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University Physics I - Classical Mechanics, 2019

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154 CHAPTER 7. IMPULSE, WORK AND POWER<br />

7.7.2 Work, energy and the choice of system: dissipative case<br />

Consider again the situation shown in Figure 7.5. Letm 1 =1kg,m 2 =2kg,andμ k =0.3. Use the<br />

solutions provided in Section 6.3 to calculate the work done by all the forces, and the changes in all<br />

energies, when the system undergoes a displacement of 0.5 m, and represent the changes graphically<br />

using bar diagrams like the ones in Figure 7.3 (for system A and B separately)<br />

Solution<br />

From Eq. (6.32), we have<br />

a = m 2 − μ k m 1<br />

m 1 + m 2<br />

g =5.55 m s 2<br />

F t = m 1m 2 (1 + μ k )<br />

g =8.49 N (7.34)<br />

m 1 + m 2<br />

We can use the acceleration to calculate the change in kinetic energy, since we have Eq. (2.10) for<br />

motion with constant acceleration:<br />

(<br />

vf 2 − v2 i =2aΔx =2× 5.55 m )<br />

s 2 × 0.5m =5.55 m2<br />

s 2 (7.35)<br />

so the change in kinetic energy of the two blocks is<br />

ΔK 1 = 1 2 m 1<br />

(<br />

v<br />

2<br />

f − v 2 i<br />

)<br />

=2.78 J<br />

ΔK 2 = 1 2 m 2<br />

(<br />

v<br />

2<br />

f − v 2 i<br />

)<br />

=5.55 J (7.36)<br />

We can also use the tension to calculate the work done by the external force on each system:<br />

W ext,A = Fr,1Δx t =(8.49 N) × (0.5m)=4.25 J<br />

W ext,B = Fr,2Δy t =(8.49 N) × (−0.5m)=−4.25 J (7.37)<br />

Lastly, we need the change in the gravitational potential energy of system B:<br />

ΔUB G = m 2 gΔy =(2kg)×<br />

(9.8 m )<br />

s 2 × (−0.5m)=−9.8 J (7.38)<br />

and the increase in dissipated energy in system A, which we can get from Eq. (7.28):<br />

ΔE diss = −Fs,1Δx k = μ k Fs,1Δx n = μ k m 1 gΔx =0.3 × (1 kg) ×<br />

(9.8 m )<br />

s 2 × (0.5m)=1.47 J (7.39)<br />

We can now put all this together to show that Eq. (7.20) indeed holds:<br />

W ext,A =ΔE A =ΔK 1 +ΔE diss =2.78 J + 1.47 J = 4.25 J<br />

W ext,B =ΔE B =ΔK 2 +ΔUB G =5.55 J − 9.8J =−4.25 J (7.40)

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