Chapter 18: Problem 646
Explain the following: Pauli exclusion principle and Hund's rule.
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Chapter 18: Problem 646
Explain the following: Pauli exclusion principle and Hund's rule.
These are the key concepts you need to understand to accurately answer the question.
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Get started for freeDetermine the de Broglie wavelength of an electron (mass \(=9.11 \times 10^{-28} \mathrm{~g}\) ) having a kinetic energy of \(100 \mathrm{eV}\)
Under ordinary conditions of temperature and pressure, nitrogen gas exists as diatomic molecules \(\left(\mathrm{N}_{2}\right) .\) As a result of its electronic configuration, \(\mathrm{N}_{2}\) is very inert and requires extreme conditions before it will react with any other species. What is the electronic ground state configuration of a nitrogen atom (atomic number \(=7) ?\)
Write possible sets of quantum numbers for electrons in the second main energy level.
What wavelength of light is needed to excite an electron in a \(0.2\) nanometer ( \(1 \mathrm{~nm}=10^{-9} \mathrm{~m}\) ) box from the ground state to the second excited state? What wavelength of light is emitted when the same electron falls from the second excited state to the first excited state?
The Rydberg - Ritz equation governing the spectral lines of hydrogen is \((1 / \lambda)=\mathrm{R}\left[\left(1 / \mathrm{n}_{1}{ }^{2}\right)-\left(1 / \mathrm{n}_{2}{ }^{2}\right)\right]\), where \(\mathrm{R}\) is the Rydberg constant, \(\mathrm{n}_{1}\) indexes the series under consideration \(\left(\mathrm{n}_{1}=1\right.\) for the Lyman series, \(\mathrm{n}_{1}=2\) for the Balmer series, \(\mathrm{n}_{1}=3\) for the Paschen series \(), \mathrm{n}_{2}=\mathrm{n}_{1}+1, \mathrm{n}_{1}+2, \mathrm{n}_{1}+3, \ldots\) indexes the successive lines in a series, and \(\lambda\) is the wave- length of the line corresponding to index \(\mathrm{n}_{2}\). Thus, for the Lyman series, \(\mathrm{n}_{1}=1\) and the first two lines are \(1215.56 \AA\left(\mathrm{n}_{2}=\mathrm{n}_{1}+1=2\right)\) and \(1025.83 \AA\left(\mathrm{n}_{2}=\mathrm{n}_{1}+2=3\right)\) Using these two lines, calculate two separate values of the Rydberg constant. The actual value of this constant is \(\mathrm{R}=109678 \mathrm{~cm}^{-1}\)
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