Assertion (A): In solid each electron will have a different energy level.
Reason (R): In solid crystal each electron has a unique position and no two electrons see exactly the same pattern of surrounding charges.
Due to the Pauli exclusion principle, no two electrons can occupy the same quantum state. In a solid, each electron experiences a unique electrostatic environment. Thus, Assertion (A) is true, and Reason (R) provides the correct explanation for it.
The wavelength of Lyman series of hydrogen atom appears in
Lyman series corresponds to transitions to the ground state (\(n=1\)). These high-energy transitions emit radiation in the ultraviolet region of the spectrum.
The ionisation potential of hydrogen is 13.6 V. The energy required to remove an electron from the third orbit of hydrogen is
The energy of an electron in the \(n\)-th orbit of hydrogen is given by \(E_n = -frac{13.6}{n^2}\text{ eV}\). For \(n=3\), \(E_3 = -frac{13.6}{9} = -1.51\text{ eV}\). Thus, the energy required to remove it is 1.51 eV.
In a hypothetical situation, all the atoms in a hydrogen sample are excited to same state. During de-excitation, photon with lowest energy was found to have \(0.66\text{ eV}\). The photon with the highest energy will have energy equal to
For hydrogen atom, \(E_n - E_{n-1} = 0.66\text{ eV}\) corresponds to \(n = 5\) to \(n = 4\) transition (since \(E_5 - E_4 = -0.85 - (-1.51) = 0.66\text{ eV}\)). The highest energy photon is emitted for transition from \(n = 5\) to \(n = 1\), which is \(E_5 - E_1 = -0.85 - (-13.6) = 12.75\text{ eV}\).
The wavelength of Balmer series of hydrogen atom appears in
The transitions in the Balmer series end on \( n = 2 \). The wavelengths of these transitions lie in the range of 380 nm to 700 nm, which belongs to the visible region of the electromagnetic spectrum.
An electron in a hydrogen atom makes a transition from \(n = n_1\) to \(n = n_2\). The time period of revolution of the electron in the initial state is eight times that in final state. The possible value of \(n_1\) and \(n_2\) are
The orbital period is proportional to \(n^3\). Since \(T_1 = 8 T_2\), we must have \(n_1^3 = 8 n_2^3\), which gives \(n_1 = 2n_2\). Thus, \(n_1 = 4\) and \(n_2 = 2\) is correct.
When an $\alpha$ particle of mass m moving with velocity v bombards on a heavy nucleus of charge ‘Ze’, its distance of closest approach from the nucleus depends on mass:
(2016 – I)
At the distance of closest approach $r_0$, kinetic energy is converted to potential energy. $\frac{1}{2} m v^2 = \frac{1}{4\pi\epsilon_0} \frac{(2e)(Ze)}{r_0}$. Rearranging gives $r_0 = \frac{4 Z e^2}{4\pi\epsilon_0 m v^2}$, which shows $r_0 \propto \frac{1}{m}$.
An alpha nucleus of energy $\frac{1}{2}mv^2$ bombards a heavy nuclear target of charge Ze. Then the distance of closest approach for the alpha nucleus will be proportional to:
(2010 Pre)
The distance of closest approach is found by equating kinetic energy to electrostatic potential energy: $K = \frac{1}{4\pi\epsilon_0} \frac{(2e)(Ze)}{r_0}$. Since $K = \frac{1}{2} m v^2$, we have $r_0 \propto \frac{1}{m}$.
In a Rutherford scattering experiment, when a projectile of charge $z_1$ and mass $M_1$ approaches a target nucleus of charge $z_2$ and mass $M_2$, the distance of closest approach is $r_0$. The energy of the projectile is
(2009)
At the distance of closest approach $r_0$, the entire kinetic energy of the projectile is converted into electrostatic potential energy. Energy $E = \frac{1}{4\pi\epsilon_0} \frac{z_1 z_2}{r_0}$. Thus, the energy is directly proportional to the product of charges $z_1 z_2$.