Phy5645/Problem 1D sample: Difference between revisions

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Consider a particle of mass m in a three dimensional potential:
Consider a particle of mass m in a three dimensional potential:
<math>V(x,y,z)=X(x) + Y(y) + Z(z)</math>
<math>V(x,y,z) = X(x)+Y(y)+Z(z)\!</math>


Using the Schroedinger's equation show that we can treat the problem like three independent one-dimensional problems. Relate the energy of the three-dimensional state to the effective energies of one-dimensional problem.
Using the Schroedinger's equation show that we can treat the problem like three independent one-dimensional problems. Relate the energy of the three-dimensional state to the effective energies of one-dimensional problem.
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The Schroedinger's equation takes the form:
The Schroedinger's equation takes the form:
<math>-\frac{\hbar^2}{2m}\frac{d^2\psi(x,y,z)}{dx^2}+(X(x)+Y(y)+Z(z))\psi(x,y,z)=E\psi(x,y,z)</math>


:<math>-\frac{\hbar^2}{2m}\frac{d^2\psi(x,y,z)}{dx^2}+\left(X(x)+Y(y)+Z(z)\right)\psi(x,y,z)=E\psi(x,y,z)</math>




Assuming that <math>\psi</math> can be write like:
Assuming that <math>\psi\!</math> can be write like:
<math>\psi(x,y,z)=\Phi(x) \Delta(y) \Omega (z) </math>
:<math>\psi(x,y,z)=\Phi(x) \Delta(y) \Omega (z) \!</math>




So,
So,


<math>-\frac{\hbar^2}{2m}[ \frac{d^2\Phi(x)}{dx^2} \Delta(y) \Omega (z)   + \Phi(x)\frac{d^2\Delta(y)}{dy^2} \Omega (z)  +  \Phi(x) \Delta (y)\frac{d^2\Omega(z)}{dz^2}   ] + [X(x)+Y(y)+Z(z)]\Phi(x) \Delta(y) \Omega (z) = E\Phi(x) \Delta(y) \Omega (z)  </math>
:<math>
-\frac{\hbar^2}{2m} \left[ \frac{d^2\Phi(x)}{dx^2} \Delta(y) \Omega (z) + \Phi(x)\frac{d^2\Delta(y)}{dy^2} \Omega (z)  +  \Phi(x) \Delta (y)\frac{d^2\Omega(z)}{dz^2} \right] + \left[X(x)+Y(y)+Z(z)\right]\Phi(x) \Delta(y) \Omega (z) = E\Phi(x) \Delta(y) \Omega (z)  </math>




Dividing by <math>\psi(x,y,z) </math>
Dividing by <math>\psi(x,y,z) \!</math>
 
<math>-\frac{\hbar^2}{2m}\frac{1}{\Phi(x)}  \frac{d^2\Phi(x)}{dx^2}    + X(x)   
      -\frac{\hbar^2}{2m}\frac{1}{\Delta(y)} \frac{d^2\Delta(y)}{dy^2}  + Y(y)
      -\frac{\hbar^2}{2m}\frac{1}{\Omega(z)} \frac{d^2\Omega(z)}{dz^2}  + Z(z)      = E  </math>


:<math>
-\frac{\hbar^2}{2m} \frac{1}{\Phi(x)} \frac{d^2\Phi(x)}{dx^2} + X(x)
-\frac{\hbar^2}{2m} \frac{1}{\Delta(y)} \frac{d^2\Delta(y)}{dy^2} + Y(y)
-\frac{\hbar^2}{2m} \frac{1}{\Omega(z)} \frac{d^2\Omega(z)}{dz^2} + Z(z)
= E 
</math>


Perfectly we can separate the right hand side in three parts, where only one depends of x, only one of y and only one of z. Then each of these parts must be equal to a constant. So:
Perfectly we can separate the right hand side in three parts, where only one depends of x, only one of y and only one of z. Then each of these parts must be equal to a constant. So:


:<math>
-\frac{\hbar^2}{2m} \frac{1}{\Phi(x)} \frac{d^2\Phi(x)}{dx^2} + X(x) = E_x  </math>


<math>-\frac{\hbar^2}{2m}\frac{1}{\Phi(x)}  \frac{d^2\Phi(x)}{dx^2}    + X(x)    = Ex  </math>
:<math>
 
-\frac{\hbar^2}{2m} \frac{1}{\Delta(y)} \frac{d^2\Delta(y)}{dy^2} + Y(y) = E_y </math>
 
<math>-\frac{\hbar^2}{2m}\frac{1}{\Delta(y)} \frac{d^2\Delta(y)}{dy^2}   + Y(y)     = Ey  </math>
 
 
<math>-\frac{\hbar^2}{2m}\frac{1}{\Omega(z)} \frac{d^2\Omega(z)}{dz^2}  + Z(z)    = Ez </math>


:<math>
-\frac{\hbar^2}{2m} \frac{1}{\Omega(z)} \frac{d^2\Omega(z)}{dz^2} + Z(z) = E_z  </math>


Ex, Ey and Ez are constant where: <math> E = Ex+Ey+Ez  </math>
where E_x, E_y and E_z are constant and <math> E = E_x+E_y+E_z \!</math>




Hence the three-dimensional problem has been divided in three one-dimensional problems where the total energy E is the sum of the energies Ex, Ey and Ez in each dimension.
Hence the three-dimensional problem has been divided in three one-dimensional problems where the total energy E is the sum of the energies <math> E_x \!</math>, <math> E_y \!</math> and <math> E_z \!</math> in each dimension.

Revision as of 00:34, 5 December 2009

(Submitted by team 1. Based on problem 3.19 in Schaum's Theory and problems of Quantum Mechanics)

Consider a particle of mass m in a three dimensional potential:

Using the Schroedinger's equation show that we can treat the problem like three independent one-dimensional problems. Relate the energy of the three-dimensional state to the effective energies of one-dimensional problem.

______________________________________________________________________________________________________________________________________

The Schroedinger's equation takes the form:


Assuming that can be write like:


So,


Dividing by

Perfectly we can separate the right hand side in three parts, where only one depends of x, only one of y and only one of z. Then each of these parts must be equal to a constant. So:

where E_x, E_y and E_z are constant and


Hence the three-dimensional problem has been divided in three one-dimensional problems where the total energy E is the sum of the energies , and in each dimension.