5.1 INTRODUCTION

The terms ‘work’, ’energy’ and ‘power’ are frequently used in everyday language. A farmer ploughing the field, a construction worker carrying bricks, a student studying for a competitive examination, an artist painting a beautiful landscape, all are said to be working. In physics, however, the word ‘Work’ covers a definite and precise meaning. Somebody who has the capacity to work for 14-16 hours a day is said to have a large stamina or energy. We admire a long distance runner for her stamina or energy. Energy is thus our capacity to do work. In Physics too, the term ’energy’ is related to work in this sense, but as said above the term ‘work’ itself is defined much more precisely. The word ‘power’ is used in everyday life with different shades of meaning. In karate or boxing we talk of ‘powerful’ punches. These are delivered at a great speed. This shade of meaning is close to the meaning of the word ‘power’ used in physics. We shall find that there is at best a loose correlation between the physical definitions and the physiological pictures these terms generate in our minds. The aim of this chapter is to develop an understanding of these three physical quantities. Before we proceed to this task, we need to develop a mathematical prerequisite, namely the scalar product of two vectors.

5.1.1 The Scalar Product

We have learnt about vectors and their use in Chapter 3. Physical quantities like displacement, velocity, acceleration, force etc. are vectors. We have also learnt how vectors are added or subtracted. We now need to know how vectors are multiplied. There are two ways of multiplying vectors which we shall come across : one way known as the scalar product gives a scalar from two vectors and the other known as the vector product produces a new vector from two vectors. We shall look at the vector product in Chapter 6. Here we take up the scalar product of two vectors. The scalar product or dot product of any two vectors A and B, denoted as A.B (read $\mathbf{A} \operatorname{dot} \mathbf{B}$) is defined as

$$ \begin{equation*} \mathbf{A} \cdot \mathbf{B}=A B \cos \theta \tag{5.1a} \end{equation*} $$

where $\theta$ is the angle between the two vectors as shown in Fig. 5.1(a). Since $A, B$ and $\cos \theta$ are scalars, the dot product of $\mathbf{A}$ and $\mathbf{B}$ is a scalar quantity. Each vector, $\mathbf{A}$ and $\mathbf{B}$, has a direction but their scalar product does not have a direction.

From Eq. (5.1a), we have

$$ \begin{aligned} \mathbf{A} \cdot \mathbf{B} & =A(B \cos \theta) \\ & =B(A \cos \theta) \end{aligned} $$

Geometrically, $B \cos \theta$ is the projection of $\mathbf{B}$ onto $\mathbf{A}$ in Fig.5.1 (b) and $A \cos \theta$ is the projection of $\mathbf{A}$ onto $\mathbf{B}$ in Fig. 5.1 (c). So, A.B is the product of the magnitude of $\mathbf{A}$ and the component of $\mathbf{B}$ along A. Alternatively, it is the product of the magnitude of $\mathbf{B}$ and the component of $\mathbf{A}$ along $\mathbf{B}$.

Equation (5.1a) shows that the scalar product follows the commutative law :

$\mathbf{A} \cdot \mathbf{B}=\mathbf{B} \cdot \mathbf{A}$

Scalar product obeys the distributive law:

$\mathbf{A} \cdot(\mathbf{B}+\mathbf{C})=\mathbf{A} \cdot \mathbf{B}+\mathbf{A} \cdot \mathbf{C}$

Further, $\quad \mathbf{A} \cdot(\lambda \mathbf{B})=\lambda(\mathbf{A} \cdot \mathbf{B})$

where $\lambda$ is a real number.

The proofs of the above equations are left to you as an exercise.

For unit vectors $\hat{\mathbf{i}}, \hat{\mathbf{j}}, \hat{\mathbf{k}}$ we have

$$ \begin{aligned} & \hat{\mathbf{i}} \cdot \hat{\mathbf{i}}=\hat{\mathbf{j}} \cdot \hat{\mathbf{j}}=\hat{\mathbf{k}} \cdot \hat{\mathbf{k}}=1 \\ & \hat{\mathbf{i}} \cdot \hat{\mathbf{j}}=\hat{\mathbf{j}} \cdot \hat{\mathbf{k}}=\hat{\mathbf{k}} \cdot \hat{\mathbf{i}}=0 \end{aligned} $$

Given two vectors

$$ \begin{aligned} & \mathbf{A}=A_{x} \hat{\mathbf{i}}+A_{y} \hat{\mathbf{j}}+A_{z} \hat{\mathbf{k}} \\ & \mathbf{B}=B_{x} \hat{\mathbf{i}}+B_{y} \hat{\mathbf{j}}+B_{z} \hat{\mathbf{k}} \end{aligned} $$

their scalar product is

$$ \begin{align*} & \mathbf{A} \cdot \mathbf{B}=\left(A_{x} \hat{\mathbf{i}}+A_{y} \hat{\mathbf{j}}+A_{z} \hat{\mathbf{k}}\right) \cdot\left(B_{x} \hat{\mathbf{i}}+B_{y} \hat{\mathbf{j}}+B_{z} \hat{\mathbf{k}}\right) \\ & =A_{x} B_{x}+A_{y} B_{y}+A_{z} B_{z} \tag{5.1b} \end{align*} $$

From the definition of scalar product and (Eq. 5.1b) we have :

$$ \begin{equation*} \text{(i)} \quad \quad \quad \quad \mathbf{A} \cdot \mathbf{A}=A_{x} A_{x}+A_{y} A_{y}+A_{z} A_{z} \end{equation*} $$

$$\text{Or, } \quad\quad\quad\quad A^{2}=A_{x}^{2}+A_{y}^{2}+A_{z}^{2} \tag{5.1c}$$

since $\mathbf{A} \cdot \mathbf{A}=|\mathbf{A}||\mathbf{A}| \cos 0=A^{2}$.

(ii) $\mathbf{A} \cdot \mathbf{B}=0$, if $\mathbf{A}$ and $\mathbf{B}$ are perpendicular.

5.2 NOTIONS OF WORK AND KINETIC ENERGY: THE WORK-ENERGY THEOREM

The following relation for rectilinear motion under constant acceleration $a$ has been encountered in Chapter 3,

$$ \begin{equation*} v^{2}-u^{2}=2 a s \tag{5.2} \end{equation*} $$

where $u$ and $v$ are the initial and final speeds and $s$ the distance traversed. Multiplying both sides by $m / 2$, we have

$$ \begin{equation*} \frac{1}{2} m v^{2}-\frac{1}{2} m u^{2}=m a s=F s \tag{5.2a} \end{equation*} $$

where the last step follows from Newton’s Second Law. We can generalise Eq. (5.2) to three dimensions by employing vectors

$$ v^{2}-u^{2}=2 \text { a.d } $$

Here $\mathbf{a}$ and $\mathbf{d}$ are acceleration and displacement vectors of the object respectively.

Once again multiplying both sides by $\mathrm{m} / 2$, we obtain

$$ \begin{equation*} \frac{1}{2} m v^{2}-\frac{1}{2} m u^{2}=m \mathbf{a} \cdot \mathbf{d}=\mathbf{F} . \mathbf{d} \tag{5.2b} \end{equation*} $$

The above equation provides a motivation for the definitions of work and kinetic energy. The left side of the equation is the difference in the quantity ‘half the mass times the square of the speed’ from its initial value to its final value. We call each of these quantities the ‘kinetic energy’, denoted by $K$. The right side is a product of the displacement and the component of the force along the displacement. This quantity is called ‘work’ and is denoted by W. Eq. (5.2b) is then

$$ \begin{equation*} K_{f}-K_{i}=W \tag{5.3} \end{equation*} $$

where $K_{i}$ and $K_{f}$ are respectively the initial and final kinetic energies of the object. Work refers to the force and the displacement over which it acts. Work is done by a force on the body over a certain displacement.

Equation (5.2) is also a special case of the work-energy (WE) theorem : The change in kinetic energy of a particle is equal to the work done on it by the net force. We shall generalise the above derivation to a varying force in a later section.

5.3 WORK

As seen earlier, work is related to force and the displacement over which it acts. Consider a constant force $\mathbf{F}$ acting on an object of mass $m$. The object undergoes a displacement $\mathbf{d}$ in the positive $x$-direction as shown in Fig. 5.2.

The work done by the force is defined to be the product of component of the force in the direction of the displacement and the magnitude of this displacement. Thus

$$ \begin{equation*} W=(F \cos \theta) d=\mathbf{F} \cdot \mathbf{d} \tag{5.4} \end{equation*} $$

We see that if there is no displacement, there is no work done even if the force is large. Thus, when you push hard against a rigid brick wall, the force you exert on the wall does no work. Yet your muscles are alternatively contracting and relaxing and internal energy is being used up and you do get tired. Thus, the meaning of work in physics is different from its usage in everyday language.

No work is done if :

(i) the displacement is zero as seen in the example above. A weightlifter holding a 150 $\mathrm{kg}$ mass steadily on his shoulder for $30 \mathrm{~s}$ does no work on the load during this time.

(ii) the force is zero. A block moving on a smooth horizontal table is not acted upon by a horizontal force (since there is no friction), but may undergo a large displacement.

(iii) the force and displacement are mutually perpendicular. This is so since, for $\theta=\pi / 2 \mathrm{rad}$ $\left(=90^{\circ}\right), \cos (\pi / 2)=0$. For the block moving on a smooth horizontal table, the gravitational force $m g$ does no work since it acts at right angles to the displacement. If we assume that the moon’s orbits around the earth is perfectly circular then the earth’s gravitational force does no work. The moon’s instantaneous displacement is tangential while the earth’s force is radially inwards and $\theta=\pi / 2$.

Work can be both positive and negative. If $\theta$ is between $0^{\circ}$ and $90^{\circ}, \cos \theta$ in Eq. (5.4) is positive. If $\theta$ is between $90^{\circ}$ and $180^{\circ}, \cos \theta$ is negative. In many examples the frictional force opposes displacement and $\theta=180^{\circ}$. Then the work done by friction is negative $\left(\cos 180^{\circ}=-1\right)$.

From Eq. (5.4) it is clear that work and energy have the same dimensions, $\left[\mathrm{ML}^{2} \mathrm{~T}^{-2}\right]$. The SI unit of these is joule (J), named after the famous British physicist James Prescott Joule (1811-1869). Since work and energy are so widely used as physical concepts, alternative units abound and some of these are listed in Table 5.1.

Table 5.1 Alternative Units of Work/Energy in $\mathrm{J}$

5.4 KINETIC ENERGY

As noted earlier, if an object of mass $m$ has velocity $\mathbf{v}$, its kinetic energy $K$ is

$$ \begin{equation*} K=\frac{1}{2} m \mathbf{v} \cdot \mathbf{v}=\frac{1}{2} m v^{2} \tag{5.5} \end{equation*} $$

Kinetic energy is a scalar quantity. The kinetic energy of an object is a measure of the work an

Table 5.2 Typical kinetic energies (K)

object can do by the virtue of its motion. This notion has been intuitively known for a long time. The kinetic energy of a fast flowing stream has been used to grind corn. Sailing ships employ the kinetic energy of the wind. Table 5.2 lists the kinetic energies for various objects.

5.5 WORK DONE BY A VARIABLE FORCE

A constant force is rare. It is the variable force, which is more commonly encountered. Fig. 5.3 is a plot of a varying force in one dimension.

If the displacement $\Delta x$ is small, we can take the force $F(x)$ as approximately constant and the work done is then

$$ \Delta W=F(x) \Delta x $$

This is illustrated in Fig. 5.3(a). Adding successive rectangular areas in Fig. 5.3(a) we get the total work done as

$$ \begin{equation*} W \cong \sum_{x_{i}}^{x_{f}} F(x) \Delta x \tag{5.6} \end{equation*} $$

where the summation is from the initial position $x_{i}$ to the final position $x_{f}$

If the displacements are allowed to approach zero, then the number of terms in the sum increases without limit, but the sum approaches a definite value equal to the area under the curve in Fig. 5.3(b). Then the work done is

$$W =\lim\limits_{\Delta x \rightarrow 0} \sum_{x_{i}}^{x_{f}} F(x) \Delta x$$

$$=\int\limits_{x_i}^{x_f} F(x) \mathrm{d} x \tag{5.7}$$

where ’lim’ stands for the limit of the sum when $\Delta x$ tends to zero. Thus, for a varying force the work done can be expressed as a definite integral of force over displacement (see also Appendix 3.1).

5.6 THE WORK-ENERGY THEOREM FOR A VARIABLE FORCE

We are now familiar with the concepts of work and kinetic energy to prove the work-energy theorem for a variable force. We confine ourselves to one dimension. The time rate of change of kinetic energy is

$$ \frac{\mathrm{d} K}{\mathrm{~d} t}=\frac{\mathrm{d}}{\mathrm{d} t} \frac{1}{2} m v^{2} $$

$$ \begin{aligned} & =m \frac{\mathrm{d} v}{\mathrm{~d} t} v \\ & =F v\text { (from Newton’s Second Law) } \\ & =F \frac{\mathrm{d} x}{\mathrm{~d} t} \end{aligned} $$

Thus

$$ \mathrm{d} K=F \mathrm{~d} x $$

Integrating from the initial position $\left(x_{i}\right)$ to final position $\left(x_{f}\right.$ ), we have

$$ \int_{K_{i}}^{K_{f}} \mathrm{~d} K=\int_{x_{i}}^{x_{f}} F \mathrm{~d} x $$

where, $K_{i}$ and $K_{f}$ are the initial and final kinetic energies corresponding to $x_{i}$ and $x_{\mathrm{f}}$.

$$ \begin{equation*} \text { or } \quad K_{f}-K_{i}=\int_{x_{i}}^{x_{f}} F \mathrm{~d} x \tag{5.8a} \end{equation*} $$

From Eq. (5.7), it follows that

$$ \begin{equation*} K_{f}-K_{i}=W \tag{5.8b} \end{equation*} $$

Thus, the WE theorem is proved for a variable force.

While the WE theorem is useful in a variety of problems, it does not, in general, incorporate the complete dynamical information of Newton’s second law. It is an integral form of Newton’s second law. Newton’s second law is a relation between acceleration and force at any instant of time. Work-energy theorem involves an integral over an interval of time. In this sense, the temporal (time) information contained in the statement of Newton’s second law is ‘integrated over’ and is not available explicitly. Another observation is that Newton’s second law for two or three dimensions is in vector form whereas the work-energy theorem is in scalar form. In the scalar form, information with respect to directions contained in Newton’s second law is not present.

5.7 THE CONCEPT OF POTENTIAL ENERGY

The word potential suggests possibility or capacity for action. The term potential energy brings to one’s mind ‘stored’ energy. A stretched bow-string possesses potential energy. When it is released, the arrow flies off at a great speed. The earth’s crust is not uniform, but has discontinuities and dislocations that are called fault lines. These fault lines in the earth’s crust are like ‘compressed springs’. They possess a large amount of potential energy. An earthquake results when these fault lines readjust. Thus, potential energy is the ‘stored energy’ by virtue of the position or configuration of a body. The body left to itself releases this stored energy in the form of kinetic energy. Let us make our notion of potential energy more concrete.

The gravitational force on a ball of mass $m$ is $m g$. gmay be treated as a constant near the earth surface. By ’near’ we imply that the height $h$ of the ball above the earth’s surface is very small compared to the earth’s radius $R_{E}\left(h«R_{E}\right)$ so that we can ignore the variation of $g$ near the earth’s surface*. In what follows we have taken the upward direction to be positive. Let us raise the ball up to a height $h$. The work done by the external agency against the gravitational force is $m g h$. This work gets stored as potential energy. Gravitational potential energy of an object, as a function of the height $h$, is denoted by $V(h)$ and it is the negative of work done by the gravitational force in raising the object to that height.

$$ V(h)=m g h $$

If $h$ is taken as a variable, it is easily seen that the gravitational force $F$ equals the negative of the derivative of $V(h)$ with respect to $h$. Thus,

$$ F=-\frac{\mathrm{d}}{\mathrm{d} h} V(h)=-m g $$

The negative sign indicates that the gravitational force is downward. When released, the ball comes down with an increasing speed. Just before it hits the ground, its speed is given by the kinematic relation,

$$ v^{2}=2 g h $$

This equation can be written as

$$ \frac{1}{2} m v^{2}=m g h $$

which shows that the gravitational potential energy of the object at height $h$, when the object is released, manifests itself as kinetic energy of the object on reaching the ground.

Physically, the notion of potential energy is applicable only to the class of forces where work done against the force gets ‘stored up’ as energy. When external constraints are removed, it manifests itself as kinetic energy. Mathematically, (for simplicity, in one dimension) the potential energy $V(x)$ is defined if the force $F(x)$ can be written as

$$ F(x)=-\frac{\mathrm{d} V}{\mathrm{~d} x} $$

This implies that

$$ \int_{x_{i}}^{x_{f}} F(x) \mathrm{d} x=-\int_{V_{i}}^{V_{f}} \mathrm{~d} V=V_{i}-V_{f} $$

The work done by a conservative force such as gravity depends on the initial and final positions only. In the previous chapter we have worked on examples dealing with inclined planes. If an object of mass $m$ is released from rest, from the top of a smooth (frictionless) inclined plane of height $h$, its speed at the bottom is $\sqrt{2 g h}$ irrespective of the angle of inclination. Thus, at the bottom of the inclined plane it acquires a kinetic energy, mgh. If the work done or the kinetic energy did depend on other factors such as the velocity or the particular path taken by the object, the force would be called nonconservative.

The dimensions of potential energy are $\left[\mathrm{ML}^{2} \mathrm{~T}^{-2}\right]$ and the unit is joule $(\mathrm{J})$, the same as kinetic energy or work. To reiterate, the change in potential energy, for a conservative force, $\Delta V$ is equal to the negative of the work done by the force

$$ \begin{equation*} \Delta V=-F(x) \Delta x \tag{5.9} \end{equation*} $$

In the example of the falling ball considered in this section we saw how potential energy was converted to kinetic energy. This hints at an important principle of conservation in mechanics, which we now proceed to examine.

5.8 THE CONSERVATION OF MECHANICAL ENERGY

For simplicity we demonstrate this important principle for one-dimensional motion. Suppose that a body undergoes displacement $\Delta x$ under the action of a conservative force $F$. Then from the WE theorem we have,

$$ \Delta K=F(x) \Delta x $$

If the force is conservative, the potential energy function $V(x)$ can be defined such that

$$ -\Delta V=F(x) \Delta x $$

The above equations imply that

$$ \begin{align*} & \Delta K+\Delta V=0 \\ & \Delta(K+V)=0 \tag{5.10} \end{align*} $$

which means that $K+V$, the sum of the kinetic and potential energies of the body is a constant. Over the whole path, $x_{i}$ to $x_{f}$, this means that

$$ \begin{equation*} K_{i}+V\left(x_{i}\right)=K_{f}+V\left(x_{f}\right) \tag{5.11} \end{equation*} $$

The quantity $K+V(x)$, is called the total mechanical energy of the system. Individually the kinetic energy $K$ and the potential energy $V(x)$ may vary from point to point, but the sum is a constant. The aptness of the term ‘conservative force’ is now clear.

Let us consider some of the definitions of a conservative force.

• A force $F(x)$ is conservative if it can be derived from a scalar quantity $V(x)$ by the relation given by Eq. (5.9). The three-dimensional generalisation requires the use of a vector derivative, which is outside the scope of this book.
• The work done by the conservative force depends only on the end points. This can be seen from the relation,

$$ W=K_{f}-K_{i}=V\left(x_{i}\right)-V\left(x_{f}\right) $$

which depends on the end points.

• A third definition states that the work done by this force in a closed path is zero. This is once again apparent from Eq. (5.11) since $x_{i}=x_{f}$.

Thus, the principle of conservation of total mechanical energy can be stated as

The total mechanical energy of a system is conserved if the forces, doing work on it, are conservative.

The above discussion can be made more concrete by considering the example of the gravitational force once again and that of the spring force in the next section. Fig. 5.5 depicts a ball of mass $m$ being dropped from a cliff of height $H$.

The total mechanical energies $E_{0}, E_{h}$, and $E_{H}$ of the ball at the indicated heights zero (ground level), $h$ and $H$, are

$$ \begin{aligned} E_H & =m g H \tag{5.11a}\\ E_h & =m g h + \frac{1}{2} mv_h^2 \\ \end{aligned} $$

$$ \begin{aligned} E_o & =(1 / 2) mv_f^2 \tag{5.11c}\\ \end{aligned} $$

The constant force is a special case of a spatially dependent force $F(x)$. Hence, the mechanical energy is conserved. Thus

$$ \begin{gathered} E_{H}=E_{O} \\ \text { or, } \quad m g H=\frac{1}{2} m v_{f}^{2} \\ v_{f}=\sqrt{2 g H} \end{gathered} $$

a result that was obtained in section 5.7 for a freely falling body.

Further,

$$ E_{H}=E_{h} $$

which implies,

$$ \begin{equation*} v_{\mathrm{h}}^{2}=2 g(H-h) \tag{5.11~d} \end{equation*} $$

and is a familiar result from kinematics.

At the height $H$, the energy is purely potential. It is partially converted to kinetic at height $h$ and is fully kinetic at ground level. This illustrates the conservation of mechanical energy.

5.9 THE POTENTIAL ENERGY OF A SPRING

The spring force is an example of a variable force which is conservative. Fig. 5.7 shows a block attached to a spring and resting on a smooth horizontal surface. The other end of the spring is attached to a rigid wall. The spring is light and may be treated as massless. In an ideal spring, the spring force $F_{s}$ is proportional to $x$ where $x$ is the displacement of the block from the equilibrium position. The displacement could be either positive [Fig. 5.7(b)] or negative [Fig. 5.7(c)]. This force law for the spring is called Hooke’s law and is mathematically stated as

$$ F_{s}=-k x $$

The constant $k$ is called the spring constant. Its unit is $\mathrm{N} \mathrm{m}^{-1}$. The spring is said to be stiff if $k$ is large and soft if $k$ is small.

Suppose that we pull the block outwards as in Fig. 5.7(b). If the extension is $x_{m}$, the work done by the spring force is

$$ \begin{align*} W_{s} & =\int_{0}^{x_{m}} F_{s} \mathrm{~d} x=-\int_{0}^{x_{m}} k x \mathrm{~d} x \\ \\ & =-\frac{k x_{m}^{2}}{2} \tag{5.15} \end{align*} $$

This expression may also be obtained by considering the area of the triangle as in Fig. 5.7(d). Note that the work done by the external pulling force $F$ is positive since it overcomes the spring force.

$$ \begin{equation*} W=+\frac{k x_{m}^{2}}{2} \tag{5.16} \end{equation*} $$

The same is true when the spring is compressed with a displacement $x_{c}(<0)$. The spring force does work $W_{s}=-k x_{c}^{2} / 2$ while the external force $F$ does work $+k x_{c}^{2} / 2$. If the block is moved from an initial displacement $x_{i}$ to a final displacement $x_{f}$, the work done by the spring force $W_{s}$ is

$$ \begin{equation*} W_{s}=-\int_{x_{i}}^{x_{f}} k x \mathrm{~d} x=\frac{k x_{i}^{2}}{2}-\frac{k x_{f}^{2}}{2} \tag{5.17} \end{equation*} $$

Thus the work done by the spring force depends only on the end points. Specifically, if the block is pulled from $x_{i}$ and allowed to return to $x_{i}$;

$$ \begin{align*} W_{s} & =-\int_{x_{i}}^{x_{i}} k x \mathrm{~d} x=\frac{k x_{i}^{2}}{2}-\frac{k x_{i}^{2}}{2} \ & =0 \tag{5.18} \end{align*} $$

The work done by the spring force in a cyclic process is zero. We have explicitly demonstrated that the spring force (i) is position dependent only as first stated by Hooke, $\left(F_{s}=-k x\right)$; (ii) does work which only depends on the initial and final positions, e.g. Eq. (5.17). Thus, the spring force is a conservative force.

We define the potential energy $V(x)$ of the spring to be zero when block and spring system is in the equilibrium position. For an extension (or compression) $x$ the above analysis suggests that

$$ \begin{aligned} V(x)=\frac{k x^{2}}{2} \tag{5.19} \end{aligned} $$

You may easily verify that $-\mathrm{d} V / \mathrm{d} x=-k x$, the spring force. If the block of mass $m$ in Fig. 5.7 is extended to $x_{m}$ and released from rest, then its total mechanical energy at any arbitrary point $x$, where $x$ lies between $-x_{m}$ and $+x_{m}$, will be given by

$$ \frac{1}{2} k x_{m}^{2}=\frac{1}{2} k x^{2}+\frac{1}{2} m v^{2} $$

where we have invoked the conservation of mechanical energy. This suggests that the speed and the kinetic energy will be maximum at the equilibrium position, $x=0$, i.e.,

$$ \frac{1}{2} m v_{m}^{2}=\frac{1}{2} k x_{m}^{2} $$

where $v_{m}$ is the maximum speed.

or $\quad v_{m}=\sqrt{\frac{k}{m}} x_{m}$

Note that $k / m$ has the dimensions of $\left[\mathrm{T}^{-2}\right]$ and our equation is dimensionally correct. The kinetic energy gets converted to potential energy and vice versa, however, the total mechanical energy remains constant. This is graphically depicted in Fig. 5.8.

5.10 POWER

Often it is interesting to know not only the work done on an object, but also the rate at which this work is done. We say a person is physically fit if he not only climbs four floors of a building but climbs them fast. Power is defined as the time rate at which work is done or energy is transferred.

The average power of a force is defined as the ratio of the work, $W$, to the total time $t$ taken

$$ P_{a v}=\frac{W}{t} $$

The instantaneous power is defined as the limiting value of the average power as time interval approaches zero,

$$ \begin{equation*} P=\frac{\mathrm{d} W}{\mathrm{~d} t} \tag{5.20} \end{equation*} $$

The work $d W$ done by a force $\mathrm{F}$ for a displacement $d \mathbf{r}$ is $\mathrm{d} W=\mathbf{F} . d \mathbf{r}$. The instantaneous power can also be expressed as

$$ \begin{align*} & P=\mathbf{F} \cdot \frac{\mathrm{d} \boldsymbol{r}}{\mathrm{d} t} \\ = & \mathbf{F} \cdot \mathbf{v} \tag{5.21} \end{align*} $$

where $\mathbf{v}$ is the instantaneous velocity when the force is $\mathbf{F}$.

Power, like work and energy, is a scalar quantity. Its dimensions are $\left[\mathrm{ML}^{2} \mathrm{~T}^{-3}\right]$. In the SI, its unit is called a watt (W). The watt is $1 \mathrm{~J} \mathrm{~s}^{-1}$. The unit of power is named after James Watt, one of the innovators of the steam engine in the eighteenth century.

There is another unit of power, namely the horse-power (hp)

$$ 1 \mathrm{hp}=746 \mathrm{~W} $$

This unit is still used to describe the output of automobiles, motorbikes, etc.

We encounter the unit watt when we buy electrical goods such as bulbs, heaters and refrigerators. A 100 watt bulb which is on for 10 hours uses 1 kilowatt hour ( $\mathrm{kWh}$ ) of energy.

100 (watt) $\times 10$ (hour)

$=1000$ watt hour

$=1$ kilowatt hour $(\mathrm{kWh})$

$=10^{3}(\mathrm{~W}) \times 3600(\mathrm{~s})$

$=3.6 \times 10^{6} \mathrm{~J}$

Our electricity bills carry the energy consumption in units of $\mathrm{kWh}$. Note that $\mathrm{kWh}$ is a unit of energy and not of power.

5.11 COLLISIONS

In physics we study motion (change in position). At the same time, we try to discover physical quantities, which do not change in a physical process. The laws of momentum and energy conservation are typical examples. In this section we shall apply these laws to a commonly encountered phenomena, namely collisions. Several games such as billiards, marbles or carrom involve collisions. We shall study the collision of two masses in an idealised form.

Consider two masses $m_{1}$ and $m_{2}$. The particle $m_{l}$ is moving with speed $v_{1 i}$, the subscript ’ $i$ ’ implying initial. We can cosider $m_{2}$ to be at rest. No loss of generality is involved in making such a selection. In this situation the mass $m_{1}$ collides with the stationary mass $m_{2}$ and this is depicted in Fig. 5.10.

The masses $m_{1}$ and $m_{2}$ fly-off in different directions. We shall see that there are relationships, which connect the masses, the velocities and the angles.

5.11.1 Elastic and Inelastic Collisions

In all collisions the total linear momentum is conserved; the initial momentum of the system is equal to the final momentum of the system. One can argue this as follows. When two objects collide, the mutual impulsive forces acting over the collision time $\Delta t$ cause a change in their respective momenta :

$$ \begin{aligned} \Delta \mathbf{p_1}=\mathbf{F_{12}} \Delta t \end{aligned} $$

$$ \begin{aligned} & \Delta \mathbf{p_{2}}=\mathbf{F_{21}} \Delta t \end{aligned} $$

where $F_{12}$ is the force exerted on the first particle by the second particle. $F_{21}$ is likewise the force exerted on the second particle by the first particle. Now from Newton’s third law, $F_{12}=-F_{21}$. This implies

$$ \Delta p_1+\Delta p_2=0 $$

The above conclusion is true even though the forces vary in a complex fashion during the collision time $\Delta t$. Since the third law is true at every instant, the total impulse on the first object is equal and opposite to that on the second.

On the other hand, the total kinetic energy of the system is not necessarily conserved. The impact and deformation during collision may generate heat and sound. Part of the initial kinetic energy is transformed into other forms of energy. A useful way to visualise the deformation during collision is in terms of a ‘compressed spring’. If the ‘spring’ connecting the two masses regains its original shape without loss in energy, then the initial kinetic energy is equal to the final kinetic energy but the kinetic energy during the collision time $\Delta t$ is not constant. Such a collision is called an elastic collision. On the other hand the deformation may not be relieved and the two bodies could move together after the collision. A collision in which the two particles move together after the collision is called a completely inelastic collision. The intermediate case where the deformation is partly relieved and some of the initial kinetic energy is lost is more common and is appropriately called an inelastic collision.

5.11.2 Collisions in One Dimension

Consider first a completely inelastic collision in one dimension. Then, in Fig. 5.10,

$$ \begin{align*} & \theta_{1}=\theta_{2}=0 \\ & m_{1} v_{1 i}=\left(m_{1}+m_{2}\right) v_{f} \text { (momentum conservation) } \\ & v_{f}=\frac{m_{1}}{m_{1}+m_{2}} v_{1 i} \tag{5.22} \end{align*} $$

The loss in kinetic energy on collision is

$$ \begin{aligned} & \Delta K=\frac{1}{2} m_{1} v_{1 i}^{2}-\frac{1}{2}\left(m_{1}+m_{2}\right) v_{f}^{2} \\ & =\frac{1}{2} m_{1} v_{1 i}^{2}-\frac{1}{2} \frac{m_{1}^{2}}{m_{1}+m_{2}} v_{1 i}^{2} \quad \text { [using Eq. (5.22)] } \\ & =\frac{1}{2} m_{1} v_{1 i}^{2} 1-\frac{m_{1}}{m_{1}+m_{2}} \\ & =\frac{1}{2} \frac{m_{1} m_{2}}{m_{1}+m_{2}} v_{1 i}^{2} \end{aligned} $$

which is a positive quantity as expected.

Consider next an elastic collision. Using the above nomenclature with $\theta_{1}=\theta_{2}=0$, the momentum and kinetic energy conservation equations are

$$ \begin{align*} & m_{1} v_{1 i}=m_{1} v_{1 f}+m_{2} v_{2 f} \tag{5.23}\\ & m_{1} v_{1 i}^{2}=m_{1} v_{1 f}^{2}+m_{2} v_{2 f}^{2} \tag{5.24} \end{align*} $$

From Eqs. (5.23) and (5.24) it follows that,

$$ m_{1} v_{1 i}\left(v_{2 f}-v_{1 i}\right)=m_{1} v_{1 f}\left(v_{2 f}-v_{1 f}\right) $$

or, $\quad v_{2 f}\left(v_{1 i}-v_{1 f}\right)=v_{1 i}^{2}-v_{1 f}^{2}$

$$ \begin{aligned} =\left(v_{1 i}-v_{1 f}\right)\left(v_{1 i}+v_{1 f}\right) \end{aligned} $$

$$ \begin{aligned} \text{Hence,} \quad \quad &\therefore v_{2 f}=v_{1 i}+v_{1 f} \tag{5.25} \end{aligned} $$

Substituting this in Eq. (5.23), we obtain

$$ \begin{align*} v_{1 f} & =\frac{\left(m_{1}-m_{2}\right)}{m_{1}+m_{2}} v_{1 i} \tag{5.26}\\ \text { and } \quad v_{2 f} & =\frac{2 m_{1} v_{1 i}}{m_{1}+m_{2}} \tag{5.27} \end{align*} $$

Thus, the ‘unknowns’ {$V_{1f} \quad V_{2f}$} are obtained in terms of the ‘knowns’ {$ m_1, m_2, v_1 i $}. Special cases of our analysis are interesting.

Case I : If the two masses are equal

$$ \begin{aligned} & V_{1 f}=0 \\ & V_{2 f}=V_{1 i} \end{aligned} $$

The first mass comes to rest and pushes off the second mass with its initial speed on collision.

Case II : If one mass dominates, e.g. $m_{2} > > m_{1}$

$$ V_{1 f} \simeq-V_{1 i} \quad V_{2 f} \simeq 0 $$

The heavier mass is undisturbed while the lighter mass reverses its velocity.

5.11.3 Collisions in Two Dimensions

Fig. 5.10 also depicts the collision of a moving mass $m_{1}$ with the stationary mass $m_{2}$. Linear momentum is conserved in such a collision. Since momentum is a vector this implies three equations for the three directions ${x, y, z}$. Consider the plane determined by the final velocity directions of $m_{1}$ and $m_{2}$ and choose it to be the $x-y$ plane. The conservation of the $z$-component of the linear momentum implies that the entire collision is in the $x-y$ plane. The $x$ - and $y$-component equations are

$$ \begin{align*} & m_{1} v_{1 i}=m_{1} v_{1 f} \cos \theta_{1}+m_{2} v_{2 f} \cos \theta_{2} \tag{5.28}\\ & 0=m_{1} v_{1 f} \sin \theta_{1}-m_{2} v_{2 f} \sin \theta_{2} \tag{5.29} \end{align*} $$

One knows $\{m_{1}, m_{2}, v_{1 i}\}$ in most situations. There are thus four unknowns $\{v_{1 f}, v_{2 f}, \theta_{1}\}$ and $\{\theta_{2}\}$, and only two equations. If $\theta_{1}=\theta_{2}=0$, we regain Eq. (5.23) for one dimensional collision.

If, further the collision is elastic,

$$ \begin{equation*} \frac{1}{2} m_{1} v_{1 i}^{2}=\frac{1}{2} m_{1} v_{1 f}^{2}+\frac{1}{2} m_{2} v_{2 f}^{2} \tag{5.30} \end{equation*} $$

We obtain an additional equation. That still leaves us one equation short. At least one of the four unknowns, say $\theta_{1}$, must be made known for the problem to be solvable. For example, $\theta_{1}$ can be determined by moving a detector in an angular fashion from the $x$ to the $y$ axis. Given $\{ m_1, m_2, v_{1i}, \theta_1 \}$ we can determine $\{V_{1 f}, V_{2 f}, \theta_{2}\}$ from Eqs. (5.28)-(5.30).

Summary

1. The work-energy theorem states that the change in kinetic energy of a body is the work done by the net force on the body.

$$ K_{f}-K_{i}=W_{\text {net }} $$

2. A force is conservative if (i) work done by it on an object is path independent and depends only on the end points $\{x_{i}, x_{j}\}$, or (ii) the work done by the force is zero for an arbitrary closed path taken by the object such that it returns to its initial position.

3. For a conservative force in one dimension, we may define a potential energy function $V(x)$ such that

$$ \begin{aligned} & F(x)=-\frac{\mathrm{d} V(x)}{\mathrm{d} x} \\ \text{or} \quad \quad \quad & V_{i}-V_{f}=\int_{x_{i}}^{x_{f}} F(x) \mathrm{d} x \end{aligned} $$

4. The principle of conservation of mechanical energy states that the total mechanical energy of a body remains constant if the only forces that act on the body are conservative.

5. The gravitational potential energy of a particle of mass $m$ at a height $x$ about the earth’s surface is

$$ V(x)=m g x $$

where the variation of $g$ with height is ignored.

5. The elastic potential energy of a spring of force constant $k$ and extension $x$ is

$$ V(x)=\frac{1}{2} k x^{2} $$

7. The scalar or dot product of two vectors $\mathbf{A}$ and $\mathbf{B}$ is written as $\mathbf{A} \cdot \mathbf{B}$ and is a scalar quantity given by $: \mathbf{A} \cdot \mathbf{B}=A B \cos \theta$, where $\theta$ is the angle between $\mathbf{A}$ and $\mathbf{B}$. It can be positive, negative or zero depending upon the value of $\theta$. The scalar product of two vectors can be interpreted as the product of magnitude of one vector and component of the other vector along the first vector. For unit vectors :

$$ \hat{\mathbf{i}} \cdot \underline{\hat{\mathbf{i}}}=\hat{\mathbf{j}} \cdot \hat{\mathbf{j}}=\hat{\mathbf{k}} \cdot \hat{\mathbf{k}}=1 \text { and } \hat{\mathbf{i}} \cdot \hat{\mathbf{j}}=\hat{\mathbf{j}} \cdot \underline{\hat{\mathbf{k}}}=\hat{\mathbf{k}} \cdot \hat{\mathbf{i}}=0 $$

Scalar products obey the commutative and the distributive laws.

POINTS TO PONDER

1. The phrase ‘calculate the work done’ is incomplete. We should refer (or imply clearly by context) to the work done by a specific force or a group of forces on a given body over a certain displacement.

2. Work done is a scalar quantity. It can be positive or negative unlike mass and kinetic energy which are positive scalar quantities. The work done by the friction or viscous force on a moving body is negative.

3. For two bodies, the sum of the mutual forces exerted between them is zero from Newton’s Third Law,

$$ F_{12}+F_{21}=0 $$

But the sum of the work done by the two forces need not always cancel, i.e.

However, it may sometimes be true.

4. The work done by a force can be calculated sometimes even if the exact nature of the force is not known. This is clear from Example 5.2 where the WE theorem is used in such a situation.

5. The WE theorem is not independent of Newton’s Second Law. The WE theorem may be viewed as a scalar form of the Second Law. The principle of conservation of mechanical energy may be viewed as a consequence of the WE theorem for conservative forces.

6. The WE theorem holds in all inertial frames. It can also be extended to noninertial frames provided we include the pseudoforces in the calculation of the net force acting on the body under consideration.

7. The potential energy of a body subjected to a conservative force is always undetermined upto a constant. For example, the point where the potential energy is zero is a matter of choice. For the gravitational potential energy mgh, the zero of the potential energy is chosen to be the ground. For the spring potential energy $k x^{2} / 2$, the zero of the potential energy is the equilibrium position of the oscillating mass.

8. Every force encountered in mechanics does not have an associated potential energy. For example, work done by friction over a closed path is not zero and no potential energy can be associated with friction.

9. During a collision : (a) the total linear momentum is conserved at each instant of the collision ; (b) the kinetic energy conservation (even if the collision is elastic) applies after the collision is over and does not hold at every instant of the collision. In fact the two colliding objects are deformed and may be momentarily at rest with respect to each other.