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A wavelength of 4.653 µm is observed in a hydrogen spectrum for a transition that ends in thenf= 5 level. What was ni for the initial level of the electron?

Short Answer

Expert verified

The initial energy level of the transition is found to be 7.

Step by step solution

01

Define the Rydberg constant

The Rydberg constant is the lowest-energy photon capable of ionising the hydrogen atom from its ground state, or the highest wavenumber of any photon that may be released from the hydrogen atom.

Consider the formula for the charge to mass ratio in the electron and the proton as follows:

\[\begin{array}{c}\frac{{{q_e}}}{{{m_e}}} = - 1.76 \times {10^{11}}\;\frac{{\rm{C}}}{{{\rm{kg}}}}\\\frac{{{q_p}}}{{{m_p}}} = 9.57 \times {10^7}\;\frac{{\rm{C}}}{{{\rm{kg}}}}\end{array}\]

Here,\[{m_e} = 9.11 \times {10^{ - 31}}\;{\rm{kg}}\]is the mass of the electron and\[{m_p} = 1.67 \times {10^{ - 27}}\;{\rm{kg}}\]is the mass of the proton.

Consider the formula for the Bohr's theory of hydrogen atom.

\[\frac{1}{\lambda } = R\left( {\frac{1}{{n_f^2}} - \frac{1}{{n_i^2}}} \right)\]

Here, wavelength of the emitted electromagnetic radiation is \[\lambda \], and the Rydberg constant is \[R = 1.097 \times {10^7}\;{{\rm{m}}^{ - 1}}\].

02

Determine the ni  for the transition occurred. 

Consider the wavelength and energy level equation is solved as:

\[\begin{array}{l}\frac{1}{\lambda } = R\left( {\frac{1}{{n_f^2}} - \frac{1}{{n_i^2}}} \right)\\\frac{1}{\lambda } = R\left( {\frac{1}{{25}} - \frac{1}{{n_i^2}}} \right)\\\frac{1}{{n_i^2}} = \frac{1}{{25}} - \frac{1}{{\lambda R}}\end{array}\]

Substitute the values and solve as:

\[\begin{array}{l}\frac{1}{{n_i^2}} = \frac{1}{{25}} - \frac{1}{{1.097 \times {{10}^7}\;{m^{ - 1}} \times 4.653 \times {{10}^{ - 6}}\;m.}}\\{n_i} \approx 7\end{array}\]

Therefore, the initial energy level of the transition is found to be 7 .

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Most popular questions from this chapter

What two pieces of evidence allowed the first calculation of me, the mass of the electron?

(a) The ratios \[\frac{{{{\bf{q}}_{\bf{e}}}}}{{{{\bf{m}}_{\bf{e}}}}}\]and \[\frac{{{{\bf{q}}_{\bf{p}}}}}{{{{\bf{m}}_{\bf{p}}}}}\].

(b) The values of qe and EB.

(c) The ratio \[\frac{{{{\bf{q}}_{\bf{e}}}}}{{{{\bf{m}}_{\bf{e}}}}}\]and qe.

Justify your response.

(a) How many angles canLmake with the z-axis for anl = 2electron?

(b) Calculate the value of the smallest angle.

The wavelength of the four Balmer series lines for hydrogen are found to be 410.3, 434.2, 486.3, and 656.5 nm. What average percentage difference is found between these wavelength numbers and those predicted by\[\frac{{\bf{1}}}{{\bf{\lambda }}}{\bf{ = R}}\left( {\frac{{\bf{1}}}{{{\bf{n}}_{\bf{f}}^{\bf{2}}}}{\bf{ - }}\frac{{\bf{1}}}{{{\bf{n}}_{\bf{i}}^{\bf{2}}}}} \right){\bf{?}}\]It is amazing how well a simple formula (disconnected originally from theory) could duplicate this phenomenon.

Consider the Doppler-shifted hydrogen spectrum received from a rapidly receding galaxy. Construct a problem in which you calculate the energies of selected spectral lines in the Balmer series and examine whether they can be described with a formula like that in the equation\[\frac{{\rm{1}}}{{\rm{\lambda }}}{\rm{ = R}}\left( {\frac{{\rm{1}}}{{{\rm{n}}_{\rm{f}}^{\rm{2}}}}{\rm{ - }}\frac{{\rm{1}}}{{{\rm{n}}_{\rm{i}}^{\rm{2}}}}} \right){\rm{,}}\]but with a different constant R.

Which of the following spectroscopic notations are allowed (that is, which violate none of the rules regarding values of quantum numbers)?

(a) \[{\bf{1}}{{\bf{s}}^{\bf{1}}}\](b) \[{\bf{1}}{{\bf{d}}^{\bf{3}}}\] (c)\[{\bf{4}}{{\bf{s}}^{\bf{2}}}\](d)\[{\bf{3}}{{\bf{p}}^{\bf{7}}}\] (e)\[{\bf{6}}{{\bf{h}}^{{\bf{20}}}}\]

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