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Fundamentals Of Physics
Found in: Page 1246

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Short Answer

On which quantum numbers does the energy of an electron depend in (a) a hydrogen atom and

(b) a vanadium atom?

  1. The quantum number that the energy of an electron depends in a hydrogen atom is the principal quantum number n .
  2. The quantum number that the energy of an electron depends in a vanadium atom is the principal quantum number n and l .
See the step by step solution

Step by Step Solution

Step 1: The given data

Atoms are Hydrogen ( Z = 1 ) and Vanadium ( Z = 23 ) .

Step 2: Understanding the concept of energy

Using the energy of an electron in the nth Bohr's orbit of an atom, we can calculate the energy of an electron of the required atom that are hydrogen-like species using their atomic number and the principal quantum number of the subshell where the electron is present. But for transition metals that are not hydrogen-like species, the energy of the electron also depends on the azimuthal number irrespective of the dependence of energy on the principal quantum number.

Formula:

The energy of an electron in the nth Bohr's orbit or shell of the atom,

E=-13.6Z2n2 ……….(i)

Step 3: a) Calculation of the energy in the hydrogen atom

According to the concept and equation (i), we can say that the energy of hydrogen or any other hydrogen-like species depends on the principal quantum number n .

Hence, it depends on the principal quantum number n .

Step 4: b) Calculation of energy in vanadium atom

Now, as Vanadium is not hydrogen-like species and is a transition metal, the energy of this atom due to transition depends on both the principal n and azimuthally quantum number l that is, the energy dependence is on the value n+l.

Hence, the energy of this atom depends on n and l .

Most popular questions for Physics Textbooks

Comet stimulated emission. When a comet approaches the Sun, the increased warmth evaporates water from the ice on the surface of the comet nucleus, producing a thin atmosphere of water vapor around the nucleus. Sunlight can then dissociate H2O molecules in the vapor to H atoms and OH molecules. The sunlight can also excite the OH molecules to higher energy levels.

When the comet is still relatively far from the Sun, the sunlight causes equal excitation to the E2 and E1 levels (Fig. 40-28a). Hence, there is no population inversion between the two levels. However, as the comet approaches the Sun, the excitation to the E1 level decreases and population inversion occurs. The reason has to do with one of the many wavelengths—said to be Fraunhofer lines—that are missing in sunlight because, as the light travels outward through the Sun’s atmosphere, those particular wavelengths are absorbed by the atmosphere.

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