Consider the Semi-circular Arc of the Wire:
Length of the semi-circular arc: \( L = \pi R \), where \( R \) is the radius of the semicircle.
Mass per unit length of the wire, \( \lambda = \frac{M}{L} = \frac{M}{\pi R} \).
Gravitational Force Element \( dF \):
Consider a small element \( dl \) of the arc at an angle \( \theta \) from the center, with a mass \( dm \):
\[ dm = \lambda dl = \frac{M}{\pi R} \times R d\theta = \frac{M}{\pi} d\theta \]
The gravitational force \( dF \) exerted by this element on the particle of mass \( m \) at the center is:
\[ dF = \frac{G \times m \times dm}{R^2} = \frac{Gm \times \frac{M}{\pi} d\theta}{R^2} = \frac{GmM}{\pi R^2} d\theta \]
Resolve \( dF \) into Components:
Each element of the arc exerts a gravitational force toward itself. The horizontal components (along the x-axis) will cancel due to symmetry, and only the vertical components (along the y-axis) will add up.
The vertical component of \( dF \) is:
\[ dF_y = dF \cos \theta = \frac{GmM}{\pi R^2} \cos \theta \, d\theta \]
Integrate \( dF_y \) Over the Semicircle:
To find the total gravitational force \( F_y \) on the particle, integrate \( dF_y \) from \( -\frac{\pi}{2} \) to \( \frac{\pi}{2} \):
\[ F_y = \int_{-\pi/2}^{\pi/2} \frac{GmM}{\pi R^2} \cos \theta \, d\theta \]
\[ F_y = \frac{GmM}{\pi R^2} \int_{-\pi/2}^{\pi/2} \cos \theta \, d\theta \]
\[ F_y = \frac{GmM}{\pi R^2} \left[ \sin \theta \right]_{-\pi/2}^{\pi/2} \]
\[ F_y = \frac{GmM}{\pi R^2} \left( \sin \frac{\pi}{2} - \sin \left( -\frac{\pi}{2} \right) \right) \]
\[ F_y = \frac{GmM}{\pi R^2} (1 + 1) = \frac{2GmM}{\pi R^2} \]
Substitute \( R = \frac{L}{\pi} \):
Since \( L = \pi R \), we have \( R = \frac{L}{\pi} \).
Substitute this into the expression for \( F_y \):
\[ F_y = \frac{2GmM}{\pi \left( \frac{L}{\pi} \right)^2} = \frac{2GmM\pi}{L^2} \]
Conclusion:
The gravitational force on the particle by the wire is:
\[ F = \frac{2GmM\pi}{L^2} \]
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,

What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)