Consider an annular region in free space containing a uniform magnetic field in the \(z\)-direction, schematically represented by the shaded region in the figure. A particle having charge \(Q\) and mass \(M\) starts from point \(P(a, 0, 0)\) in the \(+x\)-direction with constant speed \(v\). If the radii of inner and outer circles are \(a\) and \(b\), respectively, the minimum magnetic field required so that the particle returns to the inner circle is: 
Step 1: Concept of circular motion in a magnetic field.
The radius of circular motion of a charged particle moving in a magnetic field \(B\) is \[ r = \frac{Mv}{QB} \]
Step 2: Condition for returning to the inner circle.
The particle must just touch the outer boundary before returning to the starting point, forming a semicircular trajectory between \(a\) and \(b\). At the maximum deflection, the center of circular motion lies along the \(x\)-axis. The geometry gives: \[ (b - a) = 2r \]
Step 3: Substitute radius.
\[ r = \frac{b^2 - a^2}{2b} = \frac{Mv}{QB} \Rightarrow B = \frac{Mv}{Q} \left( \frac{b^2 - a^2}{2b} \right)^{-1} \]
Step 4: Conclusion.
The minimum magnetic field required is \(\dfrac{Mv}{Q} \left( \dfrac{b^2 - a^2}{2b} \right)^{-1}\).

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/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)