6/25/2018 · 6/25/2018 4 example two boxes with masses 25 kg and 35 kg are placed on a smooth...
TRANSCRIPT
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Topic B: Momentum
CONTENT
1. Newton’s laws of motion
2. Equivalent forms of the equation of motion
2.1 Force, impulse and energy
2.2 Derivation of the equations of motion for particles
2.3 Examples
3. Conservation of momentum
3.1 Momentum in collisions
3.2 Restitution
3.3 Oblique collisions
4. Friction
4.1 Types of friction
4.2 Coefficient of friction
4.3 Object on a plane
5. Systems of particles and finite objects
5.1 Dynamics of a system
5.2 The centre of mass
5.3 Important properties of the centre of mass
5.4 Finding the centre of mass
5.5 Some useful centres of mass
Philosophiae Naturalis Principia Mathematica
Lex I: Corpus omne perseverare in statu suo quiescendi vel movendi
uniformiter in directum, nisi quatenus a viribus impressis cogitur statum
illum mutare.
Lex II: Mutationem motus proportionalem esse vi motrici impressae, et
fieri secundum lineam rectam qua vis illa imprimitur.
Lex III: Actioni contrariam semper et æqualem esse reactionem: sive
corporum duorum actiones in se mutuo semper esse æquales et in partes
contrarias dirigi.
Every body perseveres in its state of rest, or of uniform motion in a right line,
unless it is compelled to change that state by forces impressed thereon.
The alteration of motion is ever proportional to the motive force impressed; and is
made in the direction of the right line in which that force is impressed.
To every action there is always opposed an equal reaction: or the mutual actions
of two bodies upon each other are always equal, and directed to contrary parts.
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NEWTON’S LAWS OF MOTION
Law 1. Every particle continues in a state of rest or
uniform motion in a straight line unless
acted on by a resultant external force.
Law 2. When acted upon by an unbalanced force F
a particle of mass 𝑚 accelerates at a rate a
such that F = 𝑚a.
Law 3. The forces of action and reaction between
interacting particles are equal in magnitude,
opposite in direction and collinear.
NEWTON’S LAWS OF MOTION
• Strictly apply only to particles
‒ apply to finite objects by summation
• Law 1 requires the concept of inertial frames
‒ accelerating (e.g. rotating) reference frames yield additional apparent forces
• Law 3 (“equal and opposite reactions”) - use with care!
‒ e.g. magnetic forces between non-parallel current-carrying wires
‒ a more general version is “total momentum is conserved”
I I
F F(=BIL)
I
F
I
F
u
In inertial frame In rotating frame
FORMS OF THE EQUATION OF MOTION
Force-momentum:
force = rate of change of momentum
Impulse (force × time):
impulse = change of momentum
Energy (force × distance):
work done = change of kinetic energy
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FORMS OF THE EQUATION OF MOTION
force = mass acceleration
force = rate of change of momentum
Rate form:
Impulse form:
impulse = change of momentum
Energy form:
work done = change of kinetic energy
F = 𝑚a
F =d(𝑚v)
d𝑡
නF d𝑡 = (𝑚v)𝑒𝑛𝑑 − (𝑚v)𝑠𝑡𝑎𝑟𝑡
නF • dx = (1
2𝑚𝑣2)𝑒𝑛𝑑 − (
1
2𝑚𝑣2)𝑠𝑡𝑎𝑟𝑡
WORK-ENERGY
force = mass × acceleration
work done = change of kinetic energy
F = 𝑚dv
d𝑡
නF • dx = න𝑚dv
d𝑡• dx
= න𝑚dv
d𝑡• vd𝑡
= න 12𝑚
d
d𝑡v • v d𝑡
= නd
d𝑡(12𝑚𝑣
2) d𝑡
= 12𝑚𝑣
2𝑠𝑡𝑎𝑟𝑡
𝑒𝑛𝑑
නF • dx = 12𝑚𝑣
2𝑒𝑛𝑑
− 12𝑚𝑣
2𝑠𝑡𝑎𝑟𝑡
ADVANTAGES OF WORK-ENERGY FORM
work done = change of kinetic energy
● Scalar – not vector – equation
● Just “start” and “end” – no need for intermediate values
● Gives velocities without having to integrate acceleration
● Most forces depend on position, not time
● Some “work” conveniently written in terms of potential energy
නF • dx = 12𝑚𝑣2
𝑒𝑛𝑑− 1
2𝑚𝑣2
𝑠𝑡𝑎𝑟𝑡
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EXAMPLE
Two boxes with masses 25 kg and 35 kg are placed on a
smooth frictionless surface. The boxes are in contact and
a force of 30 N pushes horizontally on the smaller box.
What is the force that the smaller box exerts on the
larger box?
25 kg35 kg30 N
EXAMPLE
Masses are connected by light, inelastic cables passing round
light, smooth pulleys in different configurations, as shown below.
Find the direction and magnitude of the acceleration of each
mass, and the tension in each cable, for each configuration.
(Give your answers in kg-m-s units, as multiples of 𝑔.)
20kg
30kg
30kg
20kg
(a) (b)
CONSERVATION OF MOMENTUM
Corollary (or more modern version) of Newton’s Third Law
When two bodies A and B collide:
force exerted by A on B is equal and opposite to the force
exerted by B on A
change in momentum of B equal and opposite to change in
momentum of A
total momentum (A + B) conserved.
A
B
Before After
uB
uA
vB
vA
𝑚𝐴u𝐴 +𝑚𝐵u𝐵
total momentum before
= 𝑚𝐴v𝐴 +𝑚𝐵v𝐵
total momentum after
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EXAMPLE
A vehicle A of mass 500 kg travelling at 30 m s–1 collides with a
vehicle B of mass 900 kg travelling at 21 m s–1 along the same
line. After the collision the vehicles remain stuck together for a
short distance.
What is the speed and direction of the combined assembly:
(a) if the vehicles are originally travelling in the same direction?
(b) if the vehicles are originally travelling in opposite directions?
RESTITUTION
When objects collide, they compress, and kinetic
energy is replaced by elastic potential energy. A B
When they separate, kinetic energy is recovered.
Internal friction leads to mechanical energy being lost (as heat).
Model: coefficient of restitution, e
In general (if no external forces act):
Perfectly elastic collision (all kinetic energy recovered):
Perfectly inelastic collision (objects stick together):
0 ≤ 𝑒 ≤ 1
𝑒 = 1
𝑒 = 0
𝑒 =relative velocity of separation
relative velocity of approach
RESTITUTION
Before
AftervA
A B
vB
uA uB
Total momentum:
Restitution:
𝑚𝐴𝑢𝐴 +𝑚𝐵𝑢𝐵 = 𝑚𝐴𝑣𝐴 +𝑚𝐵𝑣𝐵
𝑣𝐵 − 𝑣𝐴 = 𝑒 𝑢𝐴 − 𝑢𝐵
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EXAMPLE
A ball of mass 0.6 kg and speed 12 m s–1 collides with
a second ball of mass 0.2 kg moving in the opposite
direction with speed 18 m s–1.
Assuming that all motion takes place along a straight
line, what is the outcome of the collision if the
coefficient of restitution e is:
(a) 0.5
(b) 0.8
OBLIQUE COLLISIONS
• Apply restitution perpendicular to the surface of contact:
Before Afterx
BAA B
• Conserve total momentum in any direction, including 𝑥:
• Conserve individual momentum components (and hence
velocity components) parallel to contact surfaces
𝑣𝐵𝑥 − 𝑣𝐴𝑥 = 𝑒 𝑢𝐴𝑥 − 𝑢𝐵𝑥
𝑚𝐴𝑢𝐴𝑥 +𝑚𝐵𝑢𝐵𝑥 = 𝑚𝐴𝑣𝐴𝑥 +𝑚𝐵𝑣𝐵𝑥
ቅ𝑣𝑦 = 𝑢𝑦𝑣𝑧 = 𝑢𝑧
for both objects
EXAMPLE
A ball is dropped vertically a distance of 5 m onto a
plane surface sloping at 35° to the horizontal.
How far down the slope is its second bounce if the
coefficient of restitution 𝑒 is:
(a) 1.0;
(b) 0.5.
5 m
35o
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FRICTION
● Tangential force generated between surfaces in contact that
opposes relative motion.
● May or may not be sufficient to prevent relative motion.
● If sliding does occur, friction does negative work and
mechanical energy is lost as heat.
● For rolling rather than sliding, friction causes the rotation.
● Models where friction is neglected are called ideal.
● Many devices rely on friction; e.g. conveyor belts, belt drives,
brakes, clutch plates, screws.
TYPES OF FRICTION
● Dry friction (this course)
● Fluid friction (hydraulics courses)
● Internal friction
U(y)
y
MODELLING FRICTION
Friction between solid surfaces is:
● tangential to the surfaces in contact;
● direction opposed to relative motion or tendency to motion;
● dependent on surfaces and normal reaction N.
Up to the point of sliding:
Once sliding occurs:
μ𝑠 is the coefficient of static friction
μ𝑘 is the coefficient of kinetic friction
In most cases we won’t make a distinction: just write μ
𝐹 ≤ 𝐹𝑚𝑎𝑥 = μ𝑠𝑁
𝐹 = μ𝑘𝑁
N
F
P
F
Fmax Ns
Nk
mg
N
F P
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FRICTION – REMEMBER!
● Direction: opposite to resultant force in the
absence of friction (the “motive force”);
● Magnitude: only given by μ𝑁 when moving.
P
F
Fmax Ns
Nk
EXAMPLE
(a) A block of mass 5 kg can be pushed up a slope of 1 in 3
at constant speed by a force of 45 N applied horizontally.
Deduce the coefficient of friction, μ.
(b) If, instead, the 45 N force is applied parallel to the slope,
what is the block’s acceleration up the slope?
GRAVITY-DRIVEN MOTION ON A SLOPE
An object on a slope may:
‒ topple over
‒ stay still
‒ slide
Does it topple?
– Consider the line of action through the centre of gravity.
If it doesn’t topple:
No sliding if:
N
F
mg
𝑁 = 𝑚𝑔 cos θ 𝐹𝑚𝑎𝑥 = μ𝑠𝑁 = μ𝑠𝑚𝑔cos θ
𝑑𝑜𝑤𝑛𝑠𝑙𝑜𝑝𝑒 𝑤𝑒𝑖𝑔ℎ𝑡 𝑐𝑜𝑚𝑝𝑜𝑛𝑒𝑛𝑡 ≤ 𝐹𝑚𝑎𝑥
𝑚𝑔sin θ ≤ 𝜇𝑠𝑚𝑔 cos θ
tanθ ≤ μ𝑠
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EXAMPLE
A crate of mass 30 kg is propelled along a horizontal surface
at steady speed by a horizontal force of magnitude 𝑃 = 120 N.
(a) What is the coefficient of friction between crate and
ground?
For the same coefficient of friction, what minimum force must
be applied to move the crate if it is directed:
(b) at 25° below the horizontal;
(c) at 25° above the horizontal.
30 kgP
30 kg
P
30 kg
P25
o25
o
(a) (b) (c)
EXAMPLE
Two cars, A of mass 800 kg and B of mass 1200 kg, collide at a 90° crossroads as
shown. The collision is completely inelastic and after the collision the cars continue
to move as a single body, sliding a distance 18 m at angle 30º to the original
direction of A before stopping.
(a) If car A was travelling at 30 m s–1 before the collision, find the speed of car B
before the collision and the speed of the combined vehicles after the collision.
(b) Assuming that all car wheels lock at the point of impact, find the total
coefficient of kinetic friction between the tyres and the ground.
800 kg30 m/s
1200kg
30o
18 mA
B
FINITE OBJECTS, NOT PARTICLES
● Newton’s Laws apply to point particles.
● Real objects consist of many particles … acted upon by:
‒ internal forces (equal and opposite in pairs);
‒ external forces.
● Important properties: total mass 𝑀 and centre of mass x
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DYNAMICS OF A SYSTEM
m1m4
m3
m2
m5
F
Individual particle:
Sum over all particles:
Motion of centre of mass:
where:
f𝑖 = 𝑚𝑖
d2x𝑖
d𝑡2
f𝑖 =𝑚𝑖
d2x𝑖
d𝑡2=
d2
d𝑡2𝑚𝑖x𝑖
F =d2
d𝑡2(𝑀x)
F = 𝑀d2x
d𝑡2
𝑀 =𝑚𝑖
𝑀x =𝑚𝑖 x𝑖
MOMENTS
moment = quantity distance
CENTRE OF MASS
Lots of masses 𝑚1, 𝑚2, 𝑚3, ... at points x1, x2, x3, ...
vs
one mass 𝑀 at point x
Require: same total mass
same total moment of mass
𝑀 =𝑚𝑖
𝑀x =𝑚𝑖x𝑖
x =σ𝑚𝑖x𝑖
𝑀=𝑡𝑜𝑡𝑎𝑙 𝑚𝑜𝑚𝑒𝑛𝑡 𝑜𝑓 𝑚𝑎𝑠𝑠
𝑡𝑜𝑡𝑎𝑙 𝑚𝑎𝑠𝑠
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INDIVIDUAL COORDINATES
𝑥 =σ𝑚𝑖𝑥𝑖𝑀
, 𝑦 =σ𝑚𝑖𝑦𝑖𝑀
, 𝑧 =σ𝑚𝑖𝑧𝑖𝑀
MOMENT ABOUT THE CENTRE OF MASS
The net moment about the centre of mass is zero.
𝑚𝑖(x𝑖 − x) =𝑚𝑖x𝑖 −𝑚𝑖x
=𝑚𝑖x𝑖 −𝑀x
= 0
IMPORTANT PROPERTIES (I)
For a system of particles:
Momentum:
● The centre of mass moves like a single particle of mass 𝑀under the resultant of the external forces .
Energy:
● In uniform gravity, total gravitational potential energy is the
same as a single particle of mass 𝑀 at the centre of mass.
● Total kinetic energy of a system is:
‒ kinetic energy of the centre of mass, 1
2𝑀𝑉2; plus
‒ kinetic energy of the system relative to the centre of mass.
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IMPORTANT PROPERTIES (II)
Rotation:
● For a rigid body, the motion relative to the centre of
mass is pure rotation:
● Total angular momentum of a system is:
‒ angular momentum of the centre of mass; plus
‒ angular momentum relative to the centre of mass.
● The rotational equation of motion
torque = rate of change of angular momentum
holds for the resultant of all external torques about a
point which is either:
‒ fixed; or
‒ moving with the centre of mass.
V V
2
21 MVKE = 2
212
21 IMVKE ω+=
FINDING THE CENTRE OF MASS
1. First principles:
2. Geometric centre:
(centroid)
3. Symmetry G
4. Addition or subtraction of simpler elements
m1m2
m1
m2
add subtract
x =σ𝑚𝑖x𝑖
𝑀=𝑡𝑜𝑡𝑎𝑙 𝑚𝑜𝑚𝑒𝑛𝑡 𝑜𝑓 𝑚𝑎𝑠𝑠
𝑡𝑜𝑡𝑎𝑙 𝑚𝑎𝑠𝑠
x =σ𝑣𝑖x𝑖𝑉
=𝑡𝑜𝑡𝑎𝑙 𝑚𝑜𝑚𝑒𝑛𝑡 𝑜𝑓 𝑣𝑜𝑙𝑢𝑚𝑒
𝑡𝑜𝑡𝑎𝑙 𝑣𝑜𝑙𝑢𝑚𝑒
EXAMPLE
Three particles of mass 3, 3 and 4 units are at rest
on a smooth horizontal plane at points with position
vectors i + 4j, 5i + 10jand 3i + 2j respectively.
Find the position of their centre of mass.
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EXAMPLE
Find the position of the centre of mass of the L-shaped
lamina shown.
0.5
2.0
0.5
1.5
EXAMPLE
A uniform lamina is formed by cutting quarter-circles of radius 0.5 m and
0.2 m from the top-right and bottom-left corners respectively of a rectangle
whose original dimensions were 0.6 m by 0.8 m.
(a) Find the area of the lamina.
(b) Find the position of the centre of mass relative to the top-left corner, A.
(c) If the lamina is allowed to pivot freely in a vertical plane about corner
A, find the angle made by side AB with the vertical when hanging in
equilibrium.
(The centre of mass of a quarter-circular
lamina of radius 𝑅 is4
3𝜋𝑅 from either
straight side.)
A
B
0.5 m
0.2 m
0.8 m
0.6 m
EXAMPLE
Find the position of the centre of mass of a
uniform solid hemisphere of radius 𝑅.
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