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Lecture 2 - A few more cooking recipes for quantum mechanics

In this second lecture we will finish the discussion of the basic cooking recipes and discuss a few of the consequences like the uncertainty relation, the existance of wave packages and the Ehrenfest theorem.

In the first lecture we discussed briefly the basic principles of quantum mechanics like operators, state vectors and the Schrödinger equation. We will finish this discussion today and then introduce the most important consequences. We will continue to closely follow the discussion of the introductory chapter of Ref. 1

Composite systems

It is actually quite rare that we can label the system with a single quantum number. Any atom will involve spin, position, angular momentum. Other examples might just involve two spin which we observe. So the question is then on how we label those systems. We then have two questions to answer:

  1. How many labels do we need for a system to fully determine its quantum state ?

  2. Once I know all the labels, how do I construct the full state out of them ?

We will actually discuss the second question first as it sets the notation for the first question.

Entangled States

In AMO we typically would like to characterize is the state of an electron in a hydrogen atom. We need to define its angular momentum label LL, which might be 0, 1, 2 and also its electron spin SS, which might be {,}\{\uparrow, \downarrow\}. It state is then typically labelled as something like

L=0,S==0,\left|L=0, S=\uparrow\right\rangle = \left|0,\uparrow\right\rangle

etc.

Another, simple example is that of two spins, each one having two possible states {,}\{\uparrow, \downarrow\}. This is a standard problem in optical communication, where you send correlated photons with a certain polarization to different people. We will typically call them Alice and Bob 2.

We now would like to understand than if we can disentangle the information about the different labels. Naively, we can now associate with Alice one set of outcomes and describe it by some state ψA\left|\psi_{A}\right\rangle and the Bob has another set ψB\left|\psi_{B}\right\rangle:

ψA=aA+aAψB=bB+bB\left|\psi_A\right\rangle= a_{\uparrow} \left|\uparrow_A\right\rangle+ a_{\downarrow} \left|\downarrow_A\right\rangle\\ \left|\psi_B\right\rangle= b_{\uparrow} \left|\uparrow_B\right\rangle+ b_{\downarrow} \left|\downarrow_B\right\rangle

The full state will then be described by the possible outcomes {AB,AB,AB,AB}\{\uparrow_A\uparrow_B,\downarrow_A\uparrow_B,\uparrow_A\downarrow_B, \downarrow_A\downarrow_B\}. We can then write:

ψ=α(AB)+α(AB)+α(AB)+α(AB)=α+α+α+α\left|\psi\right\rangle = \alpha_{\uparrow\uparrow}(\left|\uparrow_A\right\rangle\otimes\left|\uparrow_B\right\rangle)+\alpha_{\uparrow\downarrow}(\left|\uparrow_A\right\rangle\otimes\left|\downarrow_B\right\rangle)+\alpha_{\downarrow\uparrow}(\left|\downarrow_A\right\rangle\otimes\left|\uparrow_B\right\rangle)+\alpha_{\downarrow\downarrow}(\left|\downarrow_A\right\rangle\otimes\left|\downarrow_B\right\rangle)\\ = \alpha_{\uparrow\uparrow}\left|\uparrow\uparrow\right\rangle+\alpha_{\uparrow\downarrow}\left|\uparrow\downarrow\right\rangle+\alpha_{\downarrow\uparrow}\left|\downarrow \uparrow\right\rangle+\alpha_{\downarrow\downarrow}\left|\downarrow\downarrow\right\rangle

So we will typically just plug the labels into a single ket and drop indices, to avoid rewriting the tensor symbol each time. We say that a state is separable, if we can write it as a product of the two individual states as above:

ψ=ψAψB=ab+ab+ab+ab\left|\psi\right\rangle = \left|\psi_A\right\rangle\otimes\left|\psi_B\right\rangle\\ =a_{\uparrow} b_\uparrow \left|\uparrow\uparrow\right\rangle+a_{\downarrow} b_\uparrow \left|\downarrow\uparrow\right\rangle+a_{\uparrow} b_\downarrow \left|\uparrow\downarrow\right\rangle+a_{\downarrow} b_\downarrow \left|\downarrow\downarrow\right\rangle

All other states are called entangled. The most famous entangled states are the Bell states:

ψBell=+2\left|\psi_\textrm{Bell}\right\rangle=\frac{\left|\uparrow\uparrow\right\rangle+\left|\downarrow\downarrow\right\rangle}{\sqrt{2}}

In general we will say that the quantum system is formed by two subsystems S1S_1 and S2S_2. If they are independent we can write each of them as:

ψ1=mMamαm,ψ2=nNbnβn.\left|\psi_1\right\rangle=\sum_m^M a_m \left|\alpha_m\right\rangle,\\ \left|\psi_2\right\rangle=\sum_n^N b_n \left|\beta_n\right\rangle.

In general we will then write:

ψ=mMnNcmn(αmβn).\left|\psi\right\rangle=\sum_m^M \sum_n^N c_{mn}(\left|\alpha_m\right\rangle\otimes \left|\beta_n\right\rangle).

So we can determine such a state by M×NM \times N numbers cmnc_{mn} here. If the states are separable, we can write ψ\left|\psi\right\rangle as a product of the individual states:

ψ=ψ1ψ2=(mMamαm)(nNbnβn)\left|\psi\right\rangle=\left|\psi_1\right\rangle\otimes\left|\psi_2\right\rangle=\left(\sum_m^M a_m \left|\alpha_m\right\rangle\right) \otimes \left(\sum_n^N b_n \left|\beta_n\right\rangle\right) ψ=mMnNambnαmβn.\left|\psi\right\rangle=\sum_m^M \sum_n^N a_m b_n \left|\alpha_m\right\rangle \otimes \left|\beta_n\right\rangle.

Separable states thus only describes a small subset of all possible states.

Statistical Mixtures and Density Operator

Having set up the formalism for writing down the full quantum state with plenty of labels, we have to solve the next problem. As an experimentalist, you will rarely measure all of them. This means that you only perform a partial measurement and you have only partial information of the system. The extreme case is the thermodynamic ensemble, where we measure only temperature to describe 102310^{23} particles.

A similiar problem arises for Alice and Bob. They typically measure the state of the qubit in their lab without knowing what the other did. So they need some way to describe the system locally. This is done through the density operator approach.

In the density operator approach the state of the system is described by a Hermitian density operator

ρ^=n=1Npnϕnϕn. \hat{\rho} = \sum_{n=1}^N p_n \left|\phi_n\right\rangle\left\langle\phi_n\right|.

Here, ϕn\left\langle\phi_n\right| are the eigenstates of ρ^\hat{\rho}, and pnp_n are the probabilities to find the system in the respective states ϕn\left|\phi_n\right\rangle. The trace of the density operator is the sum of all probabilities pnp_n:

tr(ρ^)=pn=1. \mathrm{tr}(\hat{\rho}) = \sum p_n = 1.

For a pure state ψ\left|\psi\right\rangle, we get pn=1p_n=1 for only one value of nn. For every other nn, the probabilities vanish. We thus obtain a "pure" density operator ρ^pure\hat{\rho}_{\text{pure}} which has the properties of a projection operator:

ρ^pure=ψψρ^2=ρ^.\hat{\rho}_{\text{pure}} = \left|\psi\right\rangle\left\langle\psi\right| \qquad \Longleftrightarrow \qquad \hat{\rho}^2 = \hat{\rho}.

For the simple qubit we then have:

ρ^=(α+α)(α+α)=α2+α2+αα+αα \hat{\rho}= \left(\alpha_\uparrow\left|\uparrow\right\rangle+\alpha_\downarrow\left|\downarrow\right\rangle\right)\left(\alpha_\uparrow^*\left\langle\uparrow\right|+\alpha_\downarrow^*\left\langle\downarrow\right|\right)\\ = |\alpha_\uparrow|^2\left|\uparrow\right\rangle\left\langle\uparrow\right|+|\alpha_\downarrow|^2\left|\downarrow\right\rangle\left\langle\downarrow\right|+\alpha_\downarrow\alpha_\uparrow^*\left|\downarrow\right\rangle\left\langle\uparrow\right|+\alpha_\uparrow\alpha_\downarrow^*\left|\uparrow\right\rangle\left\langle\downarrow\right|

Then it is even simpler to write in matrix form:

ρ^=(α2ααααα2) \hat{\rho}= \left(\begin{array}{cc} |\alpha_\uparrow|^2&\alpha_\uparrow\alpha_\downarrow^*\\ \alpha_\downarrow\alpha_\uparrow^*&|\alpha_\downarrow|^2 \end{array}\right)

For a thermal state on the other hand we have:

ρ^thermal=n=1NeEnkBTZϕnϕn with Z=n=1NeEnkBT\hat{\rho}_{\text{thermal}} = \sum_{n=1}^N \frac{e^{-\frac{E_n}{k_BT}}}{Z} \left|\phi_n\right\rangle\left\langle\phi_n\right|\text{ with }Z = \sum_{n=1}^N e^{-\frac{E_n}{k_BT}}

With this knowledge we can now determine the result of a measurement of an observable AA belonging to an operator A^\hat{A}. For the pure state ψ\left|\psi\right\rangle we get:

A^=ψA^ψ.\langle \hat{A}\rangle = \left\langle\psi\right| \hat{A} \left|\psi\right\rangle.

For a mixed state we get:

A^=tr(ρ^A^)=npnϕnA^ϕn.\langle \hat{A}\rangle = \mathrm{tr}(\hat{\rho}\cdot \hat{A}) = \sum_n {p_n} \left\langle\phi_n\right| \hat{A} \left|\phi_n\right\rangle.

The time evolution of the density operator can be expressed with the von Neumann equation:

itρ^(t)=[H^(t),ρ^(t)].i\hbar \partial_{t}\hat{\rho}(t) = [\hat{H}(t),\hat{\rho}(t)].

Back to partial measurements

We can now come back to the correlated photons sent to Alice and Bob, sharing a Bell pair. They full density matrix is then especially simple:

ρ^=(12001200000000120012) \hat{\rho}= \left(\begin{array}{cccc} \frac{1}{2}& 0& 0 &\frac{1}{2}\\ 0 & 0 & 0& 0\\ 0&0&0&0\\ \frac{1}{2}&0&0&\frac{1}{2} \end{array}\right)

Let us write the system as S=SASBS = S_A \otimes S_B. If we are looking for the density operator ρ^i\hat{\rho}_i of each individual, we can simply write:

ρ^A=trB(ρ^),ρ^B=trA(ρ^),\hat{\rho}_A=\mathrm{tr}_{B}(\hat{\rho}),\\ \hat{\rho}_B=\mathrm{tr}_{A}(\hat{\rho}),

where ρ^=ψψ\hat{\rho}=\left|\psi\right\rangle\left\langle\psi\right| and trj(ρ^)\mathrm{tr}_{j}(\hat{\rho}) is the trace over the Hilbert space of subsystem jj.

To reduce the density matrix of the Bell state it is actually helpful to write out the definitions:

trB(ρ^)=Bρ^B+Bρ^B=12(AA+AA)\mathrm{tr}_{B}(\hat{\rho}) = \left\langle\uparrow_B\right|\hat{\rho}\left|\uparrow_B\right\rangle+\left\langle\downarrow_B\right|\hat{\rho}\left|\downarrow_B\right\rangle\\ =\frac{1}{2}\left(\left|\uparrow_A\right\rangle\left\langle\uparrow_A\right|+\left|\downarrow_A\right\rangle\left\langle\downarrow_A\right|\right)

So we end up with the fully mixed state:

ρ^A,B=(120012) \hat{\rho}_{A,B} = \left(\begin{array}{cc} \frac{1}{2}&0\\ 0&\frac{1}{2} \end{array}\right)

Alice and Bob are simply cossing a coin if they ignore the outcome of the other member. But once they start comparing results we will see that the quantum case can dramatically differ from the classical case. This will be the content of lecture 12 [@entanglement].

Important Consequences of the Principles

Uncertainty Relation

The product of the variances o two noncommuting operators has a lower limit:

ΔA^ΔB^12[A,B^^], \Delta \hat{A} \cdot \Delta \hat{B} \geq \frac{1}{2} \left| \left\langle\left[\hat{A,\hat{B}}\right]\right\rangle \right|,

where the variance is defined as ΔA^=A2^A^2\Delta \hat{A} = \sqrt{\left\langle\hat{A^2}\right\rangle-\left\langle\hat{A}^2\right\rangle}.

Examples.

[x^,p^]=i[J^i,J^j]=iϵijkJ^k\left[ \hat{x}, \hat{p} \right] = i \hbar \\ \left[ \hat{J}_i , \hat{J}_j \right] = i \hbar \epsilon_{ijk} \hat{J}_k

Note. This is a statement about the state itself, and not the measurement!

Ehrenfest Theorem

With the Ehrenfest theorem, one can determine the time evolution of the expectation value of an operator A^\hat{A}:

ddtA^=1i[A^,H^]+tA^(t). \frac{d}{dt}\left\langle\hat{A}\right\rangle=\frac{1}{i\hbar}\left\langle\left[\hat{A},\hat{H}\right]\right\rangle+\left\langle\partial_t\hat{A}(t)\right\rangle.

If A^\hat{A} is time-independent and [A^,H^]=0\left[\hat{A},\hat{H}\right]=0, the expectation value A^\left\langle\hat{A}\right\rangle is a constant of the motion.

Complete Set of Commuting Observables

A set of commuting operators {A^,B^,C^,,X^}\{\hat{A},\hat{B},\hat{C},\cdots,\hat{X}\} is considered a complete set if their common eigenbasis is unique. Thus, the measurement of all quantities {A,B,,X}\{A,B,\cdots,X\} will determine the system uniquely. The clean identification of such a Hilbert space can be quite challenging and a nice way of its measurment even more. Coming back to our previous examples:

  1. Performing the full spectroscopy of the atom. Even for the hydrogen atom we will see that the full answer can be rather involved...

  2. The occupation number is rather straight forward. However, we have to be careful that we really collect a substantial amount of the photons etc.

  3. Are we able to measure the full position information ? What is the resolution of the detector and the point-spread function ?

  4. Here it is again rather clean to put a very efficient detector at the output of the two arms ...

  5. What are the components of the spin that we can access ? The zz component does not commute with the other components, so what should we measure ?

In the third lecture of this course will start to apply these discussions to the two-level system, which is one of the simplest yet most powerful models of quantum mechanics.

Footnotes

  1. Jean Dalibard Jean-Louis Basdevant. The Quantum Mechanics Solver. Springer-Verlag, 2006.

  2. And if someone wants to listen the person is called Eve