Heisenberg Equations of Motion for Electron in EM-field

  • #1
thatboi
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Consider the Heisenberg picture Hamiltonian $$H(t) = \int_{\textbf{r}}\psi^{\dagger}(\textbf{r},t)\frac{(-i\hbar\nabla+e\textbf{A})^{2}}{2m}\psi(\textbf{r},t)$$ where ##\psi(\textbf{r},t)## is a fermion field operator. To find the equations of motion that ##\psi,\psi^{\dagger}## obey. I would invoke the Heisenberg equations of motion ##i\hbar\partial_{t}\psi = [\psi(t),H(t)]## and ##i\hbar\partial_{t}\psi^{\dagger} = [\psi(t)^{\dagger},H(t)]##. I know the equations of motion should be $$i\hbar\partial_{t}\psi = \frac{1}{2m}((-i\hbar\nabla+e\textbf{A})^{2})\psi$$ and $$i\hbar\partial_{t}\psi^{\dagger} = -\frac{1}{2m}((i\hbar\nabla+e\textbf{A})^{2})\psi^{\dagger}$$
But I have redone this calculation so many times for ##\psi^{\dagger}## and do not understand how come the ##i## flips signs for the ##\psi^{\dagger}## case inside ##((i\hbar\nabla+e\textbf{A})^{2})##. In both instances, the calculation requires us taking the commutator with the same Hamiltonian ##H(t)## so why is there suddenly a sign flip now?
 
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  • #2
Hint: Can you explain why the momentum operator ##p=-i\hbar\nabla## is hermitian?
 
  • #3
Demystifier said:
Hint: Can you explain why the momentum operator ##p=-i\hbar\nabla## is hermitian?
Do you mean to say there is some kind of integration by parts argument I am overlooking here? I don't think I see how it plays into the calculation of the 2 commutators.
 
  • #4
thatboi said:
Do you mean to say there is some kind of integration by parts argument I am overlooking here? I don't think I see how it plays into the calculation of the 2 commutators.
Yes, there's a partial integration implicitly involved. Let me first write the Hamiltonian as
$$H=\int d^3r \psi^{\dagger} (h \psi)$$
where
$$h=\frac{(-i\hbar\nabla+eA)^2}{2m}$$
The notation ##(h\psi)## reminds us that ##h## contains a derivative operator acting on ##\psi##. Then
$$H^{\dagger}=\int d^3r (h \psi)^{\dagger} \psi =\int d^3r (h^* \psi^{\dagger}) \psi$$
In the last expression, ##h^*## acts only on ##\psi^{\dagger}##, not on ##\psi##. Now, if you want that the derivative operator acts on ##\psi##, and not on ##\psi^{\dagger}##, you must perform a partial integration. This partial integration flips the sign, so
$$H^{\dagger}=\int d^3r \psi^{\dagger} (h\psi)=H$$
confirming that ##H## is hermitian. The moral is, when you use the operator ##h## containing the derivative operator, you must always know on which object this derivative acts. When you keep track of this, you can see how the sign flips.
 
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  • #5
Demystifier said:
Yes, there's a partial integration implicitly involved. Let me first write the Hamiltonian as
$$H=\int d^3r \psi^{\dagger} (h \psi)$$
where
$$h=\frac{(-i\hbar\nabla+eA)^2}{2m}$$
The notation ##(h\psi)## reminds us that ##h## contains a derivative operator acting on ##\psi##. Then
$$H^{\dagger}=\int d^3r (h \psi)^{\dagger} \psi =\int d^3r (h^* \psi^{\dagger}) \psi$$
In the last expression, ##h^*## acts only on ##\psi^{\dagger}##, not on ##\psi##. Now, if you want that the derivative operator acts on ##\psi##, and not on ##\psi^{\dagger}##, you must perform a partial integration. This partial integration flips the sign, so
$$H^{\dagger}=\int d^3r \psi^{\dagger} (h\psi)=H$$
confirming that ##H## is hermitian. The moral is, when you use the operator ##h## containing the derivative operator, you must always know on which object this derivative acts. When you keep track of this, you can see how the sign flips.
Right, I can understand that argument but what I need to calculate is ##[\psi,H]## and ##[\psi^{\dagger},H]##. I don't see why I cannot use the same H for both commutators. The ##\psi## are just field operators so what matters most is their commutation relations right. In both cases we would end up with ##[\psi(r), \psi^{\dagger}(r')\psi(r')],[\psi(r)^{\dagger}, \psi^{\dagger}(r')\psi(r')]##.
 
  • #6
thatboi said:
Right, I can understand that argument but what I need to calculate is ##[\psi,H]## and ##[\psi^{\dagger},H]##. I don't see why I cannot use the same H for both commutators.
You can use the same H, as I will explain.

thatboi said:
The ##\psi## are just field operators so what matters most is their commutation relations right. In both cases we would end up with ##[\psi(r), \psi^{\dagger}(r')\psi(r')],[\psi(r)^{\dagger}, \psi^{\dagger}(r')\psi(r')]##.
Using a short-hand notation ##\psi(x)=\psi##, ##\psi(x')=\psi'##, etc., I take
$$H=\int dx' \psi'^{\dagger}(h'\psi')$$
First I compute ##[\psi,H]## and after a straightforward calculus I obtain
$$[\psi,H]=(h\psi)$$
without using partial integration. Similarly, with the same expression for ##H##, after a straightforward calculus I obtain
$$[\psi^{\dagger},H]=-\int dx' \psi'^{\dagger} (h'\delta(x-x'))$$
Now the point is that ##h'## contains a derivative acting on the ##\delta##-function, which is ill-defined. Hence I want that ##h'## acts on ##\psi'^{\dagger}##, and to achieve this I need a partial integration. The partial integration flips the sign, i.e. ##h'\to h'^*##, giving
$$[\psi^{\dagger},H]=-(h^*\psi^{\dagger})$$
 
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  • #7
Demystifier said:
You can use the same H, as I will explain.


Using a short-hand notation ##\psi(x)=\psi##, ##\psi(x')=\psi'##, etc., I take
$$H=\int dx' \psi'^{\dagger}(h'\psi')$$
First I compute ##[\psi,H]## and after a straightforward calculus I obtain
$$[\psi,H]=(h\psi)$$
without using partial integration. Similarly, with the same expression for ##H##, after a straightforward calculus I obtain
$$[\psi^{\dagger},H]=-\int dx' \psi'^{\dagger} (h'\delta(x-x'))$$
Now the point is that ##h'## contains a derivative acting on the ##\delta##-function, which is ill-defined. Hence I want that ##h'## acts on ##\psi'^{\dagger}##, and to achieve this I need a partial integration. The partial integration flips the sign, i.e. ##h'\to h'^*##, giving
$$[\psi^{\dagger},H]=-(h^*\psi^{\dagger})$$
Ahh, there was the missing minus sign I was looking for! Thanks so much, I was not careful enough with my treatment of the derivative of ##\delta(x-x')## and lost more time than I'd like to admit on this.
 
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  • #8
By the way, I have just checked, the same results are obtained also if ##\psi## is quantized as a bosonic field, rather than fermionic.
 
  • #9
Yes I agree, though I suppose if we were to think about bosonic fields, perhaps the sign of ##e## should change as well?
 
  • #10
thatboi said:
Yes I agree, though I suppose if we were to think about bosonic fields, perhaps the sign of ##e## should change as well?
Why would the sign of ##e## need to change? Bosonic fields can have charge of either sign. (Consider the ##W^+## and ##W^-## fields in the Standard Model, for example, or charged pions.)
 
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FAQ: Heisenberg Equations of Motion for Electron in EM-field

What are the Heisenberg Equations of Motion?

The Heisenberg Equations of Motion are a set of equations in quantum mechanics that describe how the operators corresponding to observables evolve over time. They are given by the commutator of the Hamiltonian with the observable, scaled by the factor \( \frac{i}{\hbar} \), where \( \hbar \) is the reduced Planck constant.

How do the Heisenberg Equations of Motion apply to an electron in an electromagnetic field?

For an electron in an electromagnetic field, the Hamiltonian includes terms representing the kinetic energy of the electron and its interaction with the electromagnetic field. The Heisenberg Equations of Motion are used to derive the time evolution of the position and momentum operators of the electron in this field.

What is the role of the vector potential in the Heisenberg Equations of Motion for an electron in an EM-field?

The vector potential \( \mathbf{A} \) plays a crucial role in the Hamiltonian of an electron in an electromagnetic field. It modifies the momentum operator to \( \mathbf{p} - e\mathbf{A} \), where \( e \) is the electron charge. This altered momentum operator is then used in the Heisenberg Equations of Motion.

Can you provide a simple example of the Heisenberg Equations of Motion for an electron in a uniform magnetic field?

In a uniform magnetic field \( \mathbf{B} \), the vector potential \( \mathbf{A} \) can be chosen such that \( \mathbf{B} = \nabla \times \mathbf{A} \). For an electron in this field, the Heisenberg Equations of Motion for the position \( \mathbf{r} \) and momentum \( \mathbf{p} \) operators are:\[ \frac{d\mathbf{r}}{dt} = \frac{\mathbf{p} - e\mathbf{A}}{m} \]\[ \frac{d\mathbf{p}}{dt} = e\left( \frac{d\mathbf{r}}{dt} \times \mathbf{B} \right) \]These equations describe the cyclotron motion of the electron in the magnetic field.

What are the implications of the Heisenberg Equations of Motion for quantum systems in electromagnetic fields?

The Heisenberg Equations of Motion provide a framework for understanding the dynamics of quantum systems in electromagnetic fields. They allow us to predict how quantum observables change over time and are essential for studying phenomena such as quantum Hall effects, Landau levels, and the behavior of electrons in various potential fields.

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