A point source is emitting sound waves of intensity \( 16 \times 10^{-8} \, Wm^{-2} \) at the origin. The difference in intensity (magnitude only) at two points located at distances of 2 m and 4 m from the origin respectively will be _____ \( \times 10^{-8} \, Wm^{-2} \).
The intensity of sound waves from a point source decreases with the square of the distance from the source. The formula for intensity \( I \) at a distance \( r \) from a point source is given by:
\[ I = \frac{P}{4\pi r^2}, \] where \( P \) is the power of the source.
Given Values: Intensity at the origin \( I_0 = 16 \times 10^{-8} \, Wm^{-2} \). Distances: \( r_1 = 2 \, m \) and \( r_2 = 4 \, m \).
Intensity at Distances \( r_1 \) and \( r_2 \): The intensity at distance \( r_1 = 2 \, m \):
\[ I_1 = I_0 \left( \frac{r_0}{r_1} \right)^2 = 16 \times 10^{-8} \times \left( \frac{1}{2} \right)^2 = 16 \times 10^{-8} \times \frac{1}{4} = 4 \times 10^{-8} \, Wm^{-2}. \]
The intensity at distance \( r_2 = 4 \, m \):
\[ I_2 = I_0 \left( \frac{r_0}{r_2} \right)^2 = 16 \times 10^{-8} \times \left( \frac{1}{4} \right)^2 = 16 \times 10^{-8} \times \frac{1}{16} = 1 \times 10^{-8} \, Wm^{-2}. \]
Calculating the Difference in Intensity: The difference in intensity \( \Delta I \) between the two points:
\[ \Delta I = I_1 - I_2 = (4 \times 10^{-8} - 1 \times 10^{-8}) \, Wm^{-2} = 3 \times 10^{-8} \, Wm^{-2}. \]
Match the LIST-I with LIST-II
\[ \begin{array}{|l|l|} \hline \text{LIST-I} & \text{LIST-II} \\ \hline \text{A. Gravitational constant} & \text{I. } [LT^{-2}] \\ \hline \text{B. Gravitational potential energy} & \text{II. } [L^2T^{-2}] \\ \hline \text{C. Gravitational potential} & \text{III. } [ML^2T^{-2}] \\ \hline \text{D. Acceleration due to gravity} & \text{IV. } [M^{-1}L^3T^{-2}] \\ \hline \end{array} \]
Choose the correct answer from the options given below:
A small point of mass \(m\) is placed at a distance \(2R\) from the center \(O\) of a big uniform solid sphere of mass \(M\) and radius \(R\). The gravitational force on \(m\) due to \(M\) is \(F_1\). A spherical part of radius \(R/3\) is removed from the big sphere as shown in the figure, and the gravitational force on \(m\) due to the remaining part of \(M\) is found to be \(F_2\). The value of the ratio \( F_1 : F_2 \) is: 