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Question: A \(\mu - meson\) (a charge \( - e\) , mass= \(270m\) where \(m\) is the mass of an electron) can be...

A μmeson\mu - meson (a charge e - e , mass= 270m270m where mm is the mass of an electron) can be captured by a proton to form a hydrogen-like “mesic” atom. Calculate the radius of the Bohr’s orbit, the binding energy, and the wavelength of the line in the Lyman series for such an atom. The mass of the proton is 1836 times the electron. The radius of the first Bohr’s orbit and the binding energy of the hydrogen are 0.529 angstroms and 13.6 eV, respectively. Take R=109678cm1R = 109678c{m^{ - 1}}.

Explanation

Solution

First calculate the reduced mass of the system, that is, the reduced mass of the μmeson\mu - meson and proton. With the help of reduced mass, Bohr’s first orbit radius and the binding energy can be calculated for the hydrogen-like atom.

Complete step by step answer:
Step 1:
First calculate the reduced mass of the system. Express the formula for the reduced mass of the two-particle system.
μ=mmeson×mpmmeson+mp\therefore \mu = \dfrac{{{m_{\text{meson}}} \times {m_p}}}{{{m_{\text{meson}}} + {m_p}}} , where mmeson{m_{\text{meson}}} is the mass of the μmeson\mu - meson and mp{m_p} is the mass of the proton.
Substitute mmeson=270m{m_{\text{meson}}} = 270m and mp=1836m{m_p} = 1836m , where mm is the mass of the electron.
μ=270m×1836m270m+1836m\therefore \mu = \dfrac{{270m \times 1836m}}{{270m + 1836m}}
μ=186m\Rightarrow \mu = 186m
Now express the formula for Bohr’s first orbit radius.
r1=h2124π2ke2Z\therefore {r_1} = \dfrac{{{h^2}{1^2}}}{{4{\pi ^2}k{e^2}Z}}
Now substitute Z=186mZ = 186m in the above expression.
r1=h24π2ke2186m\therefore {r_1} = \dfrac{{{h^2}}}{{4{\pi ^2}k{e^2}186m}}
r1=1186×0.529angstrom\Rightarrow {r_1} = \dfrac{1}{{186}} \times 0.529\text{angstrom}
r1=0.002844angstrom\Rightarrow {r_1} = 0.002844\text{angstrom}
This is the radius of the Bohr’s orbit of the system.

Step 2:
Now express the formula for the binding energy of the hydrogen-like atom's first orbit.
E1=2πk2e4μh212\therefore {E_1} = \dfrac{{2\pi {k^2}{e^4}\mu }}{{{h^2}{1^2}}}
Substitute the value of μ\mu .
E1=2πk2e4186mh212\therefore {E_1} = \dfrac{{2\pi {k^2}{e^4}186m}}{{{h^2}{1^2}}}
We know that the binding energy for the first orbit of the hydrogen Ehydrogen=2πk2e4mh212=13.6eV{E_{hydrogen}} = \dfrac{{2\pi {k^2}{e^4}m}}{{{h^2}{1^2}}} = 13.6eV , therefore,
E1=186×13.6eV\therefore {E_1} = 186 \times 13.6eV
E1=186×13.6eV{E_1} = 186 \times 13.6eV
This is the binding energy of the hydrogen-like atom.

Step 3:
In the Layman series, the initial position of the electron may be ni=2,3,4,........{n_i} = 2,3,4,........ . The transition ends when the electron reaches the ground state. Express the formula for the wavelength of the line in the Lyman series for hydrogen-like atoms.
1λ=R(1nf21ni2)\therefore \dfrac{1}{\lambda } = R\left( {\dfrac{1}{{{n_f}^2}} - \dfrac{1}{{{n_i}^2}}} \right) , where RR is Rydberg constant, nf{n_f} is the final position of the electron, and ni{n_i} is the initial position of the electron. Substitute Rydberg constant for the reduced mass, nf=1{n_f} = 1 and ni=2{n_i} = 2
1λ=Rμ(112122)\therefore \dfrac{1}{\lambda } = {R_\mu }\left( {\dfrac{1}{{{1^2}}} - \dfrac{1}{{{2^2}}}} \right)
1λ=34Rμ\Rightarrow \dfrac{1}{\lambda } = \dfrac{3}{4}{R_\mu }
λ=43Rμ\Rightarrow \lambda = \dfrac{4}{{3{R_\mu }}} ----(1)

Step 4:
We know that the Rydberg constant for reduced mass is expressed as
Rμ=2π2k2e2μch3\therefore {R_\mu } = \dfrac{{2{\pi ^2}{k^2}{e^2}\mu }}{{c{h^3}}}
Substitute the value of μ\mu in the above expression
Rμ=2π2k2e2186mch3\therefore {R_\mu } = \dfrac{{2{\pi ^2}{k^2}{e^2}186m}}{{c{h^3}}}
Rμ=2π2k2e2mch3×186\Rightarrow {R_\mu } = \dfrac{{2{\pi ^2}{k^2}{e^2}m}}{{c{h^3}}} \times 186
Rμ=R186\therefore {R_\mu } = R186
Substitute the value of Rμ{R_\mu } in the equation (1).
λ=43×186R\therefore \lambda = \dfrac{4}{{3 \times 186R}}
Substitute the value R=10967800m1R = 10967800{m^{ - 1}} given in the question.
λ=43×186×10967800\therefore \lambda = \dfrac{4}{{3 \times 186 \times 10967800}}
λ=653.6angstrom\lambda = 653.6\text{angstrom}
This is the wavelength of the line in the Lyman series.

Note: It is a quantity that allows the two-body problem to be solved as if it were a one-body problem. Note, however, that the mass determining the gravitational force is not reduced. In the computation, one mass can be replaced with the reduced mass, if this is compensated by replacing the other mass with the sum of both masses.