Schrödinger Equation in the classical limit

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SUMMARY

The discussion focuses on the behavior of the Schrödinger Equation in the classical limit, specifically when the Planck constant (\hbar) approaches zero. It establishes that in this limit, the Schrödinger Equation reduces to the classical Hamilton-Jacobi equation, demonstrating the transition from quantum mechanics to classical physics. The key substitution involves expressing the wave function as \Psi(x, t) = R(x, t)e^{iS(x, t)/\hbar}, leading to the classical equation \frac{\partial S}{\partial t} + H(x, \frac{\partial S}{\partial x}) = 0. This transition is contingent upon the wave packet's width being significantly larger than the de Broglie wavelength.

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  • Knowledge of quantum mechanics fundamentals
  • Concept of de Broglie wavelength
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Erland
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I am currently trying to learn a little about quantum mechanics, although not on very detailed level. There is one thing I wonder:

What happens with the Schrödinger Equation in the classical limit, i.e. when either the mass of the particle tends to infinity or when Planck's constant tends to 0?
Somehow, this should be reduced to classical physics, similar to letting c tend to infinity in the Lorentz Transformation leads to the Galilei Transformation. But I cannot see how we get some classical equation from the Schrödinger Equation in a similar case...
 
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Erland said:
I am currently trying to learn a little about quantum mechanics, although not on very detailed level. There is one thing I wonder:

What happens with the Schrödinger Equation in the classical limit, i.e. when either the mass of the particle tends to infinity or when Planck's constant tends to 0?

Big mass does not imply classical object. So the classical limit, as you will see below, concerns only with Planck constant.
Start from the Schrödinger equation (if you know it):
i \hbar \frac{ \partial \Psi ( x , t )}{ \partial t } = H ( \hat{ x } , \hat{ p } ) \Psi ( x , t ) .
Now substitute
\Psi ( x , t ) = R( x , t ) e^{ i S ( x , t ) / \hbar } ,
in the Schrödinger equation, you find
\frac{ i \hbar }{ R } \frac{ \partial R }{ \partial t } = \frac{ \partial S }{ \partial t } + H ( \hat{ x } , \frac{ \partial S }{ \partial \hat{ x } } ) .
So formally, in the limit \hbar \rightarrow 0, you obtain the classical Hamilton-Jacobi equation
\frac{ \partial S }{ \partial t } + H ( x , \frac{ \partial S }{ \partial x } ) = 0 .
What really is happening in the classical limit is that, there is a wave packet of width much larger than the de Broglie wave length, in the detailed Scrodinger equation you will have
\frac{ \hbar^{ 2 } }{ 2 m } | \frac{ \nabla^{ 2 } R }{ R } | \ll | \frac{ ( \nabla S )^{ 2 } }{ 2 m } | .
 
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Thanks! I guess I have to look up Hamilton-Jacobi theory.
 

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