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  What are some ways to (approximately) symbolically diagonalize Hamiltonian operator?

+ 8 like - 0 dislike
1440 views

Specifically the Hamiltonian takes the form of

ˆH=Δ2ˆσz+ω1ˆa1ˆa1+ω2ˆa2ˆa2+g1(ˆa1ˆσ++ˆa1ˆσ)+g2(ˆa2ˆσ++ˆa2ˆσ),

a three body version of Jaynes-Cummings model.

I'm currently trying to diagonalize this Hamiltonian, a first step in our application of quantum Zeno effect to a three-body system.

I guess this Hamiltonian simply has no close-form diagonalization, just like in classical physics there is no closed-form general solution for a three-body system. So my question is: what are several symbolic approximation techniques to diagonalize an Hermitian operator? Better if that techniques particularly suits this Hamiltonian. The values of Δ,ω1,ω2,g1,g2 need not be general; they can be set, say, all equal in order to simplify calculation.

This post has been migrated from (A51.SE)
asked Feb 7, 2012 in Theoretical Physics by Karsus Ren (40 points) [ no revision ]

2 Answers

+ 5 like - 0 dislike

At least for ω1=ω2 it is possible to solve the system exactly. Our Hamiltonian can be written

ˆH=Δ2ˆσz+ω(ˆa1ˆa1+ˆa2ˆa2)+(g1ˆa1+g2ˆa2)ˆσ++(g1ˆa1+g2ˆa2)ˆσ

We apply a change of variables

a1=a1cosθa2sinθ

a2=a1sinθ+a2cosθ

This change of variables preserves the Δ and the ω terms in the Hamiltonian but rotates the (g1,g2) vector. By choosing an appropriate θ we can achieve g2=0. This means the (a1,σ) system decouples from a2. The former is an ordinary Jaynes-Cummings model whereas the later is a Harmonic oscillator

This post has been migrated from (A51.SE)
answered Feb 7, 2012 by Squark (1,725 points) [ no revision ]
I find the eigenvectors for a1 and a2 but I can't find the common set for both (they commute so they should have a common set of eigenvectors).

This post has been migrated from (A51.SE)
I mean a'_1^\dagger a'_1 and a'_2^\dagger a'_2

This post has been migrated from (A51.SE)
Just apply the primed creation operators to the vector annihilated by the primed annihilation operators. Note though that for 1 the oscillator is still coupled to the spin so the eigenvectors are more complicated: like in th usual Jaynes-Cummings

This post has been migrated from (A51.SE)
Not to mention the eigenstates for a'_1^\dagger a'_1 are degenerate! I found at least two vacuum states when θ=π4: |01|02 and |01|12|11|00. This makes it much more complicated than it seems.

This post has been migrated from (A51.SE)
+ 4 like - 0 dislike

This is a Jaynes-Cummings model with a two mode electromagnetic field. One can find some literature about (e.g. see here and refs therein) and some exact solutions are also known. But, if you content yourself with a perturbation soulution for the full parameter Hamiltonian, this can be accomplished in the following way.

Firstly, move to interaction picture. This will give the following Hamiltonian (I will remove the hats as there is no difficulty to tell operators):

HI=g1(a1σ+eiΔ1t+a1σiΔ1te)+g2(a2σ+eiΔ2t+a2σeiΔ2t).

I obtained this after a unitary transformation on H, U0(t)=eiH0t, being H0=Δ2σz+ω1a1a1+ω2a2a2 and having introduced the detunings Δ1=Δω1 and Δ2=Δω2. Interesting physics comes into play when these detunings are allowed to go to 0 but here we take them non null. Now, your problem is to solve the equation

HI(t)UI(t)=itUI(t)

being UI(t) the time evolution operator in the interaction picture. Your solution will be obtained by computing U(t)=eiH0tUI(t). The idea is to extract the diagonal contributions from UI(t) and evaluate from these the approximate eigenvalues for the Hamiltonian we started from. Now, the Schroedinger equation can be rewritte in integral form as

UI(t)=Iit0dtHI(t)UI(t)

where I used the fact that UI(0)=I and I have put t0=0 being this arbitrary. This is now an integral equation as you realize that the unknown is also under the integral sign. But this eqaution can be solved iteratively to give the so called Dyson series for time dependent perturbations starting with a solution UI(t)=I as a first iterate

UI(t)=Iit0dtHI(t)t0dtHI(t)t0dtHI(t)+

Now, we insert our Hamiltonian in the interaction picture into this series and we get (remember that (σ+)2=(σ)2=0)

UI(t)=Iit0dt[g1(a1σ+eiΔ1t+a1σiΔ1te)+g2(a2σ+eiΔ2t+a2σeiΔ2t)]

t0dtt0dt[g21(a1a1σ+σeiΔ1(tt)+a1a1σσ+eiΔ1(tt))
+g22(a2a2σ+σeiΔ2(tt)+a2a2σσ+eiΔ2(tt))
2g1g2(a1a2σ+σei(Δ2tΔ1t)+a1a2σσ+ei(Δ2tΔ1t))]+

The terms we are interested in are those having a "secular" behavior as they increses lienarly with time and these are just the first temrs of the expansion of a time evolution operator in the form eiδH0tIiδH0t+ being δH0 the correction to the unperturbed Hamiltonian. These come out from the second order terms in the Dyson series producimg

UI(t)=Iig21Δ1(a1a1σ+σ+a1a1σσ+)t

ig22Δ2(a2a2σ+σ+a2a2σσ+)t+

At this point we will use the fact that [ai,ai]=1 obtaining

UI(t)=Iig21Δ1a1a1tig21Δ1σ+σt

ig22Δ2a2a2tig22Δ2σ+σt+

Turning back to U0(t)=IiΔ2σztiω1a1a1tiω2a2a2t+ and collecting all together we recognize a new unperturbed Hamiltonian given by

H_0^'=\frac{\Delta}{2}\sigma_z+\frac{g_1^2}{\Delta_1}\frac{1}{2}(1+\sigma_z)+\frac{g_2^2}{\Delta_2}\frac{1}{2}(1+\sigma_z)+\left(\omega_1+\frac{g_1^2}{\Delta_1}\right)a_1^\dagger a_1

+(ω2+g22Δ2)a2a2

from which you can read off the new eigenvalues. You will notice that the excited state goes higher. This is exactly what one should expect from Rayleigh-Schroedinger stationary perturbation method. From the other terms of the series you will able to recover also the eigenvectors (see here). You can also extend this approach to the case when one of the two detunings is zero as one of the two contribution is just the well-knwon Jaynes-Cummings Hamiltonian for a single mode.

This post has been migrated from (A51.SE)
answered Feb 8, 2012 by JonLester (345 points) [ no revision ]

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