Calculating the Radius & Energy of Bohr's Hydrogen Atom

In summary, the conversation discusses determining the radius of allowed orbits and calculating the first orbit for Bohr's model of the hydrogen atom. It also delves into showing the quantization of energy and calculating the energy of an electron on the first orbit. The calculations involve classical mechanics, the supposition that the electron does not emit photons, and the quantization of angular momentum. The final calculations result in the correct value for the energy of the electron on the first orbit, despite some initial algebra mistakes. There is also a brief discussion about the Rydberg constant and its relation to energy levels in the hydrogen atom.
  • #1
fluidistic
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Homework Statement


1)Determine the radius of the allowed orbits. Calculate the first orbit of Bohr's model for the hydrogen atom.
2)Show that the energy is quantized. Calculate the energy of an electron on the first orbit (fundamental state of hydrogen atom)

Homework Equations



[itex]L=n \hbar[/itex].
[itex]F=\frac{k(e^-) ^2}{R^2}[/itex]
[itex]F=m_e v^2/R[/itex]
[itex]k=\frac{1}{4\pi \varepsilon _0}[/itex].

The Attempt at a Solution


I used ideas of classical mechanics, combined with the supposition that the electron orbiting the nucleus doesn't emit photons and that the angular momentum is quantized.
I found out that [itex]v=\frac{n \hbar}{m_e R}[/itex] and that [itex]R=\frac{4\pi \varepsilon _0 n^2 \hbar ^2}{(e^-)^2m_e}[/itex]. I checked out in wikipedia and taking n=1 I indeed find the Bohr's radius, that's why I don't show all my arithmetics here.
I get that for n=1, [itex]R\approx 5.29177208 \times 10 ^{-11}m[/itex].
And that the velocity of the electron is about [itex]2187691.254 \frac{m}{s}[/itex], which is less than 10% of light's speed. Thus I can consider the classical momentum [itex]p=m_ev[/itex] as a good approximation for the momentum value of the electron. Or I can take [itex]\frac{m_e v^2}{2}[/itex] for the kinetic energy of the electron.
Precisely, this is taking this expression for the kinetic energy of the electron that I'm getting a problem for part 2).
So I answered part 1).
Now for part 2, E=T+V, where [itex]V=-\frac{k(e^-)^2}{R}[/itex].
Replacing T by [itex]\frac{m_e v^2}{2}[/itex], I reach that [itex]E=\frac{(e^-)^4m_e}{16 \pi ^2 \varepsilon _0 ^2n^2\hbar ^2}-\frac{(e^-)^4m_e}{16 \pi ^2 \varepsilon _0 ^2n^2\hbar ^2}=0[/itex].
In other words, the kinetic energy of the electron is worth minus the potential energy of the electron and thus its total energy is null. I know this is a wrong answer, I should find -13.6 eV for n=1, but I don't reach this.
Any help to spot my error(s) is welcome. I'm stuck on this since yesterday.

Edit: Nevermind, I found an algebra mistake for T by a factor 1/2. Now I think I'll reach the results.

Edit 2: Indeed, I find something (my calculator can't do the math, it shows E=0 because I'm guessing of an [itex]10^{-106}[/itex]) by hand that is of the order of [itex]-10^{-18}J[/itex] which is roughly of the order of -10 eV (compared to -13.6 eV) so I'm guessing that my expression is right.
 
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  • #2
It's correct, though you wrote it a bit confusingly :D

Since Coulomb force is the centripetal one,
[itex]\frac{Ze^2}{4\pi\epsilon_0 r^2}=\frac{mv^2}{r}\Rightarrow mv^2=\frac{Ze}{4\pi\epsilon_0 r}[/itex]
Now, [itex]E=K+V=\frac{mv^2}{2}-\frac{Ze}{4\pi\epsilon_0 r}=\frac{Ze}{2\cdot 4\pi\epsilon_0 r}-\frac{Ze}{4\pi\epsilon_0 r}=-\frac{Ze}{16\pi\epsilon_0 r}[/itex]

Substituting your expression for r in the previous equation, you get
[itex]E_n=-\frac{Ze^2 }{16\pi\epsilon_0 \frac{4\pi\epsilon_0 n^2\hbar^2}{Ze^2 m}}=-Z^2 m\left(\frac{e^2}{8\pi\epsilon_0\hbar}\right)^2
\frac{1}{n^2}=-Z^2 \frac{R_H}{n^2}[/itex] where [itex]R_H[/itex] is the Rydberg constant: [itex]R_H=13.6eV[/itex]
 
  • #3
DiracRules said:
It's correct, though you wrote it a bit confusingly :D

Since Coulomb force is the centripetal one,
[itex]\frac{Ze^2}{4\pi\epsilon_0 r^2}=\frac{mv^2}{r}\Rightarrow mv^2=\frac{Ze}{4\pi\epsilon_0 r}[/itex]
Now, [itex]E=K+V=\frac{mv^2}{2}-\frac{Ze}{4\pi\epsilon_0 r}=\frac{Ze}{2\cdot 4\pi\epsilon_0 r}-\frac{Ze}{4\pi\epsilon_0 r}=-\frac{Ze}{16\pi\epsilon_0 r}[/itex]

Substituting your expression for r in the previous equation, you get
[itex]E_n=-\frac{Ze^2 }{16\pi\epsilon_0 \frac{4\pi\epsilon_0 n^2\hbar^2}{Ze^2 m}}=-Z^2 m\left(\frac{e^2}{8\pi\epsilon_0\hbar}\right)^2
\frac{1}{n^2}=-Z^2 \frac{R_H}{n^2}[/itex] where [itex]R_H[/itex] is the Rydberg constant: [itex]R_H=13.6eV[/itex]
Thank you Mr. Dirac (may I ask you an autograph by the way?).
I am a bit confused with the Rydberg's constant. In wikipedia I read that [itex]R_{\infty }[/itex] in the case of the simplified hydrogen atom is worth [itex]\frac{m_e (e^-)^4}{8 \varepsilon _0 ^2 h^3 c}[/itex] which differs from our case.
 
  • #4
Probably my fault.

Here is the thing: the problem is that physicists usually tend to express all their constant in terms of energy (despite the original values are temperatures, wavelengths ...)
So, since it is easier to remember, I learned that [itex]R_\infty=13.6eV[/itex], that is, the lowest energy level of the hydrogen atom.

NB: in the previous note, I didn't write correctly, since I should have written [itex]R_\infty[/itex] instead of [itex]R_H[/itex]

Is that ok?
 
  • #5
I guess that the error is in the calculation of the potential energy.

Your approach seems mostly correct, but there are a few things to note:

1. In your calculation of the kinetic energy, you have used the classical expression for kinetic energy, which is not valid when dealing with small particles like electrons. Instead, you should use the relativistic expression for kinetic energy: T = (m_e c^2)/sqrt(1-(v/c)^2), where c is the speed of light. This will give you a slightly different value for the kinetic energy, and thus the total energy.

2. The potential energy expression you have used is also not quite correct. The correct expression for the potential energy of an electron in the hydrogen atom is V = -k(e^-)^2/R, where R is the distance between the electron and the nucleus. In your calculation, you have used the Bohr radius (a_0) instead of R. The Bohr radius is the average distance of the electron from the nucleus, but for the first orbit, the distance is actually a_0/2. This will result in a slightly different value for the potential energy, and thus the total energy.

Correcting these two issues should give you the correct value for the energy of the first orbit of the hydrogen atom. Keep in mind that this is still a simplified model and the actual energy may differ slightly due to quantum effects.
 

1. What is Bohr's model of the hydrogen atom?

Bohr's model is a simplified representation of the hydrogen atom, proposed by Danish physicist Niels Bohr in 1913. It states that electrons orbit the nucleus in circular paths at specific energy levels.

2. How do you calculate the radius of an electron in the hydrogen atom?

The radius of an electron in the hydrogen atom can be calculated using the formula r = n²h²/4π²me², where n is the principal quantum number, h is Planck's constant, m is the mass of the electron, and e is the elementary charge.

3. What is the significance of the radius in Bohr's model?

The radius represents the distance between the electron and the nucleus in the hydrogen atom. It also determines the energy level and stability of the electron in its orbit.

4. How do you calculate the energy of an electron in the hydrogen atom?

The energy of an electron in the hydrogen atom is calculated using the formula E = -13.6/n² eV, where n is the principal quantum number. This value represents the specific energy level at which the electron is orbiting the nucleus.

5. What is the relationship between the radius and energy in Bohr's model?

According to Bohr's model, the radius and energy of the electron in the hydrogen atom are inversely proportional. As the radius increases, the energy of the electron decreases, and vice versa. This relationship is known as the "Bohr radius" and is used to calculate the energy levels of other atoms as well.

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