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Q.M3 - Tirgul 9 Roee Steiner Physics Department, Ben Gurion University of the Negev, BeerSheva 84105, Israel 23.12.2015 Contents 1 Parity - Problem 23 from lecture 7 1 2 Finding the evolution operator in interaction picture - Dyson series 2 3 Time dependant Hamiltonian - different approach 3.1 Time perturbation in harmonic oscillator. . . . . . . . . . . . . . 2 3 4 Class Work 5 1 Parity - Problem 23 from lecture 7 Show that existence of two decay channels of a zero spin K meson into two pions,K → 2π, and into three pions,K → 3π, indicates the non-conservation of parity for K decays. Solution As you seen in the class the pions have zero spin and negative intrinsic parity. In the channel of 2π the parity is symmetric and in the channel 3π has negative parity so, if we have two channel with different parity then the parity is not conserved. ∗ e-mail: [email protected] 1 ∗ 2 Finding the evolution operator in interaction picture - Dyson series A 1/2 spin is placed in a constant magnetic field in the z direction (Bz ) - namely, the unperturbed Hamiltonian H0 is: 1 0 H0 = µBz (1) 0 −1 where µ is the magnetic moment At the time t = 0 the spin was in the | ↑i state At the time t = 0 a weak (Bx Bz ) periodic magnetic field is applied at the x direction, namely the perturbation V (t) is: 0 1 V (t) = µBx cos(ωt) (2) 1 0 Find the probability to find the system at | ↓i at time t (in the first order ?). Solution In the first order the transition amplitude is Z t h↓ |UI (t)| ↑i = −i dt1 eiΩt1 h↓ |V (t1 )| ↑i (3) 0 Z iµBx t dt1 eiΩt1 cos ωt1 (4) − 2 0 where we denoted E↑ = −E↓ = Ω/2 = µBz . The transition amplitude now becomes µBx e−i(Ω+ω)t − 1 e−i(Ω−ω)t − 1 + (5) h↓ |UI (t)| ↑i = − 2 Ω+ω Ω−ω Respectively, the rate of the spin-flips is w↑→↓ = 3 πµ2 Bx2 δ(Ω − ω) 2 (6) Time dependant Hamiltonian - different approach Consider time dependant perturbation in Hamiltonian: b =H b 0 + Vb (t) H (7) b 0 constant in time and totally soluble H b 0 |ni = En |ni. Find general way With H ¬ b b b to solve accurately H = H0 + V (t). ¬ It is question form of chapter 5.5 in Sakurai 2 Solution Lets try some wave state form: |ψ(t)i = Σn cn (t)e−iEn t/~ |ni (8) So now we put the wave function into Schroedinger equation: b H|ψ(t)i ∂ b 0 + Vb )|ψ(t)i = i~ |ψ(t)i = (H ∂t (9) So: ∂ (Σn cn (t)e−iEn t/~ |ni) ∂t b 0 + Vb )Σn cn (t)e−iEn t/~ |ni = (H i~ (10) b 0 e−iEn t/~ |ni = i~ ∂ (e−iEn t/~ |ni) = By doing the derivative and use the fact that H ∂t −iEn t/~ e En |ni we get: i~Σn ċn e−iEn t/~ |ni = Vb Σn cn (t)e−iEn t/~ |ni (11) We multiply from the left by hm| and we get: i~cm ˙ e−iEm t/~ = Σn cn Vmn e−iEn t/~ (12) i~cm ˙ = Σn cn Vmn e−(iEn −Em )t/~ (13) So finely: We have a set of first order deferential equations for cn . 3.1 Time perturbation in harmonic oscillator. A harmonic oscillator system with the energy levels En = (n+1/2)~ω is affected by the electric field applied (t) = A −t2 /2τ 2 e πτ (14) Find, in the first order, the probability to find the oscillator in the first exited state at t → ∞, if at t → ∞ it is in the ground state. Solution The potential is: V (t, x) = −e(t)b x=− eA −t2 /2τ 2 e x b πτ (15) Note that H b 0 e−iEn t/~ |ni = i~ ∂ (e−iEn t/~ |ni) = e−iEn t/~ En |ni so we look for close ∂t solution. 3 The transition amplitude in the first order is Z ∞ eA −t2 /2τ 2 dteiωt h1|UI (∞, −∞)|0i = i e h1|b x|0i πτ −∞ (16) Since 1 (a+ + a) 2mω √ h1|a+ |0i = 2 x b= √ h1|a|0i = 0 (17) (18) (19) one finds h1|b x|0i = √ 1 mω The Gaussian integral is easily calculated and finally √ ieA 2 −ω2 τ 2 /2 h1|UI (∞, −∞)|0i = √ e mωπ (20) (21) so that the probability of the transition is P0→1 = 4 2e2 A2 −ω2 τ 2 e mωπ Class Work 30 from lecture 7 21, 27, 28, 13 from lecture 8 4 (22)