15
AC Stark Effect Travis Beals Physics 208A UC Berkeley Physics (picture has nothing whatsoever to do with talk)

Beals, AC Stark Effect

Embed Size (px)

DESCRIPTION

Good presentation on the AC stark effect

Citation preview

  • AC Stark EffectTravis BealsPhysics 208A

    UC Berkeley Physics

    (picture has nothing whatsoever to do with talk)

  • What is the AC Stark Effect?

    Caused by time-varying (AC) electric field, typically a laser.

    Shift of atomic levels

    Mixing of atomic levels

    Splitting of atomic levels

    (another pretty but irrelevant picture)

  • DC Stark Shift

    Constant DC electric field

    Usually first-order (degenerate) pert. theory is sufficient

    DC Stark Effect can lift degeneracies, mix states

    H

    stark = p E

    = ezE = eEr cos

    |2, 0, 0 |2, 1, 0 |2, 1,+1|2, 1,1

    |2, 1,+1|2, 1,1

    |2, 1, 0 |2, 0, 02

    |2, 1, 0+ |2, 0, 02

    Hydrogen n=2 levels

  • AC/DC: Whats the difference?

    AC time-varying fieldsAttainable DC fields typically much smaller (105 V / cm, versus 1010 V / cm for AC)

    AC Stark Effect can be much harder to calculate.

    (highly relevant picture)

  • One-level Atom

    Monochromatic variable field

    Atom has dipole moment d, polarizability . Thus, interaction has the following form:

    Now, we solve the following using the Floquet theorem:

    Hint = dF cost1

    2F

    2cos

    2t

    id

    dt= Hint

  • One-level Atom (2)Get solution:

    AC Stark energy shift is Ea, ks correspond to quasi-energy harmonics

    (r, t) = exp(iEat)k=

    k=

    Ck(r) exp(ikt)

    Ea(F ) = 1

    4F

    2

    Ck =

    S=

    (1)kJS

    (F 2

    8

    )Jk+2S

    (dF

    )with ,

  • One-level Atom (3)

    Weak, high frequency field:

    Arguments of Bessel functions in are small, so only the k=S=0 term in is significant.

    Quasi-harmonics not populated, basically just get AC Stark shift Ea

    dF

  • One-level Atom (4)

    Strong, low-frequency field:

    Bessel functions in kill all terms except S=0, and k=dF/Only quasi-harmonics with energies dF are populated, so we get a splitting of the level into two equal populations

    dF >> , F 2

  • One-level Atom (5)Very strong, very low-frequency field:

    Only populated quasi-energy harmonics are those with

    Thus, have splitting of levels, get energies

    dF >> , F 2 >>

    k ! dF

    F 2

    4

    E(F ) = dF F 2

    4F 2

    4

  • Multilevel AC Stark Effect

    Ei =3pic2

    230

    I c2ij

    ij

    intensity

    electronic ground

    state |gi> shift

    transition co-efficient: ij = cij ||||

    detuning: ij = - ijexcited state energy: 0

    width of excited state

  • Assumptions & RemarksUsed rotating wave approximation (e.g. reasonably close to resonance)

    Assumed field not too strong, since a perturbative approach was used

    Can use non-degen. pert. theory as long as there are no couplings between degen. ground states

    In a two-level atom, excited state shift is equal magnitude but opposite sign of ground state shift

  • AC Stark in Alkalis

    Udip(r) =pic2

    230

    (2 + PgF mF

    2,F+

    1 PgF mF1,F

    )I(r)

    !,

    FS

    21P

    2

    P2

    21

    21

    23

    21

    0

    L=0

    L=1

    (b)

    J=

    J=

    (c)

    J =

    HFS!

    HFS!

    ,

    F=2

    F=1

    F=2

    F=1

    (a) F=3

    23

    2

    S

    "

    (Figure from R Grimm et al, 2000)

    I = 3/2

  • AC Stark in Alkalis (2)

    Udip(r) =pic2

    230

    (2 + PgF mF

    2,F+

    1 PgF mF1,F

    )I(r)

    F, mF are relevant ground state quantum numbers

    laser polarization0: linear, 1:

    Land factor

    detuning between 2S1/2,F=2 and 2P3/2

    detuning between 2S1/2,F=1 and 2P1/2

  • What good is it?

    Optical traps

    Quantum computing in addressable optical lattices use the shift so we can address a single atom with a microwave pulse

  • References

    N B Delone, V P Kranov. Physics-Uspekhi 42, (7) 669-687 (1999)

    R Grimm, M Weidemller. Adv. At., Mol., Opt. Phys. 42, 95 (2000) or arXiv:physics/9902072

    A Kaplan, M F Andersen, N Davidson. Phys. Rev. A 66, 045401 (2002)