Recall the Bohr Model Energy Levels for Hydrogen:
According to the Bohr model, the energy of an electron in the \(n^{th}\) orbit of a hydrogen atom is given by the formula: \[ E_n = -\frac{13.6}{n^2} \, \text{eV} \] where \(n\) is the principal quantum number (\(n = 1, 2, 3, ...\)).
Determine the Principal Quantum Number (n):
We are given that the total energy of the electron is \(E = -3.4\) eV. We can use the energy formula to find the value of \(n\) corresponding to this energy level: \[ -3.4 \, \text{eV} = -\frac{13.6}{n^2} \, \text{eV} \] Divide both sides by -1 eV: \[ 3.4 = \frac{13.6}{n^2} \] Solve for \(n^2\): \[ n^2 = \frac{13.6}{3.4} \] \[ n^2 = 4 \] Take the square root (since \(n\) must be positive): \[ n = 2 \] So, the electron is in the second energy level (n=2).
Recall Bohr's Angular Momentum Quantization Condition:
One of the postulates of the Bohr model is that the angular momentum \(L\) of an electron orbiting the nucleus is quantized and is given by: \[ L_n = n \frac{h}{2\pi} \] where \(n\) is the principal quantum number and \(h\) is Planck's constant.
Calculate the Angular Momentum:
Substitute the value \(n=2\) into the angular momentum formula: \[ L_2 = 2 \times \frac{h}{2\pi} \] Simplify the expression: \[ L_2 = \frac{2h}{2\pi} = \frac{h}{\pi} \]
The angular momentum of the electron in the state with energy -3.4 eV (which corresponds to n=2) is \( \frac{h}{\pi} \).
So, the correct option (A): \(\frac h \pi\)
Given:
In Bohr's model, the angular momentum of the electron in the nth orbit is given by:
\( L = n \cdot \frac{h}{2\pi} \)
For n = 2:
\( L = 2 \cdot \frac{h}{2\pi} = \frac{h}{\pi} \)
✅ Correct Answer: \(\frac{h}{\pi}\)
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
For the hydrogen spectrum,the wavelength in Balmer series is given by \(\frac{1}{λ}\)=R(\(\frac{1}{n_{1}^{2}}\)-\(\frac{1}{n_{2}^{2}}\)) where λ= wavelength and R is Rydberg constant. What are the values of n1 and n2,for the longest wavelength in the Balmer series?
Kepler's second law (law of areas) of planetary motion leads to law of conservation of