Introduction To Quantum Mechanics
Introduction To Quantum Mechanics
3rd Edition
ISBN: 9781107189638
Author: Griffiths, David J., Schroeter, Darrell F.
Publisher: Cambridge University Press
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Chapter 4.2, Problem 4.20P

(a)

To determine

The potential energy function.

(b)

To determine

The Bohr radius for the earth-sun system.

(c)

To determine

Show that n=r0/ag and estimate the value of the quantum number n of the earth.

(d)

To determine

The amount of energy released if the earth made a transition to the next level (n1) and the wavelength of the emitted photon.

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Problem 3.36. Consider an Einstein solid for which both N and q are much greater than 1. Think of each oscillator as a separate "particle." (a) Show that the chemical potential is N+ - kT ln N (b) Discuss this result in the limits N > q and N « q, concentrating on the question of how much S increases when another particle carrying no energy is added to the system. Does the formula make intuitive sense?
Problem 2.15 In the ground state of the harmonic oscillator, what is the probability (correct to three significant digits) of finding the particle outside the classically allowed region? Hint: Classically, the energy of an oscillator is E = (1/2)ka² = (1/2)mw²a², where a is the amplitude. So the "classically allowed region" for an oscillator of energy E extends from -√2E/mw² to +√2E/mw². Look in a math table under "Normal Distribution" or "Error Function" for the numerical value of the integral.
Problem 2.14 In the ground state of the harmonic oscillator, what is the probability (correct to three significant digits) of finding the particle outside the classically allowed region? Hint: Classically, the energy of an oscillator is E = (1/2) ka² = (1/2) mo²a², where a is the amplitude. So the “classically allowed region" for an oscillator of energy E extends from –/2E/mw² to +/2E/mo². Look in a math table under “Normal Distribution" or "Error Function" for the numerical value of the integral, or evaluate it by computer.
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