Question #56569

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2016-02-18T00:00:52-0500

Answer on Question #56569 - Physics - Mechanics - Relativity

5-10 A hollow straight tube of length 2/ and mass m can turn freely about its centre on a smooth horizontal table. Another smooth uniform rod of same length and mass is fitted into the tube so that their centres coincide. The system is set in motion with an initial angular velocity ω0\omega_0. Find the angular velocity of the tube at the instant when the rod slips out of the tube:

(A) ω04\frac{\omega_0}{4}

(B) ω05\frac{\omega_0}{5}

(C) ω07\frac{\omega_0}{7}

(D) ω02\frac{\omega_0}{2}

5-11 The moment of inertia of the pulley system as shown in the figure-5.99 is 4kgm24\,\mathrm{kgm}^2. The radii of bigger and smaller pulleys 2 m and 1 m respectively. The angular acceleration of the pulley system is:

(A) 2.1rad/s22.1\,\mathrm{rad/s^2}

(B) 4.2rad/s24.2\,\mathrm{rad/s^2}

(C) 1.2rad/s21.2\,\mathrm{rad/s^2}

(D) 0.6rad/s20.6\,\mathrm{rad/s^2}


Figure 5.99

5.10 Solution.

Let's define the moment of inertia at the initial and final moments. At the beginning:


J1=Jt+Jr=m4l212+m4l212=2ml23J_1 = J_t + J_r = \frac{m4l^2}{12} + \frac{m4l^2}{12} = \frac{2ml^2}{3}


At the final moment:


J2=Jt+Jr=m4l23+m4l23=8ml23J_2 = J_t + J_r = \frac{m4l^2}{3} + \frac{m4l^2}{3} = \frac{8ml^2}{3}


As the energy of the system is constant:


J1ω022=J2ω22\frac{J_1\omega_0^2}{2} = \frac{J_2\omega^2}{2}2ml23ω02=8ml23ω2\frac{2ml^2}{3}\omega_0^2 = \frac{8ml^2}{3}\omega^2ω=ω02\omega = \frac{\omega_0}{2}


Answer: D ω=ω02\omega = \frac{\omega_0}{2}

5.11 Solution.

{m1gT1=m1a1=m1r1εm2g+T2=m2a2=m2r2εT1r1T2r2=Jε{T1=m1gm1r1εT2=m2g+m2r2εT1r1T2r2=Jε(m1gm1r1ε)r1(m2g+m2r2ε)r2=Jεε=g(m1r1m2r2)J+m1r12+m2r22=9.8(5241)4+522+412=2.1\begin{array}{l} \left\{ \begin{array}{c} m _ {1} g - T _ {1} = m _ {1} a _ {1} = m _ {1} r _ {1} \varepsilon \\ - m _ {2} g + T _ {2} = m _ {2} a _ {2} = m _ {2} r _ {2} \varepsilon \\ T _ {1} r _ {1} - T _ {2} r _ {2} = J \varepsilon \end{array} \right. \\ \left\{ \begin{array}{l} T _ {1} = m _ {1} g - m _ {1} r _ {1} \varepsilon \\ T _ {2} = m _ {2} g + m _ {2} r _ {2} \varepsilon \\ T _ {1} r _ {1} - T _ {2} r _ {2} = J \varepsilon \end{array} \right. \\ (m _ {1} g - m _ {1} r _ {1} \varepsilon) r _ {1} - (m _ {2} g + m _ {2} r _ {2} \varepsilon) r _ {2} = J \varepsilon \\ \varepsilon = \frac {g (m _ {1} r _ {1} - m _ {2} r _ {2})}{J + m _ {1} r _ {1} ^ {2} + m _ {2} r _ {2} ^ {2}} = \frac {9 . 8 (5 * 2 - 4 * 1)}{4 + 5 * 2 ^ {2} + 4 * 1 ^ {2}} = 2. 1 \\ \end{array}

Answer: A 2.1

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