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Three problems about Atomic and Optical Physics I: try to solve them!
Typology: Exercises
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Spring 2012, Prof. Wolfgang Ketterle
Due Wednesday, February 22, 2012
h¯ H = −~μ · B~ =. 2
( ω 0 ωR e−iωt (1) ωR eiωt^ −ω 0
)
This Hamiltonian corresponds to a magnetic moment ~μ in a combination of static and rotating fields B^ ~(t) = −(B 1 cos ωt, B 1 sin ωt, B 0 ). Here ω 0 = γB 0 and ωR = γB 1 are the Larmor and Rabi frequency associated with the static field B 0 and (^) (the rotating field of magnitude B 1 , respectively, 1
) ( 0 and γ is the gyromagnetic ratio. The basis is = |↓〉 ≡ |e〉,
) = , 0 |↑〉 g 1 ≡ | 〉 where
|↑〉, |↓〉 are the states where ~μ is oriented along the ∓z axis. The time evolution of any state |ψ(t)〉 = ag(t)|g〉 + ae(t)|e〉 is determined by the two coefficients ag(t), ae(t).
a.) Find the equations of motion for the system, i.e. derive explicit expressions for a˙ (^) g(t) and a˙ (^) e(t).
b.) Solve the equations of motion and find ag(t) and ae(t) in terms of ag(0) and ae(0).
c.) Given the initial conditions ag(0) = 1 and ae(0) = 0 show that the probability to find the system in the state |e〉 agrees with the classical result.
σ̂ (^) x =
( 0 1
) , σ̂ x =
( 0 −i
) 1 0 , σ̂ z = , 1 0 i 0
(
0 − 1
) (2)
are the Pauli spin matrices.
Employing the von Neumann equation ih¯ρ˙ = [H, ρ] show that ~r = r 1 xˆ + r 2 yˆ + r 3 zˆ obeys the relation d~ dtr = ~ω × ~r with ~ω = V 1 xˆ + V 2 ˆy + ω 0 zˆ. Can you interpret this result?
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8.421 Atomic and Optical Physics I Spring 2014
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