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)
The component of gravitational acceleration along the incline is:
a = g sinθ = 9.8 sin(π/6)
Substituting sin(π/6) = 0.5:
a = 9.8 × 0.5 = 4.9 m/s²
Using the equation of motion:
s = ut + (1/2) a t²
Since u = 0, substitute a = 4.9 m/s² and t = 2 seconds:
s = 0 + (1/2) × 4.9 × (2)²
s = (1/2) × 4.9 × 4 = 9.8 m
The perpendicular distance from point O to the line of action of the gravitational force is:
r⊥ = s cosθ
Substituting s = 9.8 m and cos(π/6) = √3/2 ≈ 0.866:
r⊥ = 9.8 × (√3/2) ≈ 9.8 × 0.866 = 8.48 m
The gravitational force acting on the particle is:
F = mg = 1 × 9.8 = 9.8 N
The torque about point O is:
τ = r⊥ × F
Substituting r⊥ = 8.48 m and F = 9.8 N:
τ = 8.48 × 9.8 ≈ 83.1 N·m
The torque about point O is 83.1 N·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.
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.)