Modern Physics - NEET Physics Chapterwise MCQs & PYQs

NEET Modern Physics MCQs & PYQs

Question 301:

easy

The wavelength of the first line of Lyman series for hydrogen atom is equal to that of the second line of Balmer series for a hydrogen like ion. The atomic number Z of hydrogen like ion is:

(2011 Pre)

For first line of Lyman for H-atom ($n=2 \rightarrow 1$), $1/\lambda = R(1/1^2 - 1/2^2) = 3R/4$. For second line of Balmer for ion ($n=4 \rightarrow 2$), $1/\lambda = Z^2 R(1/2^2 - 1/4^2) = Z^2 R(3/16)$. Equating them gives $3R/4 = Z^2 R(3/16) \Rightarrow Z^2 = 4 \Rightarrow Z = 2$.

Question 302:

easy

The electron in the hydrogen atom jumps from excited state (n = 3) to its ground state (n = 1) and the photons thus emitted irradiate a photosensitive material. If the work function of the material is 5.1 eV, the stopping potential is estimated to be: (the energy of the electron in $n^{th}$ state)

(2010 Mains)

Energy of emitted photon $E = E_3 - E_1 = -1.51 - (-13.6) = 12.09 eV$. Using Einstein's photoelectric equation, max kinetic energy $K_{max} = E - \phi = 12.09 - 5.1 = 6.99 eV \approx 7 eV$. Hence, the stopping potential is $7 V$.

Question 303:

easy

The energy of a hydrogen atom in the ground state is -13.6 eV. The energy of a $He^+$ ion in the first excited state will be:

(2010 Pre)

The energy of an electron in a hydrogen-like ion is $E_n = -13.6 \frac{Z^2}{n^2} eV$. For a $He^+$ ion, $Z=2$. The first excited state corresponds to $n=2$. Thus, $E_2 = -13.6 \frac{2^2}{2^2} = -13.6 eV$.

Question 304:

easy

According to Bohr’s principle, the relation between principal quantum number (n) and radius of orbit (r) is

(1996)

The radius of the nth Bohr orbit is given by $r_n = \frac{n^2 h^2 \epsilon_0}{\pi m Z e^2}$. This shows that the radius is directly proportional to the square of the principal quantum number, so $r \propto n^2$.

Question 305:

easy

An electron makes a transition from orbit $n = 4$ to the orbit $n = 2$ of a hydrogen atom. What is the wavelength of the emitted radiations? (R – Rydberg’s constant)

(1995)

Using Rydberg's formula $\frac{1}{\lambda} = R \left(\frac{1}{n_1^2} - \frac{1}{n_2^2}\right)$, we substitute $n_1=2$ and $n_2=4$. $\frac{1}{\lambda} = R \left(\frac{1}{4} - \frac{1}{16}\right) = \frac{3R}{16}$. This gives $\lambda = \frac{16}{3R}$.

Question 306:

easy

When a hydrogen atom is raised from the ground state to an excited state,

(1995)

Kinetic energy $K.E. \propto \frac{1}{n^2}$, so it decreases as $n$ increases. Total energy $E = -\frac{13.6}{n^2} eV$ increases (becomes less negative). Since $P.E. = 2E$, potential energy also becomes less negative, meaning it increases.

Question 307:

easy

Hydrogen atoms are excited from ground state of the principle quantum number 4. Then the number of spectral lines observed will be:

(1993)

The number of possible spectral lines emitted when transitioning from the nth state to the ground state is $\frac{n(n-1)}{2}$. For $n=4$, the number of lines is $\frac{4 \times 3}{2} = 6$.

Question 308:

easy

Which source is associated with a line emission spectrum?

(1993)

Line emission spectra are characteristic of excited atoms in low-pressure gases. A neon street sign contains low-pressure neon gas which, when excited, emits a characteristic line spectrum.

Question 309:

easy

In terms of Bohr radius $a_0$, the radius of the second Bohr orbit of a hydrogen atom is given by:

(1992)

The radius of the nth Bohr orbit for a hydrogen atom is $r_n = a_0 n^2$. For the second orbit ($n=2$), the radius is $r_2 = a_0 (2^2) = 4a_0$.

Question 310:

easy

Energy E of a hydrogen atom with principal quantum number n is given by $E = \frac{-13.6}{n^2} eV$. The energy of a photon ejected when the electron jumps from n = 3 state to n = 2 state of hydrogen is approximately:

(2004)

The energy of the emitted photon is $\Delta E = 13.6 \left(\frac{1}{2^2} - \frac{1}{3^2}\right) = 13.6 \left(\frac{1}{4} - \frac{1}{9}\right) eV$. This gives $\Delta E = 13.6 \times \frac{5}{36} = 1.88 eV \approx 1.9 eV$.