In the Bohr model, the centripetal force required for an electron to revolve in a circular orbit is provided by the electrostatic force of attraction between the electron and the nucleus. The centripetal force is given by: \[ F_{\text{centripetal}} = \frac{m v^2}{r} \] where \( m \) is the mass of the electron, \( v \) is its speed, and \( r \) is the radius of the orbit. The electrostatic force is given by Coulomb's law: \[ F_{\text{electrostatic}} = \frac{k e^2}{r^2} \] where \( e \) is the charge of the electron, and \( k \) is Coulomb's constant. Equating these two forces: \[ \frac{m v^2}{r} = \frac{k e^2}{r^2} \] From this, we can solve for \( v \) and \( r \) in terms of \( n \), the principal quantum number. Using Bohr's quantization condition: \[ m v r = n h \quad \Rightarrow \quad v = \frac{n h}{2 \pi m r} \] Substitute \( v \) into the force equation: \[ \frac{m \left( \frac{n h}{2 \pi m r} \right)^2}{r} = \frac{k e^2}{r^2} \] Solving for \( r \) gives: \[ r \propto n^2 \] Now, the time period \( T \) is the time taken for one complete revolution, and it is related to the velocity \( v \) and the radius \( r \) by: \[ T = \frac{2 \pi r}{v} \] Substituting \( v \) and \( r \) into this equation: \[ T \propto n^3 \] Thus, the time period of revolution of the electron in the \( n \)-th orbit is proportional to \( n^3 \).
A racing track is built around an elliptical ground whose equation is given by \[ 9x^2 + 16y^2 = 144 \] The width of the track is \(3\) m as shown. Based on the given information answer the following: 
(i) Express \(y\) as a function of \(x\) from the given equation of ellipse.
(ii) Integrate the function obtained in (i) with respect to \(x\).
(iii)(a) Find the area of the region enclosed within the elliptical ground excluding the track using integration.
OR
(iii)(b) Write the coordinates of the points \(P\) and \(Q\) where the outer edge of the track cuts \(x\)-axis and \(y\)-axis in first quadrant and find the area of triangle formed by points \(P,O,Q\).