Work, Energy And Power Notes - Class 11 - Science Physics | Kedovo | Kedovo
Chapter Notes
Work, Energy And Power
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Introduction
In everyday language, we use terms like 'work', 'energy', and 'power' quite freely. For instance, studying for an exam is considered 'work'. In physics, these terms have very precise meanings.
Work: In physics, work is only done when a force causes an object to move a certain distance. Pushing against a wall that doesn't move results in zero work, even though you might feel tired.
Energy: This is the capacity to do work. A person with high stamina has a lot of energy, and in physics, energy is directly related to the ability to perform work.
Power: This relates to how quickly work is done. A 'powerful' punch in boxing is one that is delivered very fast. This is close to the physics definition of power, which is the rate of doing work.
To understand these concepts mathematically, we first need to learn about the scalar product of vectors.
The Scalar Product
Many physical quantities like force and displacement are vectors, meaning they have both magnitude and direction. We can multiply vectors in two ways. One is the scalar product, and the other is the vector product (which will be covered in a later chapter).
The scalar product, also known as the dot product, of two vectors A and B gives a scalar (a number without direction) as the result. It is written as A⋅B and defined by the formula:
Scalar Product: A⋅B=ABcosθ
Here, A and B are the magnitudes of the vectors, and θ is the angle between them.
The scalar product can be interpreted in two ways:
The magnitude of vector A multiplied by the component of vector B that is along the direction of A (Bcosθ).
The magnitude of vector B multiplied by the component of vector A that is along the direction of B (Acosθ).
Properties of the Scalar Product:
Commutative Law: The order of multiplication doesn't matter.
A⋅B=B⋅A
Distributive Law: It can be distributed over vector addition.
A⋅(B+C)=A⋅B+A⋅C
Scalar Product with Unit Vectors:
For the standard unit vectors i^,j^,k^:
The dot product of a unit vector with itself is 1 (since θ=0∘ and cos0∘=1).
i^⋅i^=j^⋅j^=k^⋅k^=1
The dot product of two different unit vectors is 0 (since they are perpendicular, θ=90∘ and cos90∘=0).
i^⋅j^=j^⋅k^=k^⋅i^=0
Scalar Product in Component Form:
If we have two vectors in component form:
A=Axi^+Ayj^+Azk^B=Bxi^+Byj^+Bzk^
Their scalar product is:
A⋅B=AxBx+AyBy+AzBz
Note
If two vectors A and B are perpendicular to each other, their scalar product is zero: A⋅B=0.
Example
Find the angle between force F=(3i^+4j^−5k^) unit and displacement d=(5i^+4j^+3k^) unit. Also find the projection of F on d.
Given
Force vector, F=(3i^+4j^−5k^) unit
Displacement vector, d=(5i^+4j^+3k^) unit
To Find
The angle θ between F and d.
The projection of F on d.
Formula
F⋅d=Fxdx+Fydy+FzdzF⋅d=FdcosθF2=Fx2+Fy2+Fz2d2=dx2+dy2+dz2
Projection of F on d is Fcosθ=dF⋅d.
Solution
First, calculate the dot product F⋅d:
F⋅d=(3)(5)+(4)(4)+(−5)(3)=15+16−15=16 unit
Next, find the magnitudes of F and d:
F2=32+42+(−5)2=9+16+25=50 unitF=50 unitd2=52+42+32=25+16+9=50 unitd=50 unit
Now, find the angle θ using the dot product formula:
cosθ=FdF⋅d=505016=5016=0.32θ=cos−1(0.32)
The projection of F on d is the component of F along d, which is Fcosθ.
Fcosθ=dF⋅d=5016
Final Answer
The angle between the force and displacement is θ=cos−1(0.32). The projection of F on d is 5016 unit.
Notions of Work and Kinetic Energy: The Work-Energy Theorem
Let's start with a familiar equation of motion for an object moving in a straight line with constant acceleration:
v2−u2=2as
where u is initial speed, v is final speed, a is acceleration, and s is distance.
If we multiply both sides by 2m (where m is the mass of the object), we get:
21mv2−21mu2=mas
From Newton's Second Law, we know that force F=ma. So, we can replace mas with Fs:
21mv2−21mu2=Fs
This equation gives us the foundation for defining two important concepts:
Kinetic Energy (K): The quantity 21mv2 is called the kinetic energy of the object. It's the energy an object possesses due to its motion.
Work (W): The quantity on the right side, Fs, is the product of the force and the displacement. This is defined as the work done by the force on the object. In vector form, this is W=F⋅d.
With these definitions, the equation becomes:
Kf−Ki=W
where Ki is the initial kinetic energy and Kf is the final kinetic energy.
This relationship is known as the Work-Energy Theorem. It states that the change in the kinetic energy of an object is equal to the net work done on it by all forces.
Example
A raindrop of mass 1.00 g falls from a height of 1.00 km. It hits the ground with a speed of 50.0 m s−1. (a) What is the work done by the gravitational force? (b) What is the work done by the unknown resistive force? (Assume g=10 m/s2)
Given
Mass of raindrop, m=1.00 g=10−3 kg
Height, h=1.00 km=103 m
Initial speed, u=0 (assumed at rest)
Final speed, v=50.0 m s−1
Acceleration due to gravity, g=10 m s−2
To Find
(a) Work done by gravity, Wg
(b) Work done by resistive force, Wr
Formula
Change in kinetic energy: ΔK=21mv2−21mu2
Work done by gravity: Wg=mgh
Work-Energy Theorem: ΔK=Wg+Wr
Solution
(a) Calculate the work done by gravity
The change in kinetic energy of the drop is:
ΔK=21mv2−0=21×10−3 kg×(50 m s−1)2ΔK=21×10−3×2500=1.25 J
The work done by the gravitational force is:
Wg=mgh=(10−3 kg)×(10 m s−2)×(103 m)Wg=10.0 J
Answer for part (a) = 10.0 J
(b) Calculate the work done by the resistive force
According to the work-energy theorem, the total work done by all forces (gravity and resistance) equals the change in kinetic energy.
ΔK=Wg+Wr
We can rearrange this to find Wr:
Wr=ΔK−WgWr=1.25 J−10.0 J=−8.75 J
The work done by the resistive force is negative because it acts in the opposite direction to the raindrop's motion.
Answer for part (b) = −8.75 J
Work
Work is done when a force causes a displacement. For a constant force F acting on an object that undergoes a displacement d, the work done is defined as the product of the magnitude of the displacement and the component of the force in the direction of the displacement.
Mathematically, this is expressed using the scalar product:
W=(Fcosθ)d=F⋅d
Here, θ is the angle between the force vector and the displacement vector.
Conditions for Zero Work:
No work is done if:
Displacement is zero (d=0): A weightlifter holding a heavy weight steady on his shoulders does no work on the weight, no matter how much force he applies.
Force is zero (F=0): An object sliding on a frictionless horizontal surface may move a large distance, but with no horizontal force acting on it, no work is done.
Force and displacement are perpendicular (θ=90∘): Since cos90∘=0, the work done is zero. For example, the Earth's gravitational force does no work on the Moon in a perfectly circular orbit, because the force is always perpendicular to the Moon's instantaneous displacement.
Positive and Negative Work:
Positive Work: If the angle θ is between 0∘ and 90∘, cosθ is positive, and the work done is positive. This means the force helps the motion.
Negative Work: If the angle θ is between 90∘ and 180∘, cosθ is negative, and the work done is negative. This means the force opposes the motion. Frictional force always does negative work.
The SI unit for work is the joule (J). The dimensions of work are [ML2T−2].
Example
A cyclist comes to a skidding stop in 10 m. During this process, the force on the cycle due to the road is 200 N and is directly opposed to the motion. (a) How much work does the road do on the cycle? (b) How much work does the cycle do on the road?
Given
Displacement, d=10 m
Stopping force, F=200 N
Angle between force and displacement, θ=180∘ (since the force opposes motion)
To Find
(a) Work done by the road on the cycle, Wr
(b) Work done by the cycle on the road, Wc
Formula
W=Fdcosθ
Solution
(a) Work done by the road on the cycle
The force is from the road, and the displacement is that of the cycle.
Wr=(200 N)×(10 m)×cos(180∘)
Since cos(180∘)=−1:
Wr=200×10×(−1)=−2000 J
This negative work is what brings the cycle to a stop.
Answer for part (a) = −2000 J
(b) Work done by the cycle on the road
According to Newton's Third Law, the cycle exerts an equal and opposite force of 200 N on the road. However, the road does not move. Its displacement is zero.
Wc=(200 N)×(0 m)×cosθ=0 J
Answer for part (b) = 0 J
Kinetic Energy
As defined earlier, the kinetic energy of an object of mass m moving with velocity v is:
K=21mv⋅v=21mv2
Kinetic energy is a scalar quantity and is a measure of the work an object can do because of its motion. For example, the kinetic energy of flowing water is used to generate electricity, and the kinetic energy of wind is used by sailing ships.
Example
In a ballistics demonstration, a police officer fires a bullet of mass 50.0 g with speed 200 m s−1 on soft plywood of thickness 2.00 cm. The bullet emerges with only 10% of its initial kinetic energy. What is the emergent speed of the bullet?
Given
Mass of bullet, m=50.0 g=0.05 kg
Initial speed, vi=200 m s−1
Final kinetic energy, Kf=10% of initial kinetic energy, Ki
To Find
Emergent speed of the bullet, vf
Formula
K=21mv2
Solution
First, calculate the initial kinetic energy (Ki):
Ki=21mvi2=21×(0.05 kg)×(200 m s−1)2Ki=21×0.05×40000=1000 J
The final kinetic energy (Kf) is 10% of this value:
Kf=0.10×Ki=0.10×1000 J=100 J
Now, use the kinetic energy formula to find the final speed (vf):
Kf=21mvf2100 J=21×(0.05 kg)×vf2vf2=0.05 kg2×100 J=0.05200=4000vf=4000≈63.2 m s−1
Final Answer
The emergent speed of the bullet is approximately 63.2 m s−1.
Work Done by a Variable Force
In most real-world situations, forces are not constant. For example, the force of a spring changes as it is stretched. To calculate the work done by a variable force, we can use a graphical method or calculus.
Imagine a force F(x) that changes with position x. We can divide the total displacement into tiny segments, Δx. Over each tiny segment, the force is almost constant. The small amount of work done, ΔW, is:
ΔW=F(x)Δx
This corresponds to the area of a small rectangle on a Force vs. Displacement graph.
To find the total work done from an initial position xi to a final position xf, we sum the areas of all these small rectangles:
W≅∑xixfF(x)Δx
In the limit as Δx approaches zero, this sum becomes a definite integral, which gives the exact area under the curve.
Work done by a variable force:
W=∫xixfF(x)dx
Example
A woman pushes a trunk on a railway platform. She applies a constant force of 100 N over 10 m. Then, she gets tired and her applied force reduces linearly with distance to 50 N over the next 10 m. The total distance moved is 20 m. The frictional force is a constant 50 N. Plot the forces versus displacement and calculate the work done by both forces over 20 m.
Given
Applied force F: 100 N for 0≤x≤10 m.
Applied force F: Reduces linearly from 100 N to 50 N for 10<x≤20 m.
Frictional force f: -50 N (constant, opposes motion).
Total displacement: 20 m.
To Find
Work done by the woman, WF.
Work done by the frictional force, Wf.
Formula
Work is the area under the Force-Displacement graph.
Area of rectangle = length × width
Area of trapezium = 21×(sum of parallel sides)× height
Solution
The work done is the area under the F-x graph.
Work done by the woman (WF)
The area can be split into a rectangle (from 0 to 10 m) and a trapezium (from 10 to 20 m).
Area of rectangle (ABCD) = 100 N×10 m=1000 J
Area of trapezium (CEID) = 21(100 N+50 N)×(20−10) m=21×150×10=750 J
Total work done by the woman:
WF=1000 J+750 J=1750 J
Work done by the frictional force (Wf)
The frictional force is constant at -50 N over the entire 20 m displacement. The area is a rectangle below the x-axis.
Area of rectangle (AGHI) = (−50 N)×20 m=−1000 J
Final Answer
The work done by the woman is 1750 J. The work done by the frictional force is −1000 J.
The Work-Energy Theorem for a Variable Force
The work-energy theorem (Kf−Ki=W) also holds true for variable forces. We can prove this using calculus.
The rate of change of kinetic energy with time is:
dtdK=dtd(21mv2)
Using the chain rule, this becomes:
dtdK=mdtdvv
We know that acceleration a=dtdv and from Newton's Second Law, F=ma. So, mdtdv=F.
dtdK=Fv
Since velocity v=dtdx, we can write:
dtdK=Fdtdx
Multiplying by dt, we get:
dK=Fdx
To find the total change in kinetic energy over a displacement from xi to xf, we integrate both sides:
∫KiKfdK=∫xixfFdx
The left side is Kf−Ki, and the right side is the definition of work, W.
Kf−Ki=W
This proves the work-energy theorem for a variable force in one dimension.
Note
The work-energy theorem is a scalar equation and doesn't contain information about the direction of motion or the time taken, unlike Newton's second law, which is a vector equation that applies at every instant.
Example
A block of mass m=1 kg, moving on a horizontal surface with speed vi=2 m s−1 enters a rough patch from x=0.10 m to x=2.01 m. The retarding force in this range is Fr=x−k, where k=0.5 J. What is the final kinetic energy and speed vf of the block as it crosses this patch?
Given
Mass, m=1 kg
Initial speed, vi=2 m s−1
Retarding force, Fr=x−k for 0.1<x<2.01 m
Constant, k=0.5 J
To Find
Final kinetic energy, Kf
Final speed, vf
Formula
Work-Energy Theorem: Kf−Ki=W=∫xixfF(x)dx
Initial kinetic energy: Ki=21mvi2
Solution
First, calculate the initial kinetic energy:
Ki=21(1 kg)(2 m s−1)2=2 J
Now, use the work-energy theorem. The work done by the retarding force is:
W=∫0.12.01x−kdx=−k[ln(x)]0.12.01W=−k(ln(2.01)−ln(0.1))=−kln(0.12.01)=−0.5ln(20.1)
Given ln(20.1)≈3.00, the work done is W≈−0.5×3.00=−1.5 J.
(Using the value from the source, 0.5ln(20.1)=1.5)
So, W=−1.5 J.
Now apply the work-energy theorem to find Kf:
Kf−Ki=WKf=Ki+W=2 J−1.5 J=0.5 J
Finally, calculate the final speed vf:
Kf=21mvf20.5 J=21(1 kg)vf2vf2=1⟹vf=1 m s−1
Final Answer
The final kinetic energy is 0.5 J and the final speed is 1 m s−1.
The Concept of Potential Energy
Potential energy is 'stored' energy that an object has due to its position or configuration. For example, a stretched bowstring has potential energy, which is converted into the kinetic energy of the arrow when released.
This concept applies only to a special class of forces called conservative forces. For these forces, the work done against them gets stored as potential energy.
Gravitational Potential Energy:
Consider lifting a ball of mass m to a height h. The work you do against the gravitational force (mg) is mgh. This work is stored as gravitational potential energy, denoted by V(h).
V(h)=mgh
If you release the ball, this stored potential energy is converted back into kinetic energy as it falls.
Conservative Forces and Potential Energy:
A force F(x) is conservative if it can be expressed as the negative derivative of a potential energy function V(x):
F(x)=−dxdV
This relationship implies that the work done by a conservative force only depends on the initial and final positions, not on the path taken between them.
W=∫xixfF(x)dx=−∫ViVfdV=Vi−Vf
Forces like gravity and the spring force are conservative. Friction is a non-conservative force because the work done by friction depends on the length of the path taken.
The Conservation of Mechanical Energy
For a system where only conservative forces are doing work, the total mechanical energy is conserved (remains constant).
The total mechanical energy (E) is the sum of the kinetic energy (K) and the potential energy (V) of the system.
E=K+V
Let's see why it's conserved. From the work-energy theorem, the change in kinetic energy is:
ΔK=W
For a conservative force, the work done is equal to the negative change in potential energy:
W=−ΔV
Combining these, we get:
ΔK=−ΔV⟹ΔK+ΔV=0
This can be written as:
Δ(K+V)=0
This equation means that the change in the total mechanical energy (K+V) is zero. Therefore, the total mechanical energy is constant.
Principle of Conservation of Mechanical Energy:
Ki+Vi=Kf+Vf
The total mechanical energy of a system remains constant if the forces doing work on it are conservative.
Example: A Freely Falling Body
Consider a ball of mass m dropped from a height H. Let's define the potential energy to be zero at the ground level (V=0 at h=0).
At height H (top): The ball is at rest, so K=0. The potential energy is V=mgH.
Total Energy EH=0+mgH=mgH.
At height h (mid-fall): The potential energy is V=mgh. The kinetic energy is K=21mvh2.
Total Energy Eh=21mvh2+mgh.
At height 0 (ground): The potential energy is V=0. The kinetic energy is K=21mvf2.
Total Energy E0=21mvf2+0=21mvf2.
Since gravity is a conservative force, mechanical energy is conserved: EH=Eh=E0.
mgH=21mvh2+mgh=21mvf2
From this, we can find the speed at any point. For example, equating the energy at the top and the bottom gives mgH=21mvf2, which simplifies to vf=2gH.
Example
A bob of mass m is suspended by a light string of length L. It is given a horizontal velocity vo at the lowest point A, just enough to complete a semi-circular path and reach the topmost point C, where the string becomes slack. Find (i) vo; (ii) the speeds at points B (horizontal position) and C; (iii) the ratio of kinetic energies at B and C.
Given
Mass of bob = m
Length of string = L
Potential energy at lowest point A is zero.
Tension at highest point C is zero (TC=0).
To Find
(i) Initial velocity, vo
(ii) Speeds at B and C, vB and vC
(iii) Ratio of kinetic energies, KB/KC
Formula
Conservation of Mechanical Energy: EA=EB=EC
Newton's Second Law for circular motion: Fnet=Lmv2
Solution
The only force doing work is gravity (conservative), as the tension is always perpendicular to the displacement. So, mechanical energy is conserved. Let's set the potential energy V=0 at point A.
(i) Find the initial velocity vo
At point A (lowest): VA=0, KA=21mvo2. Total energy E=21mvo2.
At point C (highest): The height is 2L, so VC=mg(2L). The kinetic energy is KC=21mvC2.
Total energy E=21mvC2+2mgL.
At point C, the string goes slack (TC=0). The only force providing the centripetal acceleration is gravity.
mg=LmvC2⟹vC2=gL
Substitute this into the energy equation for C:
E=21m(gL)+2mgL=25mgL
By conservation of energy, EA=EC:
21mvo2=25mgL⟹vo2=5gLvo=5gL
Answer for part (i) = 5gL
(ii) Find the speeds at B and C
From the calculation above, the speed at C is:
vC=gL
At point B (horizontal): The height is L, so VB=mgL. The kinetic energy is KB=21mvB2.
Total energy EB=21mvB2+mgL.
By conservation of energy, EA=EB:
21mvo2=21mvB2+mgL
Substitute vo2=5gL:
21m(5gL)=21mvB2+mgL25mgL−mgL=21mvB2⟹23mgL=21mvB2vB2=3gL⟹vB=3gL
Answer for part (ii) = vB=3gL and vC=gL
(iii) Find the ratio of kinetic energies
KB=21mvB2=21m(3gL)=23mgLKC=21mvC2=21m(gL)=21mgL
The ratio is:
KCKB=21mgL23mgL=3
Answer for part (iii) = 3:1
The Potential Energy of a Spring
The force exerted by an ideal spring is a variable, conservative force. It follows Hooke's Law:
Fs=−kx
where k is the spring constant (a measure of the spring's stiffness, in N m−1), and x is the displacement from the equilibrium position. The negative sign indicates that the spring force always acts to restore the spring to its equilibrium position.
Since the spring force is conservative, we can define a potential energy for it. The work done by the spring force when it is stretched from 0 to a displacement xm is:
Ws=∫0xmFsdx=∫0xm−kxdx=−21kxm2
The potential energy stored in the spring is the negative of the work done by the spring force. We define the potential energy to be zero at the equilibrium position (x=0).
Elastic Potential Energy:
V(x)=21kx2
For a mass attached to a spring, the total mechanical energy is conserved (if there is no friction):
E=K+V=21mv2+21kx2=constant
When the spring is at its maximum stretch (x=xm), the velocity is zero, so all the energy is potential: E=21kxm2.
When the mass passes through the equilibrium position (x=0), the potential energy is zero, and the speed is maximum (v=vm). All the energy is kinetic: E=21mvm2.
Therefore, 21mvm2=21kxm2.
Example
To simulate car accidents, a car of mass 1000 kg moving at 18.0 km/h collides with a spring of spring constant 6.25×103 N m−1. What is the maximum compression of the spring?
Given
Mass of car, m=1000 kg
Speed of car, v=18.0 km/h=5 m s−1
Spring constant, k=6.25×103 N m−1
To Find
Maximum compression of the spring, xm
Formula
Conservation of Mechanical Energy: Ki+Vi=Kf+Vf
Kinetic Energy: K=21mv2
Spring Potential Energy: V=21kx2
Solution
At the moment of maximum compression, the car comes to a momentary stop (vf=0), so its kinetic energy is zero. All of its initial kinetic energy has been converted into the potential energy of the spring.
Initial state: Car is moving, spring is uncompressed.
Ki=21mv2, Vi=0
Final state: Car is stopped, spring is maximally compressed.
Kf=0, Vf=21kxm2
By conservation of energy:
Ki=Vf21mv2=21kxm2
Calculate the initial kinetic energy:
Ki=21×(1000 kg)×(5 m s−1)2=21×1000×25=12500 J=1.25×104 J
Now set this equal to the final potential energy:
1.25×104 J=21(6.25×103 N m−1)xm2xm2=6.25×1032×1.25×104=0.625×1042.5×104=4xm=4=2.00 m
Final Answer
The maximum compression of the spring is 2.00 m.
Presence of Non-Conservative Forces
If a non-conservative force like friction is present, mechanical energy is not conserved. The work done by the non-conservative force (Wnc) equals the change in the total mechanical energy of the system.
ΔE=Ef−Ei=Wnc
Example
Consider the previous example, but now with a coefficient of friction μ=0.5. Calculate the maximum compression of the spring. (Take g=10.0 m s−2)
Given
Mass of car, m=1000 kg
Initial speed, v=5 m s−1
Spring constant, k=6.25×103 N m−1
Coefficient of friction, μ=0.5
To Find
Maximum compression, xm
Formula
Work-Energy Theorem: ΔK=Wnet
Work done by spring: Ws=−21kxm2
Work done by friction: Wf=−f×xm=−μmgxm
Solution
The change in kinetic energy is from its initial value to zero.
ΔK=Kf−Ki=0−21mv2=−1.25×104 J
The net work done is the sum of the work done by the spring force and the frictional force.
Wnet=Ws+Wf=−21kxm2−μmgxm
According to the work-energy theorem, ΔK=Wnet:
−21mv2=−21kxm2−μmgxm
Multiplying by -1 gives:
21mv2=21kxm2+μmgxm
Substitute the values:
1.25×104=21(6.25×103)xm2+(0.5)(1000)(10)xm12500=3125xm2+5000xm
Divide by 125:
100=25xm2+40xm
Rearrange into a quadratic equation:
25xm2+40xm−100=0
Using the quadratic formula x=2a−b±b2−4ac:
xm=2(25)−40+402−4(25)(−100)xm=50−40+1600+10000=50−40+11600≈50−40+107.7=5067.7≈1.35 m
(We take the positive root since compression must be a positive distance).
Final Answer
The maximum compression of the spring is 1.35 m.
Power
Power is the rate at which work is done or energy is transferred.
Average Power (Pav) is the total work done divided by the total time taken.
Pav=tW
Instantaneous Power (P) is the rate of doing work at a specific moment.
P=dtdW
Since work dW=F⋅dr, we can also express instantaneous power as:
P=F⋅dtdr=F⋅v
where v is the instantaneous velocity.
Power is a scalar quantity. Its SI unit is the watt (W), where 1 W=1 J s−1. Another common unit is horsepower (hp), where 1 hp=746 W.
Note
The kilowatt-hour (kWh) is a unit of energy, not power. It is the energy consumed when 1 kilowatt of power is used for 1 hour.
1 kWh=(1000 W)×(3600 s)=3.6×106 J.
Example
An elevator with a maximum load of 1800 kg (elevator + passengers) moves up at a constant speed of 2 m s−1. The frictional force opposing the motion is 4000 N. Determine the minimum power delivered by the motor in watts and in horsepower.
Given
Total mass, m=1800 kg
Constant speed, v=2 m s−1
Frictional force, Ff=4000 N
Acceleration due to gravity, g≈10 m s−2
To Find
Minimum power delivered by the motor, P.
Formula
P=F⋅v
Solution
To move the elevator up at a constant speed, the motor must provide an upward force F that exactly balances the downward forces. The downward forces are gravity (mg) and friction (Ff).
Fdown=mg+Ff=(1800 kg×10 m s−2)+4000 NFdown=18000 N+4000 N=22000 N
The motor must supply an upward force F=22000 N.
Since the force and velocity are in the same direction, the power delivered is:
P=F×v=22000 N×2 m s−1=44000 W
To convert this to horsepower:
Php=746 W/hp44000 W≈59 hp
Final Answer
The minimum power delivered by the motor is 44000 W or approximately 59 hp.
Collisions
A collision is an event where two or more bodies exert forces on each other for a relatively short time. In any collision, one fundamental principle always holds true: the conservation of total linear momentum.
Conservation of Linear Momentum in Collisions:
When two objects collide, they exert equal and opposite forces on each other (Newton's Third Law, F12=−F21). The change in momentum (impulse) for each object is:
Δp1=F12ΔtΔp2=F21Δt
Since the forces are equal and opposite, the changes in momentum are also equal and opposite:
Δp1=−Δp2⟹Δp1+Δp2=0
This means the total change in momentum of the system is zero, so the total momentum before the collision is equal to the total momentum after the collision.
Elastic and Inelastic Collisions
While momentum is always conserved, kinetic energy may not be.
Elastic Collision: A collision where the total kinetic energy of the system is also conserved. The objects bounce off each other without any loss of kinetic energy (though it might be temporarily converted to potential energy during the impact).
Inelastic Collision: A collision where some of the kinetic energy is lost, usually converted into other forms like heat, sound, or deformation of the objects.
Completely Inelastic Collision: An inelastic collision where the objects stick together and move with a common final velocity after the impact. This is where the maximum possible kinetic energy is lost.
Collisions in One Dimension
Let's consider a mass m1 with initial velocity v1i hitting a stationary mass m2 (v2i=0) in a head-on collision.
Completely Inelastic Collision:
The two masses stick together and move with a final velocity vf.
Loss in Kinetic Energy:
ΔK=Ki−Kf=21m1v1i2−21(m1+m2)vf2ΔK=21m1+m2m1m2v1i2
Since masses and velocity squared are positive, ΔK is always positive, meaning kinetic energy is always lost.
Elastic Collision:
Both momentum and kinetic energy are conserved.
Momentum Conservation: m1v1i=m1v1f+m2v2f
Kinetic Energy Conservation: 21m1v1i2=21m1v1f2+21m2v2f2
Solving these two equations gives the final velocities:
v1f=m1+m2m1−m2v1iv2f=m1+m22m1v1i
Special Cases for Elastic Collisions:
Case I: Equal Masses (m1=m2):
v1f=0v2f=v1i
The first mass stops completely, and the second mass moves off with the initial velocity of the first. This is often seen in billiards.
Case II: A heavy target (m2≫m1):
v1f≈−v1iv2f≈0
The light object bounces back with nearly its original speed, and the heavy object barely moves. Think of a ball bouncing off a wall.
Example
In a nuclear reactor, a fast neutron (m1) must be slowed down by colliding with a moderator nucleus (m2), like deuterium or carbon. Show that a neutron can lose most of its kinetic energy in an elastic collision with a light nucleus.
Given
Elastic collision between a neutron (m1) and a moderator nucleus (m2).
To Find
The fractional kinetic energy lost by the neutron.
Formula
Initial KE of neutron: K1i=21m1v1i2
Final KE of neutron: K1f=21m1v1f2
Final velocity of neutron: v1f=(m1+m2m1−m2)v1i
Solution
The fractional kinetic energy remaining for the neutron is f1=K1f/K1i.
f1=21m1v1i221m1v1f2=v1i2v1f2
Substitute the expression for v1f:
f1=(v1im1+m2m1−m2v1i)2=(m1+m2m1−m2)2
The fractional energy transferred to the moderator nucleus is f2=1−f1.
f2=1−(m1+m2m1−m2)2=(m1+m2)2(m1+m2)2−(m1−m2)2=(m1+m2)24m1m2
Let's analyze for deuterium, where m2≈2m1.
f1=(m1+2m1m1−2m1)2=(3m1−m1)2=91
The fraction of energy transferred is f2=1−f1=1−1/9=8/9.
Final Answer
When a neutron collides with a deuterium nucleus, it transfers 8/9 (almost 90%) of its kinetic energy, effectively slowing it down. This is why light nuclei are used as moderators.
Collisions in Two Dimensions
When objects collide at an angle (not head-on), the collision is two-dimensional. We must apply the conservation of momentum in both the x and y directions.
Consider a mass m1 with initial velocity v1i along the x-axis hitting a stationary mass m2. After the collision, m1 moves off at an angle θ1 with velocity v1f, and m2 moves off at an angle θ2 with velocity v2f.
We have two equations but four unknowns (v1f,v2f,θ1,θ2). If the collision is elastic, we have a third equation:
Kinetic Energy Conservation:
21m1v1i2=21m1v1f2+21m2v2f2
Even with three equations, we still have four unknowns. To solve the problem, we must know at least one of the final parameters, such as one of the scattering angles.
Example
Two billiard balls of equal mass (m1=m2) collide. The first ball (cue) is moving, and the second ball (target) is at rest. The player wants to sink the target ball in a pocket at an angle θ2=37∘. Assuming the collision is elastic, find the angle θ1 at which the cue ball moves.
Given
Equal masses, m1=m2=m
Elastic collision
Initial velocity of target, v2i=0
Final angle of target, θ2=37∘
To Find
Final angle of cue ball, θ1
Formula
Vector momentum conservation: v1i=v1f+v2f
Kinetic energy conservation: v1i2=v1f2+v2f2
Solution
From vector momentum conservation, we can square the equation using the dot product:
v1i⋅v1i=(v1f+v2f)⋅(v1f+v2f)v1i2=v1f⋅v1f+v2f⋅v2f+2v1f⋅v2fv1i2=v1f2+v2f2+2v1fv2fcos(θ1+θ2)
The angle between the final velocity vectors is θ1+θ2.
From kinetic energy conservation for equal masses:
v1i2=v1f2+v2f2
Comparing the two expressions for v1i2, we see that the extra term in the momentum equation must be zero:
2v1fv2fcos(θ1+θ2)=0
This implies that cos(θ1+θ2)=0.
For the cosine to be zero, the angle must be 90∘.
θ1+θ2=90∘
Substitute the given value for θ2:
θ1+37∘=90∘θ1=90∘−37∘=53∘
Final Answer
The cue ball moves off at an angle of 53∘. This shows that in a glancing elastic collision between two equal masses (with one initially at rest), the two masses will move off at right angles to each other.
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