Solutions of of the time-independent Schrodinger eq.

In summary, in order to show that \psi_1 + \psi_2 and c*\psi_1 are also solutions of the TISE with energy E, we can use the linearity of the operator and the fact that \psi_1 and \psi_2 are both solutions with energy E.
  • #1
xago
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Homework Statement



Supposed that [tex]\psi[/tex]1 and [tex]\psi[/tex]2 are two different solutions of the TISE with the same energy E.

a) show that [tex]\psi[/tex]1 + [tex]\psi[/tex]2 is also a solution with energy E.
b) show that c*[tex]\psi[/tex]1 is also a solution with energy E.

Homework Equations



TISE: (-[tex]\hbar[/tex]/2m)*[tex]\nabla[/tex]^2*[tex]\psi[/tex](r) +V(r)*[tex]\psi[/tex](r) = E*[tex]\psi[/tex](r)

The Attempt at a Solution



My first thought was to solve by substitution but since it doesn't give us the 2 solutions as a function I can't do that. Should I just find 2 different solutions and plug them into the TISE to see if they satisfy? I feel I am missing a rule or a postulate to solve this with.

P.S. I am very new to QM, be gentle
 
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  • #2
xago said:

Homework Statement



Supposed that [tex]\psi[/tex]1 and [tex]\psi[/tex]2 are two different solutions of the TISE with the same energy E.

a) show that [tex]\psi[/tex]1 + [tex]\psi[/tex]2 is also a solution with energy E.
b) show that c*[tex]\psi[/tex]1 is also a solution with energy E.

Homework Equations



TISE: (-[tex]\hbar[/tex]/2m)*[tex]\nabla[/tex]^2*[tex]\psi[/tex](r) +V(r)*[tex]\psi[/tex](r) = E*[tex]\psi[/tex](r)

The Attempt at a Solution



My first thought was to solve by substitution but since it doesn't give us the 2 solutions as a function I can't do that. Should I just find 2 different solutions and plug them into the TISE to see if they satisfy? I feel I am missing a rule or a postulate to solve this with.

P.S. I am very new to QM, be gentle

If [tex]\psi_1[/tex] is a solution of the TISE with energy E, what must

[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_1(r) [/tex]

equal? You don't need to know the functional form of [tex]\psi_1(r)[/tex] to answer this.
 
  • #3
[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_1(r)[/tex] = E*[tex]\psi[/tex]1

I don't see what this proves though, isn't the equation just re-arranged?
 
  • #4
xago said:
[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_1(r)[/tex] = E*[tex]\psi[/tex]1

I don't see what this proves though, isn't the equation just re-arranged?

Well it's reiterating what information you're given. The problem wants you to compute

[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) (\psi_1(r)+\psi_2(r))[/tex]

and

[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) ( c \psi_1(r)).[/tex]
 
  • #5
[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_1(r) = E\psi_1(r)[/tex]
[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_2(r) = E\psi_2(r)[/tex]

therefore [tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) (\psi_1(r)+\psi_2(r)) = E(\psi_1(r)+\psi_2(r)) ?[/tex]

It just doesn't feel like I'm proving anything.

Edit*Perhaps I just have to show that E[f(x)] is a linear operator? (where f(x) would be [tex]\psi[/tex])
 
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  • #6
xago said:
[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_1(r) = E\psi_1(r)[/tex]
[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_2(r) = E\psi_2(r)[/tex]

therefore [tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) (\psi_1(r)+\psi_2(r)) = E(\psi_1(r)+\psi_2(r)) ?[/tex]

It just doesn't feel like I'm proving anything.

It's not a really deep problem. You're just verifying that the wave equation is linear.

Edit*Perhaps I just have to show that E[f(x)] is a linear operator? (where f(x) would be [tex]\psi[/tex])

E is a scalar, I don't think you'd be expected to prove that multiplication by a scalar is a linear operation.
 
  • #7
xago said:
[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_1(r) = E\psi_1(r)[/tex]
[tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_2(r) = E\psi_2(r)[/tex]

therefore [tex]\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) (\psi_1(r)+\psi_2(r)) = E(\psi_1(r)+\psi_2(r)) ?[/tex]

It just doesn't feel like I'm proving anything.
You're supposed to show how what's after "therefore" follows from the first two lines.
 
  • #8
[tex]
\left[\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_1(r) = E\psi_1(r)\right]+
[/tex] [tex]
\left[\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \psi_2(r) = E\psi_2(r)\right]
[/tex]
[tex]
\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \left(\psi_1(r)+\psi_2(r)\right) = E\psi_1(r) + E\psi_2(r)
[/tex]
Since they both have the same E, it can be factored out:
[tex]
=\left(-\frac{\hbar}{2m}\nabla^2 + V(r) \right) \left(\psi_1(r)+\psi_2(r)\right) = E\left(\psi_1(r) + \psi_2(r)\right)
[/tex]

??
 
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  • #9
It's clear you understand conceptually what's going on, but you want to write it down in a clear, organized way. A lot of students have trouble writing down a proof because it seems so obvious.

To show [itex]\psi_1(\vec{r})+\psi_2(\vec{r})[/itex] is a solution means to show that

[tex]\left[-\frac{\hbar}{2m}\nabla^2 + V(\vec{r}) \right] \left(\psi_1(\vec{r})+\psi_2(\vec{r})\right) = E(\psi_1(\vec{r})+\psi_2(\vec{r}))[/tex]

For problems like this, it's good to start with one side of the equation, apply concepts one at a time, and show what you get after each step until you end up at the other side of the equation.

[tex]\begin{align*}
\left[-\frac{\hbar}{2m}\nabla^2 + V(r) \right] \left(\psi_1(r)+\psi_2(r)\right) &= \cdots \\
& = \cdots \\
&& \vdots \\
&= E(\psi_1(\vec{r})+\psi_2(\vec{r}))
\end{align*}[/tex]

In the first step, you'd use the linearity of

[tex]\left[-\frac{\hbar}{2m}\nabla^2 + V(r) \right][/tex]

In the next step, you'd use the fact that [itex]\psi_1[/itex] and [itex]\psi_2[/itex] are solutions with energy E, and so on.
 
  • #10
I understand now, thanks for your help!
 

FAQ: Solutions of of the time-independent Schrodinger eq.

1. What is the time-independent Schrodinger equation?

The time-independent Schrodinger equation is a fundamental equation in quantum mechanics that describes the behavior of a quantum system in terms of its energy and wave function. It is used to calculate the allowed energy levels and corresponding wave functions of a quantum system.

2. How is the time-independent Schrodinger equation solved?

The time-independent Schrodinger equation is solved by finding the eigenvalues and eigenfunctions of the Hamiltonian operator, which represents the total energy of the system. These eigenvalues and eigenfunctions correspond to the allowed energy levels and wave functions of the system.

3. What are the assumptions made in the time-independent Schrodinger equation?

The time-independent Schrodinger equation assumes that the system is in a stationary state, meaning that its properties do not change over time. It also assumes that the system is isolated and not affected by external forces or interactions.

4. How does the time-independent Schrodinger equation relate to the Heisenberg uncertainty principle?

The time-independent Schrodinger equation is a mathematical representation of the Heisenberg uncertainty principle, which states that the more precisely we know the position of a particle, the less precisely we can know its momentum, and vice versa. The wave function in the Schrodinger equation describes the probability of finding a particle in a certain position, and the eigenvalues represent the possible values of its momentum.

5. What are some applications of the time-independent Schrodinger equation?

The time-independent Schrodinger equation is used in many areas of physics, including atomic and molecular physics, solid state physics, and nuclear physics. It is also essential for understanding phenomena such as quantum tunneling, quantum entanglement, and superposition, which have important applications in quantum computing and cryptography.

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