogen-like atoms lots of energy degeneracy, only n-dependence () ( ) ϕ θ ψ , lm nl nlm Y r R = ( ) 2 2 2 2 2 1 / = = n Z c m hcR n Z E n α µ µ 137 1 4 0 2 = c e πε α Today : corrections to these energies due to stuff we ignored new terms will be come in at higher powers of [e.g. relativity, electron spin, QED, etc.]

Transcript of Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift...

Page 1: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Lecture 2: Fine structure, Lamb shiftReadings: Foot 1.4, 2.3

Last Time: eigenstates and energies for hydrogen-like atomslots of energy degeneracy, only n-dependence

( ) ( )ϕθψ ,lmnlnlm YrR=

( )2

22

2

21/

−=−= ∞ n

ZcmhcRnZEn

αµµ

1371

4 0

2

≈=c

eπε

α

Today: corrections to these energies due to stuff we ignored

new terms will be come in at higher powers of 𝛼𝛼[e.g. relativity, electron spin, QED, etc.]

Page 2: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (1) KE correction

electrons can run very fast, and so we need to considerrelativistic corrections to their kinetic energy (p2/2m)

Page 3: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (1) KE correction

( ) ( ) ...2222 =−+= mcpcmcKE

Page 4: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (2) Darwin term

The electron actually wiggles very fast, on a short length scale(Zitterbewegung)

Effectively feels a “time-averaged” or “wiggle-averaged” potential,modifying the energy when the electron is near the nucleus

Page 5: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (2) Darwin term

Page 6: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (2) Darwin term

Page 7: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (2) Darwin term

Page 8: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (2) Darwin term

Page 9: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (2) Darwin term

( )rZeH wiggleDδξ

πεπ 2

0

2

42

=

Page 10: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (1&2)

Page 11: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (1&2)

Page 12: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Relativistic effects: (3) Spin-Orbit

EcvB

×−= 2

sg Bs µµ −=

BE ⋅−=∆ µ

wikipedia

Page 13: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Fine structure

2P3/2

2P1/2

nLJ

Page 14: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Lamb shift – interactions with the vacuumObserved energy shift between states with same J value

Also, no explanation for spontaneous emission

Page 15: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Lamb shift – interactions with the vacuum

Page 16: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Lamb shift – interactions with the vacuum

Page 17: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Lamb shift – interactions with the vacuum

value from Udem paper 1045.0079(72) MHz

Page 18: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Lamb shift – coupling to virtual phonons

Page 19: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Precision measurements in AMO physics

Page 20: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Precision measurements in AMO physics

Page 21: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Precision measurements in AMO physics

Page 22: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Quantum-limited measurements

Kasevich group, Nature 2016

Page 23: Lecture 2: Fine structure, Lamb shift - University Of IllinoisLecture 2: Fine structure, Lamb shift Readings: Foot 1.4, 2.3. Last Time: eigenstates and energies for hydrogen-like atoms.

Looking aheadReadings: Foot Ch.3

Next week: multi-electron atoms, and then hyperfine structure

Homework due next Friday, office hours on Wed / Thurs