The time dilation formula is given by:
\[ \tau' = \frac{\tau}{\sqrt{1 - \frac{v^2}{c^2}}} \]
Substituting \( v = 0.998c \) and \( \tau = 632 \) ns:
\[ \tau' = \frac{632ns}{\sqrt{1 - \frac{(0.998c)^2}{c^2}}} \]
\[ \tau' = \frac{632ns}{\sqrt{1 - 0.996004}} \]
\[ \tau' = \frac{632ns}{\sqrt{0.003996}} \]
\[ \tau' = \frac{632ns}{0.06333} \]
\[ \tau' \approx 9984ns \]
The distance traveled by the particle is given by:
\[ d = v \times \tau' \]
Substituting \( v = 0.998c \) and \( \tau' = 9984 \) ns:
\[ d = 0.998 \times 3 \times 10^8 \text{ m/s} \times 9984 \times 10^{-9} \text{ s} \]
\[ d = 0.998 \times 3 \times 10^8 \times 9984 \times 10^{-9} \]
\[ d \approx 2992.1 \text{ m} \]
The distance between points P and Q is approximately 2992 m.
In order to achieve the static equilibrium of the see-saw about the fulcrum \( P \), shown in the figure, the weight of Box B should be _________ kg, if the weight of Box A is 50 kg.
A particle of mass 1kg, initially at rest, starts sliding down from the top of a frictionless inclined plane of angle \(\frac{𝜋}{6}\)\(\frac{\pi}{6}\) (as schematically shown in the figure). The magnitude of the torque on the particle about the point O after a time 2seconds is ______N-m. (Rounded off to nearest integer)
(Take g = 10m/s2)
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.)