When the two waves \( y_1 \) and \( y_2 \) are superposed, the resultant wave can be expressed as a combination of a carrier wave and a modulation wave. The carrier frequency is determined by the average of the angular frequencies, while the modulation frequency is determined by their difference.
\[ y_1 = A_0 \sin(kx - \omega t), \quad y_2 = A_0 \sin(\alpha kx - \beta \omega t) \]
The resultant wave is given by the superposition of \( y_1 \) and \( y_2 \):
\[ y_{\text{resultant}} = 2A_0 \cos\left(\frac{\beta \omega - \omega}{2} t\right) \sin\left(\frac{\beta \omega + \omega}{2} t\right) \]
For \( \alpha = \beta = 2 \), the carrier frequency becomes:
\[ \text{Carrier Frequency} = \frac{\omega + 2\omega}{2} = \frac{3}{2} \omega \]
Thus, the correct statement is that the carrier frequency of the resultant wave is \( \frac{3}{2} \omega \).
The center of a disk of radius $ r $ and mass $ m $ is attached to a spring of spring constant $ k $, inside a ring of radius $ R>r $ as shown in the figure. The other end of the spring is attached on the periphery of the ring. Both the ring and the disk are in the same vertical plane. The disk can only roll along the inside periphery of the ring, without slipping. The spring can only be stretched or compressed along the periphery of the ring, following Hookeβs law. In equilibrium, the disk is at the bottom of the ring. Assuming small displacement of the disc, the time period of oscillation of center of mass of the disk is written as $ T = \frac{2\pi}{\omega} $. The correct expression for $ \omega $ is ( $ g $ is the acceleration due to gravity): 
Given below are two statements: one is labelled as Assertion (A) and the other is labelled as Reason (R).
Assertion (A): Time period of a simple pendulum is longer at the top of a mountain than that at the base of the mountain.
Reason (R): Time period of a simple pendulum decreases with increasing value of acceleration due to gravity and vice-versa. In the light of the above statements.
choose the most appropriate answer from the options given below:

At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/mΒ³, which is dimensionally incorrect for a spectral density. The correct unit J/(mΒ³Β·Hz) or JΒ·s/mΒ³ is used here for the solution.)