When the stone is released, it moves down executing a circular motion. At any instant, the stone accelerates towards (w.r.t.) the center of its revolution 0, that is, centripetal acceleration a, and simultaneously accelerates down with an acceleration, that is, gravitational acceleration g; →ar=ω2r. Resolving →ar, and along the tangent, we obtain the tangential acceleration of the stone as at=gcosθ
Angular acceleration, α=atr
⇒α=gcosθl(sincer=l)
Putting α=ωdωdθ, we obtain ωdωdθ=gcosθr
⇒ωdω=(g/l)cosθdθ.
Integrating both the sides, we obtain
∫ω0ωdθ=gl∫θ0cosθdθ
⇒ ω22=glsinθorω=√2glsinθ
Putting l=1m and θ=30o, we obtain
ω=√2(10)sin30o(1)=√10⇒ω≅3.1rads−1