An Introduction to Thermal Physics
An Introduction to Thermal Physics
1st Edition
ISBN: 9780201380279
Author: Daniel V. Schroeder
Publisher: Addison Wesley
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Chapter 6.1, Problem 6P
To determine

The probability of finding a hydrogen atom in 1st excited state at room temperature and also in the atmosphere of the star γUMa .

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Estimate the probability that a hydrogen atom at room temperature is in one of its first excited states (relative to the probability of being in the ground state). Don't forget to take degeneracy into account. Then repeat the calculation for a hydrogen atom in the atmosphere of the star y UMa, whose surface temperature is approximately 9500 K.
Consider a one dimensional atom trap with an ideal harmonic oscillator potential with the zero-point energy of 4 eV. Assume the temperature of zero Kelvin, 8 atoms in the trap and that interactions between atoms in the trap are negligible. Calculate the total energy of atoms in the trap if 0 atoms have spin 0. O atoms have spin 1/2. 3. atoms have spin 1. atoms have spin 3/2.
The three lowest energy levels of a hydrogen atom are -13.6 eV, -3.4 eV, and -1.5 eV. Assume that there is only one way to occupy any one of these levels. Calculate the relative probability that a hydrogen atom in thermal equilibrium in a star, at temperature T = 9674 K, is in its first excited state (at -3.4 eV) relative to its ground state (at -13.6 eV). Write your answer in exponential form. Recall that Boltzmann's constant can be written as 8.617 x 10-5 eV K-1.
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