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Q16E

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Modern Physics
Found in: Page 556
Modern Physics

Modern Physics

Book edition 2nd Edition
Author(s) Randy Harris
Pages 633 pages
ISBN 9780805303087

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Short Answer

In non-relavistic quantum mechanics, governed by the Schrodinger equation, the probability of finding a particle does not change with time.

(a)

Prove it, Begin with the time derivative of the total probability

ddtΨ*(x,t)Ψ'(x,t)dx=(Ψ(x,t)tΨ*(x,t)+Ψ*(x,t)tΨ(x,t))dx

Then use the Schrodinger equation to eliminate the partial time derivatives, integrate by parts, and show that the result is zero. Assume that the particle is well localised, so that ψ and ψxare 0 when evaluated at .±

(b) Does this procedure lead to the same conclusion if Wave function obeyKlein-Gordon rather than Shrodinger equation? Why and why not?

(a) The integrals from the two integrals by parts cancel each other, and the result is 0.

(b) It will not work if the wave function obeys Klein-Gordon equations.

See the step by step solution

Step by Step Solution

Step 1: Given data

The given integral isddtΨ*(x,t)Ψ'(x,t)dx=(Ψ(x,t)tΨ*(x,t)+Ψ*(x,t)tΨ(x,t))dx .

Step 2: Concept of the symmetric and asymmetric wave equation

The symmetric wave function is given as,

tΨ(x,t)=i22m2x2Ψ(x,t)

The Anti-symmetric wave function is given as,

tΨ*(x,t)=i22m2x2Ψ*(x,t)

Step 3: Proof of the integrals from the two integrals by parts cancel each other

(a)

The time derivative of the probability density function is given, as shown below.

ddtΨ*Ψdx=(ΨtΨ*+Ψ*tΨ)dx=(Ψi22m2x2Ψ*+Ψ*i22m2x2Ψ)dx=i22mΨx(xΨ*)dx+i22mΨ*x(xΨ)dx=i22m(ΨxΨ*+xΨ*(xΨ)dx)+i22m(Ψ*dxΨ+xΨ(xΨ*)dx)

The integrals from the two integrals by parts, and we obtain:

.ddtΨ*Ψdx=0

The integrals from the two integrals by parts cancel each other, and the result is 0 .

Step 4: Explanation of wave function obeying Klein-Gordon equation lead to the same result or not

(b)

It will not work if the wave function obeys the Klein-Gordon equation.

Because the first-time derivative of the wave function does not appear in the equations.

So we cannot trade them into space derivatives.

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