Showing posts with label collisions. Show all posts
Showing posts with label collisions. Show all posts

Wednesday, March 20, 2019

Chapter 6.25 - Two-Dimensional Collision - Examples

In the previous section, we discussed two-dimensional collision. We also saw a solved example. In this section, we will see a few more solved examples.

Solved example 6.40
Two objects 'A' and 'B' have masses 5 kg and 2.5 kg respectively. 'A' moves with a velocity of 4.5 ms-1 towards 'B' which is initially at rest. After the collision, object 'A' moves in a direction which makes 30o with it's original direction. Object 'B' moves in a direction which makes -30o with the original direction of 'A'. Find the final velocities of 'A' and 'B'. Is the collision elastic or inelastic?
Solution:
1. Fig.6.80 below shows the collision:
Fig.6.80
2. The table is shown below:
• All the cells in columns 1 to 5 can be filled up (using the given data) except (A,3) and (B,3)
    ♦ (A,3) contains the unknown $\mathbf\small{|\vec{v_{Af}}|}$
    ♦ (B,3) contains the unknown $\mathbf\small{|\vec{v_{Bf}}|}$
• So there are two unknowns. We need to form two equations only
• Also note that, there are two 'question marks' in the fig.6.80 above
3. Considering momenta in the x-direction, we have:
• Sum in column 6 = Sum in column 8
$\mathbf\small{\Rightarrow [22.5+0]=[5|\vec{v_{Af(x)}}|+2.5|\vec{v_{Bf(x)}}|]}$
$\mathbf\small{\Rightarrow [22.5]=[5|\vec{v_{Af}}| \cos \theta_{Af}+2.5|\vec{v_{Bf}}| \cos \theta_{Bf}]}$
$\mathbf\small{\Rightarrow [22.5]=[5|\vec{v_{Af}}| \cos 30+|\vec{v_{Bf}}| \cos (-30)]}$
Dividing both sides by 2.5, we get:
$\mathbf\small{[9]=[2|\vec{v_{Af}}| \cos 30+|\vec{v_{Bf}}| \cos (-30)]}$
$\mathbf\small{\Rightarrow [9]=[1.732|\vec{v_{Af}}|+0.866|\vec{v_{Bf}}| ]}$
4. Considering momenta in the y-direction, we have:
• Sum in column 7 = Sum in column 9
$\mathbf\small{\Rightarrow [0]=[5|\vec{v_{Af(y)}}|+2.5|\vec{v_{Bf(y)}}|]}$
$\mathbf\small{\Rightarrow [0]=[5|\vec{v_{Af}}| \sin 30+|\vec{v_{Bf}}| \sin (-30)]}$
Deviding both sides by 2.5, we get:
$\mathbf\small{\Rightarrow [0]=[2|\vec{v_{Af}}| \sin 30+|\vec{v_{Bf}}| \sin (-30)]]}$
$\mathbf\small{\Rightarrow [0]=[2|\vec{v_{Af}}| 0.5+|\vec{v_{Bf}}| (-0.5)]}$
$\mathbf\small{\Rightarrow [0]=[|\vec{v_{Af}}|-.5|\vec{v_{Bf}}|]}$
5. So we have two equations:
(i) From (3) we have: $\mathbf\small{1.732|\vec{v_{Af}}|+0.866|\vec{v_{Bf}}|=9}$
(ii) From (4) we have: $\mathbf\small{|\vec{v_{Af}}|-0.5|\vec{v_{Bf}}|=0}$
• To solve the equations, the following steps can be used:
    ♦ Multiply (i) by '0.5'
    ♦ Multiply (ii) by 0.866
    ♦ Add the results 
• We get:
vAf = 2.598 ms-1
vBf = 5.196 ms-1
6. Let us check whether it is an elastic collision or not:
• Applying law of conservation of kinetic energy, we have:
$\mathbf\small{\frac{1}{2}m_A|\vec{v}_{Ai}|^2+\frac{1}{2}m_B|\vec{v}_{Bi}|^2=\frac{1}{2}m_A|\vec{v}_{Af}|^2+\frac{1}{2}m_B|\vec{v}_{Bf}|^2}$
• Let us first calculate the LHS:
$\mathbf\small{\frac{1}{2}m_A|\vec{v}_{Ai}|^2+\frac{1}{2}m_B|\vec{v}_{Bi}|^2=\frac{1}{2}\times 5 \times 4.5^2+\frac{1}{2}\times 2.5 \times0^2=50.625\; \text{J}}$
• Next we calculate the RHS:
$\mathbf\small{\frac{1}{2}m_A|\vec{v}_{Af}|^2+\frac{1}{2}m_B|\vec{v}_{Bf}|^2=\frac{1}{2}\times 5 \times 2.598^2+\frac{1}{2}\times 2.5 \times 5.196^2=50.628\; \text{J}}$
■ We get: LHS = RHS
So kinetic energy is conserved and so it is an elastic collision


• We saw solved example 6.39 in the previous section
• We saw solved example 6.40 above in the present section
• Both of those examples involves only two unknowns
• Such problems can be easily solved using two equations that we obtain from the law of conservation of momentum
■ The calculations become even more easier if the two objects stick together after collision
• Let us see such a problem: 

Solved example 6.41
Car A has a mass of 1800 kg. It moves towards the North with a velocity of 15 ms-1. Car B has a mass of 1500 kg. It moves in a South-East direction, making an angle of 30o with the East-West direction. It has a velocity of 10 ms-1. After collision, they stick together. Find the velocity (magnitude and direction) of the combined mass after the collision
Solution:
1. Fig.6.81 below shows the collision:
Fig.6.81
• East-West direction can be taken as the x-axis
2. The table is shown below:
• The first 5 columns can be filled up using the given data
• However, be careful while filling column 4
    ♦ Velocity of 'A' makes an angle of 90o with the East-West direction (the x-axis)
    ♦ So we have '90' in the cell (A,4)
    ♦ Velocity of 'B' makes an angle of 30with the x-axis
    ♦ So we have '30' in the cell (B,4)
    ♦ sin 30 is not negative
    ♦ But we must put a negative value in the cell (B,7)
    ♦ This is because, that velocity is towards the negative side of the y-axis
• After collision, both cars move together. So they will be having the same velocity
    ♦ Thus we have: $\mathbf\small{|\vec{v}_{Af}|=|\vec{v}_{Bf}|}$
    ♦ We can put: $\mathbf\small{|\vec{v}_{Af}|=|\vec{v}_{Bf}|=|\vec{v}_{f}|}$ 
    ♦ We see this in the cells (A,3) and (B,3)
• After collision, since they move together with the same velocity, they will be making the same angle with the x axis
    ♦ Thus we have: $\mathbf\small{\theta_{Af}=\theta_{Bf}}$
    ♦ We can put: $\mathbf\small{\theta_{Af}=\theta_{Bf}=\theta_{f}}$ 
    ♦ We see this in the cells (A,5) and (B,5)
• After filling the first five columns, we see that there are two unknowns. So we need to form two equations only
• Also note that, there are two 'question marks' in the fig.6.81 above
3. Considering momenta in the x-direction, we have:
• Sum in column 6 = Sum in column 8
$\mathbf\small{\Rightarrow [0+12990]=[1800|\vec{v_{f(x)}}|+1500|\vec{v_{f(x)}}|]}$
$\mathbf\small{\Rightarrow [12990]=[(1800+1500)|\vec{v_{f(x)}}|]}$
$\mathbf\small{\Rightarrow [12990]=[3300|\vec{v_{f(x)}}|]}$
$\mathbf\small{\Rightarrow |\vec{v}_{f(x)}|=\frac{12990}{3300}=3.936\;\text{ms}^{-1}}$
4. Considering momenta in the y-direction, we have:
• Sum in column 7 = Sum in column 9
$\mathbf\small{\Rightarrow [27000-7500]=[1800|\vec{v_{f(y)}}|+1500|\vec{v_{f(y)}}|]}$
$\mathbf\small{\Rightarrow [19500]=[(1800+1500)|\vec{v_{f(y)}}|]}$
$\mathbf\small{\Rightarrow [19500]=[3300|\vec{v_{f(y)}}|]}$
$\mathbf\small{\Rightarrow |\vec{v}_{f(y)}|=\frac{19500}{3300}=5.91\;\text{ms}^{-1}}$
5. Now we can find the magnitude of the resultant
$\mathbf\small{|\vec{v}_{f}|=\sqrt{|\vec{v}_{fx}|^2+|\vec{v}_{fy}|^2}=\sqrt{3.936^2+5.91^2}=7.1\;\text{ms}^{-1}}$
6. Direction of this resultant is given by: $\mathbf\small{\tan \theta_f=\frac{|\vec{v}_{fy}|}{|\vec{v}_{fx}|}=\frac{5.91}{3.936}=1.501}$
$\mathbf\small{\Rightarrow \theta_f=\tan^{-1}1.501=56.33^\text{o}}$
7. Thus we can write:
■ The final velocity shown in fig.6.81 has a magnitude of 7.1 ms-1 and a direction which makes 56.33o with the x-axis

• Next we will see problems with 3 unknowns.  Such problems involve somewhat lengthy calculations
■ But those calculations will be greatly simplified if the two colliding objects have the same mass
• The Solved examples 6.42 and 6.43 given below will demonstrate this idea

Solved example 6.42
Prove that an elastic collision between equal masses in 2 dimensions always results in the objects bouncing off each other at a 90o degrees angle (assume one of the objects to be initially stationary). 
Solution:
1. Fig.6.82 below shows a 2-dimensional collision between two spheres 'A' and 'B'
Fig.6.82
• Both the spheres have the same mass. So we can write: mA = mB = m
• We have to prove that $\mathbf\small{(\theta_{Af}+\theta_{Bf})=90^\text{o}}$
2. The table is shown below:
3. Considering momenta in the x-direction, we have:
• Sum in column 6 = Sum in column 8
$\mathbf\small{\Rightarrow \sum |\vec{p}_{i(x)}|=\sum |\vec{p}_{f(x)}|}$
$\mathbf\small{\Rightarrow [m|\vec{v}_{Ai(x)}|+0]=[m|\vec{v}_{Af(x)}|+m|\vec{v}_{Bf(x)}|]}$
$\mathbf\small{\Rightarrow [|\vec{v}_{Ai(x)}|]=[|\vec{v}_{Af(x)}|+|\vec{v}_{Bf(x)}|]}$
$\mathbf\small{\Rightarrow [|\vec{v}_{Ai}|\cos \theta_{Ai}]=[|\vec{v}_{Af}|\cos \theta_{Af}+|\vec{v}_{Bf}|\cos \theta_{Bf}]}$
4. Considering momenta in the y-direction, we have:
• Sum in column 7 = Sum in column 9
$\mathbf\small{\Rightarrow \sum |\vec{p}_{i(y)}|=\sum |\vec{p}_{f(y)}|}$
$\mathbf\small{\Rightarrow [0+0]=[m|\vec{v}_{Af(y)}|+m|\vec{v}_{Bf(y)}|]}$
$\mathbf\small{\Rightarrow [0]=[|\vec{v}_{Af(y)}|+|\vec{v}_{Bf(y)}|]}$
$\mathbf\small{\Rightarrow [0]=[|\vec{v}_{Af}|\sin \theta_{Af}+|\vec{v}_{Bf}|\sin \theta_{Bf}]}$
5. So we have two equations:
(i) From (3) we have: $\mathbf\small{|\vec{v}_{Af}|\cos \theta_{Af}+|\vec{v}_{Bf}|\cos \theta_{Bf}=|\vec{v}_{Ai}|\cos \theta_{Ai}}$
(ii) From (4) we have: $\mathbf\small{|\vec{v}_{Af}|\sin \theta_{Af}+|\vec{v}_{Bf}|\sin \theta_{Bf}=0}$
6. But we have three unknowns. So we must have three equations
• For the third equation, we apply conservation of kinetic energy
• Total initial kinetic energy = Total final kinetic energy
• Since the masses are equal, we have: $\mathbf\small{|\vec{v_{Ai}}|^2+|\vec{v_{Bi}}|^2=|\vec{v_{Af}}|^2+|\vec{v_{Bf}}|^2}$
$\mathbf\small{\Rightarrow |\vec{v_{Ai}}|^2=|\vec{v_{Af}}|^2+|\vec{v_{Bf}}|^2}$
[∵ vBi = 0]
7. Let us write the three equations together:
(i) From (3) we have: $\mathbf\small{|\vec{v}_{Af}|\cos \theta_{Af}+|\vec{v}_{Bf}|\cos \theta_{Bf}=|\vec{v}_{Ai}|\cos \theta_{Ai}}$
(ii) From (4) we have: $\mathbf\small{|\vec{v}_{Af}|\sin \theta_{Af}+|\vec{v}_{Bf}|\sin \theta_{Bf}=0}$
(iii) From (6) we have: $\mathbf\small{|\vec{v_{Af}}|^2+|\vec{v_{Bf}}|^2=|\vec{v_{Ai}}|^2}$
8. Let us write them in a 'easy to manipulate' form:
(i) $\mathbf\small{A\;\cos \theta_{A}+B\cos \theta_{B}=k_1}$
(ii) $\mathbf\small{A\;\sin \theta_{A}+B\sin \theta_{B}=0}$
(iii) $\mathbf\small{A^2+B^2=(k_1)^2}$ 
Where:
• $\mathbf\small{A=|\vec{v_{Af}}|}$. A quantity that we have to find
• $\mathbf\small{B=|\vec{v_{Bf}}|}$. A quantity that we have to find
• $\mathbf\small{\theta_{B}=\theta_{B_f}}$. A quantity that we have to find
• $\mathbf\small{\theta_{A}=\theta_{Af}}$. A constant, which can be calculated from the given data
• $\mathbf\small{k_1=|\vec{v}_{Ai}|\cos \theta_{Ai}}$ 
    ♦ But $\mathbf\small{\theta_{Ai}=0}$. So $\mathbf\small{\cos \theta_{Ai}}$ =1
    ♦ Thus we get: $\mathbf\small{k_1=|\vec{v}_{Ai}|\cos \theta_{Ai}=|\vec{v}_{Ai}|}$ 
    ♦ So k1 is a constant, which can be calculated from the given data
■ Now we can write the steps for obtaining the 3 unknowns:
(iv) Squaring (i), we get:
$\mathbf\small{A^2\,\cos^2\theta_A+B^2\,\cos^2\theta_B+2AB\,\cos\theta_A\,\cos\theta_B=(k_1)^2}$
(v) Squaring (ii), we get:
$\mathbf\small{A^2\,\sin^2\theta_A+B^2\,\sin^2\theta_B+2AB\,\sin\theta_A\,\sin\theta_B=0}$
(vi) Adding (iv) and (v), we get:
$\mathbf\small{(A^2\,\cos^2\theta_A+A^2\,\sin^2\theta_A)+(A^2\,\sin^2\theta_B+B^2\,\sin^2\theta_B)+(2AB\,\cos\theta_A\,\cos\theta_B+2AB\,\sin\theta_A\,\sin\theta_B)=(k_1)^2+0}$
$\mathbf\small{\Rightarrow A^2(\cos^2\theta_A+\sin^2\theta_A)+B^2(\sin^2\theta_B+\sin^2\theta_B)+(2AB\,\cos\theta_A\,\cos\theta_B+2AB\,\sin\theta_A\,\sin\theta_B)=(k_1)^2+0}$
$\mathbf\small{\Rightarrow A^2+B^2+(2AB\,\cos\theta_A\,\cos\theta_B+2AB\,\sin\theta_A\,\sin\theta_B)=(k_1)^2}$
(vii) But from (iii), we have: $\mathbf\small{A^2+B^2=(k_1)^2}$
• Substituting this in (v), we get:
$\mathbf\small{(k_1)^2+(2AB\,\cos\theta_A\,\cos\theta_B+2AB\,\sin\theta_A\,\sin\theta_B)=(k_1)^2}$
$\mathbf\small{\Rightarrow 2AB\,\cos\theta_A\,\cos\theta_B+2AB\,\sin\theta_A\,\sin\theta_B=0}$
$\mathbf\small{\Rightarrow 2AB(\cos\theta_A\,\cos\theta_B+\,\sin\theta_A\,\sin\theta_B)=0}$
(viii) Using the identity $\mathbf\small{\cos(\theta_1-\theta_2)=\cos\theta_1\,\cos\theta_2+\sin\theta_1\,\sin\theta_2}$, we get:
$\mathbf\small{2AB\,\cos(\theta_A-\theta_B)=0}$
(ix) Putting back the values, we get:
• $\mathbf\small{2|\vec{v}_{Af}|\,|\vec{v}_{Bf}|\,\cos(\theta_{Af}-\theta_{Bf})=0}$
• $\mathbf\small{|\vec{v}_{Af}|}$ can be zero only if all the three conditions given below are satisfied:
    ♦ It is a one-dimensional collision (Details here)
    ♦ The two masses are equal
    ♦ Object B is stationary before collision
• In our present case, the second and third conditions are satisfied
• But it is not a one-dimensional collision. What we have is a two-dimensional collision
• So $\mathbf\small{|\vec{v}_{Af}|}$ cannot be zero  
• $\mathbf\small{|\vec{v}_{Bf}|}$ can be zero only if the mass of B is very large compared to mass of A. But in our present case, both masses are equal
• So $\mathbf\small{|\vec{v}_{Bf}|}$ cannot be zero
• Thus the only option is: $\mathbf\small{\cos(\theta_{Af}-\theta_{Bf})=0}$
• If $\mathbf\small{\cos(\theta_{Af}-\theta_{Bf})=0}$, then $\mathbf\small{(\theta_{Af}-\theta_{Bf})=90^\text{o}}$  
■ This relation $\mathbf\small{(\theta_{Af}-\theta_{Bf})=90^\text{o}}$ is our key
9. In fig.6.83(a) below, we see that, $\mathbf\small{(\theta_{Af}-\theta_{Bf})}$ is the 'angle between the two final vectors'
Proof that an elastic 2-dimensional collision between equal masses in 2 dimensions always results in the objects bouncing off each other at a 90 degrees angle when one of the objects to be initially stationary
Fig.6.83
• If $\mathbf\small{(\theta_{Af}-\theta_{Bf})}$ is to be 90, the 'after collision' fig. will be as in (b)
• Here also, $\mathbf\small{(\theta_{Af}-\theta_{Bf})}$ is the 'angle between the two final vectors'
10. Another possibility is shown in fig.c
• After collision, the object 'B' is below the x-axis. It's final velocity vector makes an angle of $\mathbf\small{-\theta_{Bf}}$ with the x-axis  
• So $\mathbf\small{(\theta_{Af}-\theta_{Bf})}$ becomes: $\mathbf\small{[\theta_{Af}-(-\theta_{Bf})]=[theta_{Af}+\theta_{Bf}]}$ 
• Here also, $\mathbf\small{(\theta_{Af}-\theta_{Bf})}$ is the 'angle between the two final vectors'
■ Thus we can write: After a 2-dimensional collision, the two objects will scatter at 90o to each other when the following two conditions are satisfied:
    ♦ The two objects have the same mass
    ♦ One of the objects is stationary before collision

Solved example 6.43
Two identical objects A and B collide on a smooth horizontal surface. B was originally at rest. A has an initial velocity of 6 ms-1. After collision it scatters at an angle of 30o to the original direction.
(a) What is the magnitude of the velocity of 'A' after the collision ?
(b) What is the magnitude and direction of the velocity of 'B' after the collision ?
Solution:
1. Fig.6.84 below shows the collision:
Fig.6.84
• In the fig.6.84, Î¸Bf is shown below the initial direction. But the initial direction is considered as the x-axis
• So Î¸Bf is below the x-axis. That means, Î¸Bf is negative
• But we need not write '(-θBf)' and do the calculations. We can do the calculations using '(+θBf)'
• If in the final results, we get a negative value for 'θBf', the positions in fig.6.83 will be justified
2. The table is shown below:

• All the cells in columns 1 to 5 can be filled up (using the given data) except (A,3), (B,3) and (B,5)
    ♦ (A,3) contains the unknown $\mathbf\small{|\vec{v_{Af}}|}$
    ♦ (B,3) contains the unknown $\mathbf\small{|\vec{v_{Bf}}|}$
    ♦ (B,5) contains the unknown $\mathbf\small{\theta_{Bf}}$
• So there are three unknowns. We need to form three equations
• Also note that, there are 3 'question marks' in the fig.6.84 above
• Most of the cells in columns 6 to 9 need to be calculated except (B,6), (A,7) and (B,7)
• Those 3 cells have zero values because:
    ♦ B has zero initial x-velocity
    ♦ A has zero initial y-velocity
    ♦ B has zero initial y-velocity
3. Considering momenta in the x-direction, we have:
• Sum in column 6 = Sum in column 8
$\mathbf\small{\Rightarrow [6m+0]=[m|\vec{v_{Af(x)}}|+m|\vec{v_{Bf(x)}}|]}$
$\mathbf\small{\Rightarrow [6]=[|\vec{v_{Af}}| \cos \theta_{Af}+|\vec{v_{Bf}}| \cos \theta_{Bf}]}$
$\mathbf\small{\Rightarrow [6]=[|\vec{v_{Af}}| \cos 30+|\vec{v_{Bf}}| \cos \theta_{Bf}]}$
$\mathbf\small{\Rightarrow [6]=[0.866|\vec{v_{Af}}|+|\vec{v_{Bf}}| \cos \theta_{Bf}]}$
4. Considering momenta in the y-direction, we have:
• Sum in column 7 = Sum in column 9
$\mathbf\small{\Rightarrow [0]=[m|\vec{v_{Af(y)}}|+m|\vec{v_{Bf(y)}}|]}$
$\mathbf\small{\Rightarrow [0]=[|\vec{v_{Af}}| \sin \theta_{Af}+|\vec{v_{Bf}}| \sin \theta_{Bf}]}$
$\mathbf\small{\Rightarrow [0]=[|\vec{v_{Af}}| \sin 30+|\vec{v_{Bf}}| \sin \theta_{Bf}]}$
$\mathbf\small{\Rightarrow [0]=[0.5|\vec{v_{Af}}|+|\vec{v_{Bf}}| \sin \theta_{Bf}]}$
5. So we have two equations:
(i) From (3) we have: $\mathbf\small{0.866|\vec{v_{Af}}|+|\vec{v_{Bf}}| \cos \theta_{Bf}=6}$
(ii) From (4) we have: $\mathbf\small{0.5|\vec{v_{Af}}|+|\vec{v_{Bf}}| \sin \theta_{Bf}=0}$
6. But we have three unknowns. So we must have three equations
• For the third equation, we apply conservation of kinetic energy
Total initial kinetic energy = Total final kinetic energy
• Since the masses are equal, we have: $\mathbf\small{|\vec{v_{Ai}}|^2+|\vec{v_{Bi}}|^2=|\vec{v_{Af}}|^2+|\vec{v_{Bf}}|^2}$
$\mathbf\small{\Rightarrow |\vec{v_{Ai}}|^2+0=|\vec{v_{Af}}|^2+|\vec{v_{Bf}}|^2}$
$\mathbf\small{\Rightarrow 6^2=|\vec{v_{Af}}|^2+|\vec{v_{Bf}}|^2}$
$\mathbf\small{\Rightarrow |\vec{v_{Af}}|^2+|\vec{v_{Bf}}|^2=36}$
7. Let us write the three equations together:
(i) From (3) we have: $\mathbf\small{0.866|\vec{v_{Af}}|+|\vec{v_{Bf}}| \cos \theta_{Bf}=6}$
(ii) From (4) we have: $\mathbf\small{0.5|\vec{v_{Af}}|+|\vec{v_{Bf}}| \sin \theta_{Bf}=0}$
(iii) From (6) we have: $\mathbf\small{|\vec{v_{Af}}|^2+|\vec{v_{Bf}}|^2=36}$
8. Now we apply the relation $\mathbf\small{\theta_{Af}-\theta_{Bf}=90^\text{o}}$
We get: $\mathbf\small{30-\theta_{Bf}=90}$
$\mathbf\small{\Rightarrow \theta_{Bf}=30-90=-60^\text{o}}$ 
• Note: We can apply this relation because, the following two conditions are satisfied:
    ♦ The two objects have the same mass
    ♦ One of the objects is stationary before collision
9. Substituting this value of $\mathbf\small{\theta_{Bf}}$ in (i), we get:
$\mathbf\small{0.866|\vec{v_{Af}}|+|\vec{v_{Bf}}| \cos (-60)=6}$
$\mathbf\small{\Rightarrow 0.866|\vec{v_{Af}}|+0.5|\vec{v_{Bf}}|=6}$
10. Substituting this value of $\mathbf\small{\theta_{Bf}}$ in (ii), we get:
$\mathbf\small{0.5|\vec{v_{Af}}|+|\vec{v_{Bf}}| \sin (-60)=0}$
$\mathbf\small{\Rightarrow 0.5|\vec{v_{Af}}|-0.866|\vec{v_{Bf}}|=0}$
11. Solving (9) and (10), we get:
$\mathbf\small{|\vec{v_{Af}}|}$ = 5.196 ms-1
$\mathbf\small{|\vec{v_{Bf}}|}$ = 3
• Note: For solving, the following steps can be used:
    ♦ Multiply (9) by 0.866
    ♦ Multiply (10) by 0.5
    ♦ Add the results
12. Check:
• Let us substitute the velocities in (iii). We have:
$\mathbf\small{|\vec{v_{Af}}|^2+|\vec{v_{Bf}}|^2=36}$
• The LHS will be: $\mathbf\small{5.196^2+3^2=(27+9)=36}$
• RHS = 36
• So the results obtained in (11) are correct

We have completed this discussion on work, energy and power. In the next chapter, we will discuss about rotational motion

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Monday, March 4, 2019

Chapter 6.22 - Completely Inelastic Collisions

In the previous section, we saw elastic collision. It was illustrated in the first row 'a' in fig.6.64 of the previous section. Now we take up the second row 'b'. For convenience, the fig.6.64 is shown again below:
Fig.6.64
1. Consider the row 'b', column '1' in fig.6.64 above.
• Two objects A and B of masses mA and mB move towards each other
• Their initial velocities are respectively vAi and vBi
    ♦ vAi is 'velocity of A (initial)'
    ♦ vBi is 'velocity of B (initial)'
2. Row 'b', column '2' shows the instant at which collision takes place
• We see that both the masses undergo deformation
    ♦ A is compressed due to the impact
    ♦ B is also compressed due to the impact
3. Assume that, both the masses are made of 'perfectly inelastic' materials
• So they do not even try to regain their original shapes after impact
• That means, whatever 'deformation caused' remains as such  
• Since they do not even try to recover, they do not get separated  
• After impact, they move together with velocity vf
    ♦ vf is 'velocity of (A+B) (final)'
• This is shown in row 'b', column '3'
■ This is called a completely inelastic collision or a perfectly inelastic collision
• A portion of the initial energy will be lost as heat, sound, vibrations etc.,
4. This situation is just like compressing and not releasing a spring
• The energy used up for compressing the spring will not be obtained back if the spring is not released
• So there is a reduction in total energy
5. That means, in a completely inelastic collision, 
Total energy before collision > Total energy after collision
6. The two masses are at the same level
• The levels do not change even after collision
• So they have the same gravitational potential energy before and after collision
• Thus, we need not consider the gravitational potential energy 
7. So the result in (5) becomes:
■ In an elastic collision, 
Total kinetic energy before collision > Total kinetic energy after collision
• That is:
$\mathbf\small{\frac{1}{2}m_A v_{Ai}^2+\frac{1}{2}m_B v_{Bi}^2>\frac{1}{2}(m_A+m_B) v_f^2}$
• So we have the '>' sign instead of the '=' sign
8. We can replace the '>' sign by the '=' sign by making a small modification
• The modification is: Bring in the 'lost energy' also
• If we add the 'lost energy' on the right side, the energies will balance. So we get:
$\mathbf\small{\frac{1}{2}m_A v_{Ai}^2+\frac{1}{2}m_B v_{Bi}^2=\frac{1}{2}(m_A+m_B) v_f^2+\text{Energy lost due to collision}}$
9. On many occasions, we will want to know the 'lost energy'
• For example, in a collision between two cars, the 'lost energy' is the energy which causes the damage to the cars and the passengers
• For finding the 'lost energy', we can use the equation in (8)
• All the quantities in that equation are known except 'vf' and the 'energy lost'
• To find two unknowns, we need two equations
10. To write the second equation, we use the law of conservation of momentum
• If there is no external force acting on the system, the law of conservation of momentum is valid
• So we have:
$\mathbf\small{m_A v_{Ai}+m_B v_{Bi}=(m_A+m_B) v_f}$ (Details here)
11. Equations in (8) and (10) can be used together, to solve problems in 'one-dimensional perfectly inelastic collisions'

Solved example 6.35
Two objects undergo a one-dimensional, completely inelastic collision (Fig.6.67 below)
Fig.6.67
(i) Calculate the velocity of (A+B) after collision
(ii) Also calculate the amount of energy lost
Given that: mA = 0.150 kg, mB = 70.0 kg, vAi = 35 ms-1, vBi = 0
Solution:
We are required to find vf
1. For a completely inelastic collision, we have:
$\mathbf\small{\frac{1}{2}m_A v_{Ai}^2+\frac{1}{2}m_B v_{Bi}^2=\frac{1}{2}(m_A+m_B) v_f^2+\text{Energy lost due to collision}}$
• Substituting the values, we get:
$\mathbf\small{\frac{1}{2}\times 0.150 \times 35^2+\frac{1}{2}\times 70 \times 0^2=\frac{1}{2}\times (70.15) v_f^2+\text{Energy lost}}$
$\mathbf\small{\Rightarrow 91.875+0=35.075\;v_f^2+\text{Energy lost}}$
$\mathbf\small{\Rightarrow 91.875=35.075\;v_f^2+\text{Energy lost}}$
2. If there is no external force acting on the system, the law of conservation of momentum is valid
So we have:
$\mathbf\small{m_A v_{Ai}+m_B v_{Bi}=(m_A+m_B) v_f}$
• Substituting the values, we get:
$\mathbf\small{0.150 \times 35+70 \times 0=70.15\;v_f}$
$\mathbf\small{\Rightarrow 5.25=70.15\;v_f}$
$\mathbf\small{\Rightarrow v_f=0.0748\;\text{ms}^{-1}}$
• This is the answer for part (i)
3. Substituting this value of vf in (1), we get:
$\mathbf\small{91.875=35.075\times 0.0748^2+\text{Energy lost}}$
⇒ Energy lost = 91.68 J
• This is the answer for part (ii)

Solved example 6.36
A bullet of mass 0.012 kg and horizontal speed 70 ms-1, strikes a block of wood of mass 0.4 kg and instantly comes to rest with respect to the block. The block is suspended from the ceiling by means of thin wires. Calculate the height to which the block rises. Also estimate the amount of heat produced in the block
Solution:
1. In the fig.6.68(a) below, the wooden block of mass 0.4 kg is suspended from point 'O'
Fig.6.68
• 'O' is a point in the ceiling
2. When the bullet strikes the block, it gets embedded in the block
• Due to the initial velocity of the bullet, the block (with the bullet embedded) will tend to move horizontally
3. But since the block is suspended from the ceiling, horizontal motion is not possible. Instead, it will move in a circular path
• This circular path UVWX is shown in green color. U is the initial position of the block    
• The block cannot complete the full circle because the ceiling is present
• If the length of the suspending wires is sufficiently large, the block will not reach even up to the ceiling
4. Let 'P' be the 'maximum possible point'. This is shown in fig.b 
• Draw a horizontal through P. This horizontal meets the vertical (through O) at Q
• Then UQ = 'h', the maximum possible height 
• We want to know this height 'h'
5. When the bullet strikes the block, a 'completely inelastic collision' takes place
• Because, after the collision, the bullet and the block move together
6. For a completely inelastic collision, we have:
$\mathbf\small{\frac{1}{2}m_A v_{Ai}^2+\frac{1}{2}m_B v_{Bi}^2=\frac{1}{2}(m_A+m_B) v_f^2+\text{Energy lost due to collision}}$
• Substituting the values, we get:
$\mathbf\small{\frac{1}{2}\times 0.012 \times 70^2+\frac{1}{2}\times 0.4 \times 0^2=\frac{1}{2}\times (0.412) v_f^2+\text{Energy lost}}$
$\mathbf\small{\Rightarrow 29.4=0.206\;v_f^2+\text{Energy lost}}$
7. If there is no external force acting on the system, the law of conservation of momentum is valid
So we have:
$\mathbf\small{m_A v_{Ai}+m_B v_{Bi}=(m_A+m_B) v_f}$
• Substituting the values, we get:
$\mathbf\small{0.012 \times 70+0.4 \times 0=0.412\;v_f}$
$\mathbf\small{\Rightarrow 0.84=0.412\;v_f}$
$\mathbf\small{\Rightarrow v_f=2.039\;\text{ms}^{-1}}$
8. Substituting this value of vf in (6), we get:
$\mathbf\small{29.4=0.206\times 2.039^2+\text{Energy lost}}$
⇒ Energy lost = 28.54 J
• This is the answer for part (ii)
9. Next, let us apply the law of conservation of energy to the points U and P
■ By the Law of conservation of energy, the total energy must be the same at those two points
• We can write EU = EP
12. Let us write the various energies:
(i) Total energy EU:
• Kinetic energy = $\mathbf\small{\frac{m_{(A+B)}\,v_f^2}{2}}$
• Gravitational potential energy = 0
■ So total energy EA = $\mathbf\small{\frac{m_{(A+B)}\,v_f^2}{2}}$
(ii) Total energy EP
• Kinetic energy = 0
• Gravitational potential energy = $\mathbf\small{m_{(A+B)}gh}$ 
■ So total energy EP = $\mathbf\small{m_{(A+B)}gh}$
13. Equating the two energies we get:
$\mathbf\small{\frac{m_{(A+B)}\,v_f^2}{2}=m_{(A+B)}gh}$
$\mathbf\small{\Rightarrow \frac{v_f^2}{2}=gh}$
$\mathbf\small{\Rightarrow h=\frac{v_f^2}{2g}}$
• Substituting the known values, we get:
$\mathbf\small{h=\frac{2.039^2}{2 \times 9.8}=0.212\;\text{m}}$
• This is the answer for part (i)


So we have seen the discussion on 'completely inelastic collision'. It was illustrated in the second row 'b' in fig.6.64 above. Now we take up the third row 'c'.
1. Consider the row 'c', column '1' in fig.6.64 above.
• Two objects A and B of masses mA and mB move towards each other
• Their initial velocities are respectively vAi and vBi
    ♦ vAi is 'velocity of A (initial)'
    ♦ vBi is 'velocity of B (initial)'
2. Row 'b', column '2' shows the instant at which collision takes place
• We see that both the masses undergo deformation
    ♦ A is compressed due to the impact
    ♦ B is also compressed due to the impact
3. Assume that, the masses are neither 'perfectly elastic' nor  'perfectly inelastic'
• Since they are not 'perfectly elastic', they will not 'fully regain' their original shapes 
• Since they are not 'perfectly inelastic', they will not stay in the 'deformed shape'
■ So this is an intermediate state between 'elastic collision' and 'completely inelastic collision'
4. After collision, they will move separately with velocities vAf and vBf
• Also there will be some 'lost energy'. We can be sure about this because, the original shapes are not regained
• In other words, some energy is lost for 'causing the deformations'
5. So there are 3 unknowns: vAf vBf and 'lost energy'  
• But we have only two equations:
(i) $\mathbf\small{m_A v_{Ai}+m_B v_{Bi}=m_A v_{Af}+m_B v_{Bf}}$
(ii) $\mathbf\small{\frac{1}{2}m_A v_{Ai}^2+\frac{1}{2}m_B v_{Bi}^2=\frac{1}{2}m_A v_{Af}^2+\frac{1}{2}m_B v_{Bf}^2+\text{Energy lost due to collision}}$
• We will see the methods to solve such problems in higher classes

• The collisions that we saw in this section and in the previous section, were all one-dimensional collisions. They are also called head-on collisions
• We will see more details about such collisions in the next section. After that, we will discuss about two-dimensional collisions

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Saturday, March 2, 2019

Chapter 6.21 - Elastic Collisions

In the previous section, we completed a discussion on power. In this section we will see collisions

• In a previous chapter, we saw the Law of conservation of Momentum (Details here
• In a previous section of the present chapter, we saw the law of conservation of Energy (Details here)
• We are now going to apply these two laws to a common phenomenon that we encounter in our day-to-day life, which is: collisions

1. Consider the row 'a', column '1' in fig.6.64 below:
Fig.6.64
• Two objects A and B of masses mA and mB move towards each other
• Their initial velocities are respectively vAi and vBi
    ♦ vAi is 'velocity of A (initial)'
    ♦ vBi is 'velocity of B (initial)'
2. Row 'a', column '2' shows the instant at which collision takes place
• We see that both the masses undergo deformation
    ♦ A is compressed due to the impact
    ♦ B is also compressed due to the impact
3. Assume that, both the masses are made of 'perfectly elastic' materials
• So they regain their original shapes after impact
• After impact, they move with velocities vAf and vBf
    ♦ vAf is 'velocity of A (final)'
    ♦ vBf is 'velocity of B (final)'
• This is shown in row 'a', column '3'
4. This situation is just like compressing and releasing a spring
• The energy used up for compressing the spring will be obtained back when the spring is released
• So there is no net change in energy
5. That means, in an elastic collision, 
Total energy before collision = Total energy after collision
6. But the two masses are at the same level
• The levels do not change even after collision
• So they have the same gravitational potential energy before and after collision
• Thus, we need not consider the gravitational potential energy 
7. So the result in (5) becomes:
■ In an elastic collision, 
Total kinetic energy before collision = Total kinetic energy after collision
That is:
$\mathbf\small{\frac{1}{2}m_A v_{Ai}^2+\frac{1}{2}m_B v_{Bi}^2=\frac{1}{2}m_A v_{Af}^2+\frac{1}{2}m_B v_{Bf}^2}$
Thus we get:
$\mathbf\small{m_A v_{Ai}^2+m_B v_{Bi}^2=m_A v_{Af}^2+m_B v_{Bf}^2}$
8. If there is no external force acting on the system, the law of conservation of momentum is valid
So we have:
$\mathbf\small{m_A v_{Ai}+m_B v_{Bi}=m_A v_{Af}+m_B v_{Bf}}$ (Details here)
9. Equations in (7) and (8) can be used together, to solve problems in 'one-dimensional elastic collisions'

Solved example 6.33
Two objects undergo a one-dimensional elastic collision (Fig.6.65 below)
Fig.6.65
Calculate their velocities after collision. Given that: mA = 0.5 kg, mB = 3.5 kg, vAi = 4 ms-1, vBi = 0
Solution:
• We are required to find vAf and vBf
1. In an elastic collision, kinetic energy is conserved. So we have:
$\mathbf\small{m_A v_{Ai}^2+m_B v_{Bi}^2=m_A v_{Af}^2+m_B v_{Bf}^2}$
• Substituting the values, we get:
$\mathbf\small{0.5 \times 4^2+3.5 \times 0^2=0.5 v_{Af}^2+3.5 v_{Bf}^2}$
$\mathbf\small{\Rightarrow 16=v_{Af}^2+7 v_{Bf}^2}$
2. If there is no external force acting on the system, the law of conservation of momentum is valid
• So we have:
$\mathbf\small{m_A v_{Ai}+m_B v_{Bi}=m_A v_{Af}+m_B v_{Bf}}$
• Substituting the values, we get:
$\mathbf\small{0.5 \times 4+3.5 \times 0=0.5v_{Af}+3.5 v_{Bf}}$
$\mathbf\small{\Rightarrow 4=v_{Af}+7 v_{Bf}}$
$\mathbf\small{\Rightarrow v_{Af}=4-7 v_{Bf}}$
3. Substituting this value of vAf in (1), we get:
$\mathbf\small{16=(4-7 v_{Bf})^2+7 v_{Bf}^2}$
$\mathbf\small{\Rightarrow 16=16-56v_{Bf}+49v_{Bf}^2+7v_{Bf}^2}$
$\mathbf\small{\Rightarrow 0=-56v_{Bf}+56v_{Bf}^2}$
$\mathbf\small{\Rightarrow 0 =56v_{Bf}(-1+v_{Bf})}$
$\mathbf\small{\Rightarrow v_{Bf}=0\,\, \text{OR}\,\,v_{Bf}=1\,\, \text{ms}^{-1}}$
4. Substituting these values of vBf in (2), we get:
vAf = 4 ms-1 OR vAf = -3 ms-1.
5. Let us analyse the results:
• 'A' moved with a certain velocity and collided with 'B' (which was stationary)
• Since there is no external force, B will certainly move. So the result 'vBf = 0' should be discarded
• We get vBf = 1
• When vBf = 1, vAf is -3
• So the required result is: vAf = -3 vBf = 1
• This result is understandable
• A small mass (mA = 0.5 kg) moves towards the right (∵ vAi is positive)
• It collides with a larger mass (mB = 3.5 kg) which was stationary       
• As a result of the collision, 
    ♦ the larger mass move towards the right (∵ vBf is positive)
    ♦ the smaller mass rebounds and moves to the left ( vAf is negative)

• If one of the masses is initially at rest, calculations become simpler. For such cases, we can derive some formulas. They will help us to solve problems quickly. We will write the steps:
1. Applying conservation of kinetic energy, we have:
$\mathbf\small{m_A v_{Ai}^2+m_B v_{Bi}^2=m_A v_{Af}^2+m_B v_{Bf}^2}$
• Where mA is the mass of A
• mB is the mass of B
• vAi is the initial velocity of A
• vBi is the initial velocity of B
• vAf is the final velocity of A
• vBf is the final velocity of B
2. But B is initially at rest. So vBi = 0
• So the equation becomes: $\mathbf\small{m_A v_{Ai}^2=m_A v_{Af}^2+m_B v_{Bf}^2}$
3. Applying the law of conservation of momentum, we have:
$\mathbf\small{m_A v_{Ai}+m_B v_{Bi}=m_A v_{Af}+m_B v_{Bf}}$
• But B is initially at rest. So vBi = 0
• So the equation becomes: $\mathbf\small{m_A v_{Ai}=m_A v_{Af}+m_B v_{Bf}}$ 
4. The result in (3) is: $\mathbf\small{m_A v_{Ai}=m_A v_{Af}+m_B v_{Bf}}$
• Multiply both sides by vBf. We get: $\mathbf\small{m_A v_{Ai}v_{Bf}=m_A v_{Af}v_{Bf}+m_B v_{Bf}^2}$
$\mathbf\small{\Rightarrow m_B v_{Bf}^2=m_A v_{Ai}v_{Bf}-m_A v_{Af}v_{Bf}}$
5. We can put this in the place of $\mathbf\small{m_B v_{Bf}^2}$ in (2). We get:
$\mathbf\small{m_A v_{Ai}^2=m_A v_{Af}^2+m_A v_{Ai}v_{Bf}-m_A v_{Af}v_{Bf}}$
$\mathbf\small{\Rightarrow  v_{Ai}^2= v_{Af}^2+ v_{Ai}v_{Bf}- v_{Af}v_{Bf}}$
$\mathbf\small{\Rightarrow  v_{Ai}^2-v_{Af}^2= v_{Bf}(v_{Ai}- v_{Af})}$
$\mathbf\small{\Rightarrow  (v_{Ai}+ v_{Af})(v_{Ai}- v_{Af})= v_{Bf}(v_{Ai}- v_{Af})}$
$\mathbf\small{\Rightarrow  (v_{Ai}+ v_{Af})= v_{Bf}}$
6. We can use this value of $\mathbf\small{v_{Bf}}$ in (3). We get:
$\mathbf\small{m_A v_{Ai}=m_A v_{Af}+m_B (v_{Ai}+ v_{Af})}$
$\mathbf\small{\Rightarrow m_A v_{Ai}=m_A v_{Af}+m_Bv_{Ai}+ m_Bv_{Af}}$
$\mathbf\small{\Rightarrow (m_A-m_B) v_{Ai}=(m_A + m_B)v_{Af}}$
$\mathbf\small{\Rightarrow v_{Af}=\frac{(m_A-m_B)v_{Ai}}{(m_A + m_B)}}$
• Thus we get the final velocity of A in terms of the three known quantities: 
(i) Mass of A
(ii) Mass of B
(iii) Initial velocity of A
7. We can obtain the final velocity of B also
• For that, we put the above obtained value of $\mathbf\small{v_{Af}}$ in (5). We get:  
$\mathbf\small{v_{Ai}+ \frac{(m_A-m_B)v_{Ai}}{(m_A + m_B)}= v_{Bf}}$
$\mathbf\small{\Rightarrow \frac{(m_A+m_B)v_{Ai}+(m_A-m_B)v_{Ai}}{(m_A + m_B)}= v_{Bf}}$
$\mathbf\small{\Rightarrow v_{Bf}=\frac{2m_Av_{Ai}}{(m_A + m_B)}}$
• Thus we get the final velocity of B in terms of the three known quantities: 
(i) Mass of A
(ii) Mass of B
(iii) Initial velocity of A
8. Some interesting special cases can be analysed using the above expressions
Case 1: The two masses are equal
• When the two masses are equal, we can put: mA = mB = m
• Then from (6) we get: $\mathbf\small{\Rightarrow v_{Af}=\frac{(m-m)v_{Ai}}{(m + m)}=0}$
• From (7) we get: $\mathbf\small{v_{Bf}=\frac{2m\;v_{Ai}}{(m + m)}=v_{Ai}}$  
• So 'case 1' can be written in the following 6 steps:
(i) Two bodies 'A' and 'B' collide elastically with each other
(ii) The two masses are equal. That is., mA = mB = m  
(iii) Before the collision, 'A' was moving with a velocity vAi
(iv) Before the collision, 'B' was stationary. That is., vBi = 0
[Remember that, the equations in (6) and (7) are valid only if 'B' is initially at rest]
(v) After the collision, 'A' becomes stationary
(vi) After the collision, 'B' begins to move with vAi (the same velocity with which 'A' was moving)
Case 2: One of the two masses is very large when compared to the other
• Let us assume mB >> mA
• Then (mA-mB) will be very nearly equal to -mB
(That is., mA ≃ 0)
• Also (mA+mAwill be very nearly equal to mB
• Then from (6) we get: $\mathbf\small{v_{Af}=\frac{(-m_B)v_{Ai}}{( m_B)}=-v_{Ai}}$ 
• From (7) we get: $\mathbf\small{v_{Bf}=\frac{2\times 0\times v_{Ai}}{(0 + m_B)}=0}$   
• So 'case 2' can be written in the following 6 steps:
(i) Two bodies 'A' and 'B' collide elastically with each other
(ii) mB >> mA
(iii) Before the collision, 'A' was moving with a velocity vAi
(iv) Before the collision, 'B' was stationary. That is., vBi = 0
[Remember that, the equations in (6) and (7) are valid only if 'B' is initially at rest]
(v) After the collision, 'A' begins to move with -vAi 
(the same magnitude but opposite direction of the velocity with which 'A' was moving)
(vi) After the collision, 'B' remains stationary

In the solved example 6.33, one of the two objects is at rest. So the formulas should be applicable. Let us check:
1. Given that: mA = 0.5 kg, mB = 3.5 kg, vAi = 4 ms-1, vBi = 0
2. We have: $\mathbf\small{v_{Af}=\frac{(m_A-m_B)v_{Ai}}{(m_A + m_B)}}$
Substituting the known values, we get:
$\mathbf\small{v_{Af}=\frac{(0.5-3.5)\times 4}{(0.5 + 3.5)}=-3\,\,\text{ms}^{-1}}$ (Same as before)
3. We have: $\mathbf\small{v_{Bf}=\frac{2m_Av_{Ai}}{(m_A + m_B)}}$
Substituting the known values, we get:
$\mathbf\small{v_{Bf}=\frac{2\times 0.5\times 4}{(0.5 + 3.5)}=1\,\,\text{ms}^{-1}}$ (Same as before)

Solved example 6.34
In a nuclear reactor, a neutron of high speed (typically 107 ms-1) must be slowed to 103 ms-1. So that it can have a high probability of interacting with isotope $\mathbf\small{\overset{235}{\underset{92}{}}\text{U}}$ and causing it to fission. Show that a neutron can  lose most of it's kinetic energy in an elastic collision with a light nuclei like deuterium which has only a few times the neutron mass. The material making up the light nuclei, usually heavy water (D2O) or graphite, is called a moderator
Solution:
1. We want to slow down a neutron
• We have to achieve this by making the neutron to collide with a deuterium nucleus
• This is shown in fig.6.66 below:
Fig.6.66
• It is an elastic collision
• We want to show that deuterium can be effectively used for slowing down a neutron
2. The deuterium nucleus is initially at rest. So we will use the formula:
$\mathbf\small{v_{Af}=\frac{(m_A-m_B)v_{Ai}}{(m_A + m_B)}}$
• Where mA is the mass of neutron
• mB is the mass of deuterium
• vAi is the initial velocity of neutron
• vAf is the final velocity of neutron
3. We have: $\mathbf\small{v_{Af}=\frac{(m_A-m_B)v_{Ai}}{(m_A + m_B)}}$
So final kinetic energy of the neutron (KAf
$\mathbf\small{\frac{1}{2}m_A\,v_{Af}^2=\frac{1}{2}m_A\,\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2v_{Ai}^2}$
4. Initial kinetic energy of the neutron (KAi) = $\mathbf\small{\frac{1}{2}m_A\,v_{Ai}^2}$
5. Now take the ratio: $\mathbf\small{\frac{K_{Af}}{K_{Ai}}}$
• That is., ratio of the initial kinetic energy of neutron to it's final kinetic energy
• We will denote it as fA
• We have:
$\mathbf\small{f_A=\frac{K_{Af}}{K_{Ai}}=\frac{\frac{1}{2}m_A\,\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2v_{Ai}^2}{\frac{1}{2}m_A\,v_{Ai}^2}=\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2}$
6. So we can write:
Final kinetic energy of the neutron is $\mathbf\small{\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2}$ times it's initial kinetic energy      
• The numerator (mA-mB) will be less than the denominator (mA+mB)
• So the ratio $\mathbf\small{\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2}$ is a fraction. It is not a whole number
• So final kinetic energy of the neutron will be certainly less than it's initial kinetic energy
• That means the final velocity of the neutron will be certainly less than the initial kinetic energy
• That means the neutron will be certainly slowed down 
7. But knowing that the 'neutron will be slowed down' is not good enough
• We want to know 'how much slowing down' can be achieved
• If the neutron is not slowed down to a required value, the uranium nucleus will not be able to capture it
8. So we proceed as follows:
• Since it is an elastic collision, 
Initial kinetic energy of the neutron-deuterium system = It's final kinetic energy
9. But initial velocity of deuterium = 0
• So initial kinetic energy of the system is contributed by the neutron alone
• That is., initial kinetic energy of the system = initial kinetic energy of the neutron 
$\mathbf\small{\frac{1}{2}m_A\,v_{Ai}^2}$      
10. Combining (8) and (9), we get:
• Final kinetic energy of the system = Kf = KAi $\mathbf\small{\frac{1}{2}m_A\,v_{Ai}^2}$
11. But the final kinetic energy of the system is made up by two items:
(i) Final kinetic energy of neutron KAf = $\mathbf\small{\frac{1}{2}m_A\,v_{Af}^2}$ 
(ii) Final kinetic energy of deuterium KBf = $\mathbf\small{\frac{1}{2}m_A\,v_{Bf}^2}$  
• So we can write: Kf = KAi KAf KBf
12. Take out the second and third terms. We get: KAi KAf KBf
Divide both sides by KAi. We get: $\mathbf\small{1=\frac{K_{Af}}{K_{Ai}}+\frac{K_{Bf}}{K_{Ai}}}$
13. But we have already calculated $\mathbf\small{\frac{K_{Af}}{K_{Ai}}}$ in (5)
• We have: $\mathbf\small{\frac{K_{Af}}{K_{Ai}}=\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2}$
• So the result in (12) becomes: $\mathbf\small{1=\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2+\frac{K_{Bf}}{K_{Ai}}}$
$\mathbf\small{\Rightarrow \frac{K_{Bf}}{K_{Ai}}=1-\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2}$
$\mathbf\small{\Rightarrow \frac{K_{Bf}}{K_{Ai}}=\frac{(m_A+m_B)^2-(m_A-m_B)^2}{(m_A + m_B)^2}}$
$\mathbf\small{\Rightarrow \frac{K_{Bf}}{K_{Ai}}=\frac{(m_A+m_B+m_A-m_B)(m_A+m_B-m_A+m_B)}{(m_A + m_B)^2}}$
$\mathbf\small{\left[\text{Using the identity}:(a^2-b^2)=(a+b)(a-b) \right]}$
$\mathbf\small{\Rightarrow \frac{K_{Bf}}{K_{Ai}}=\frac{(2m_A)(2m_B)}{(m_A + m_B)^2}}$
$\mathbf\small{\Rightarrow \frac{K_{Bf}}{K_{Ai}}=\frac{4m_A\;m_B}{(m_A + m_B)^2}}$
14. So we have two ratios:
(i) From (5) we have: $\mathbf\small{\frac{K_{Af}}{K_{Ai}}=\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2}$
(ii) From (13) we have: $\mathbf\small{\frac{K_{Bf}}{K_{Ai}}=\frac{4m_A\;m_B}{(m_A + m_B)^2}}$
15.  Given that: deuterium has only a few times the neutron mass  
Assume that mB = 2 mA
(i) Then from 14(i), we get:
$\mathbf\small{\frac{K_{Af}}{K_{Ai}}=\left[\frac{m_A-m_B}{m_A + m_B}\right ]^2=\left[\frac{m_A-2m_A}{m_A + 2m_A}\right ]^2=\frac{1}{9}}$ 
(ii) From 14(ii) we get:
$\mathbf\small{\frac{K_{Bf}}{K_{Ai}}=\frac{4m_A\;m_B}{(m_A + m_B)^2}=\frac{4m_A\times 2m_A}{(m_A + 2m_A)^2}=\frac{8}{9}}$
16. So from 15(i) we get:
• Final kinetic energy of neutron is 1of initial kinetic energy of neutron
⇒ Final kinetic energy of neutron is 1of total kinetic energy of the system
• From 15(ii) we get:
Final kinetic energy of deuterium is 8of initial kinetic energy of neutron
⇒ Final kinetic energy of deuterium is 8of total kinetic energy of the system
• In percentage form:
1= 11.1% 
8= 88.9%
17. So we can write:
• After the collision with deuterium, the neutron loses (100-11.1) = 88.9% of it's initial kinetic energy
    ♦ That means., the neutron will be left with only 11.1% of it's initial energy
• The lost 88.9% is acquired by the deuterium
18. Instead of deuterium, we can use carbon (graphite) as the moderator
• The formulas are the same that we wrote in (14)
• The only difference is this:
    ♦ When deuterium is used, we wrote: mB = 2 × mA
    ♦ When carbon is used, we can write: mB = k × mA
    ♦ We must put a suitable value for 'k'
• The results obtained are as follows:
After the collision with carbon, the neutron loses 71.6% of it's initial kinetic energy
    ♦ That means., the neutron will be left with only (100-71.6) = 28.4% of it's initial energy
• The lost 71.6% is acquired by the carbon

• So deuterium and carbon are very effective moderators
• However high losses like 88.9% and 71.6% can be achieved only if the neutron does a head-on collision with deuterium or carbon
• We will see the details of head-on collisions in a later section

In the next section we will see inelastic collisions

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