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Friction, Forces and Motion-II, Schemes and Mind Maps of Physics

The concept of friction, static friction, kinetic friction, and centripetal force, with examples and problems. It also covers the forces acting on objects in circular motion and the source of centripetal force. calculations for the force required to move a box, the accelerations of blocks on an incline, and the motion of a ball on a string.

Typology: Schemes and Mind Maps

2021/2022

Uploaded on 09/12/2022

laskhminaran
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6. Forces and Motion-II
Friction:
The resistance between two surfaces when
attempting to slide one object across the
other.
Friction is due to interactions at molecular
level where “rough edges” bond together:
Friction is always opposite to the direction of
motion.
F
f
F
f
Friction are both friend and foe of everyday
life, for example:
H Allow you to start your car from rest
H Slow the car down
H Allow you to break
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6. Forces and Motion-II

Friction:

  • The resistance between two surfaces when attempting to slide one object across the other.
  • Friction is due to interactions at molecular level where “rough edges” bond together:
  • Friction is always opposite to the direction of motion.

F f

F f

  • Friction are both friend and foe of everyday life, for example: H Allow you to start your car from rest H Slow the car down H Allow you to break

Static Friction: N

f mg

F

s

  • The frictional force between two surfaces in attempting to slide one object across the other but neither objects are moving with respect to each other.
  • The friction is always equal to the net force parallel to the surface.
  • If one net force increases or decreases, the friction force will also increase or decrease to compensate.
  • Experimentally, the maximum magnitude of static friction is proportional to the magnitude of the normal force: f (^) s^ max^ = (^) μ s N

∑ Fy =^ N^ −^ mg^ −^ Fsin^ θ^ =^0 N (^) = mg (^) + F sin θ ∑ Fx =^ F^ cos θ^ −^ f^ s >^0 F cos θ (^) − μ s N (^) > 0

F cos θ − μ s (mg + Fsin θ ) > 0

F cos θ (^) − μ s Fsin θ (^) > μ smg

F (^) > μ smg cos θ (^) − μ s sin θ

  • If we increase the angle to the critical angle, cos θ^ =^ μ s sin θ^ , no matter how hard the student pushes, the box will not move, i.e. the vertical component of the force produces a normal force which yields a frictional force that is larger than the horizontal component of the force.

Kinetic Friction: Once an object is in motion, the friction force changes to kinetic friction force, which is proportional to the magnitude of normal force, f (^) k = μ k N

where μ k is the coefficient of kinetic friction.

  • Unlike the static friction force, the kinetic friction force does not change in magnitude. It has a single value.
  • μ k < μ s, i.e. once you start moving an object, it

is easier to keep it moving.

Problem 39 (p. 127): A 10 kg block rests on top of a 40 kg slab which rests on a frictionless floor. The coefficient of static and kinetic friction between the block and the slab are 0.60 and 0.40 respectively. The block is pulled with a force of 100 N. What are the accelerations of (a) the block and (b) the slab?

(^100) m

m

y

x

1 2 N F (^) f

m 1 g

N f

m 2 g

N

'

N

a 1 = μ k g −

F

m 1 = −6.1 m / s^2 Slab: (^) ∑Fx = − μ k N (^) = m 2 a 2 − μ k m 1 g^ = m 2 a 2

a 2 = − μ k m 1 g m 2 = − 0. 98 m / s^2

Example: Two identical blocks of 10 kg each are sitting on an incline with an angle θ = 30°. One block is released so that its initial speed is zero, while the other block is released with an initial speed of 1 m/s. What are the accelerations of each block just after the release and 10 s later? The coefficients of static and kinetic friction are 0.7 and 0.6. N (^) f

θ mg

θ

0 =^ N^ f

θ mg

θ

= 1 y

x

v 0 v (^0) x m/s

Block 1 : (^) ∑ Fy = N (^) − mg cos θ (^) = 0

N (^) = mg cos θ f (^) s = μ s N = μ smg^ cos θ = 59 N Fgx = mgsin θ = 49 N < f (^) s  The block will remain stationary.

Block 2 : (^) ∑ Fy = N (^) − mg cos θ = 0

N (^) = mg cos θ ∑ Fx =^ mgsin^ θ^ −^ f^ =^ ma mgsin (^) θμ k N (^) = ma mgsin (^) θμ k mg cos θ = ma a = g(sin θμ k cos θ ) = −0.19 m / s^2

  • Since the acceleration is in the -x direction (up the plane), the block will slow down and come to a stop.

d (^) m

v k k

0 1 1

2 2

= 5

μ μ

θ θ

N (^) f

θ mg

θ

y

x 1 1

k

∑ Fy = N − mg cos θ 1 = 0

N = mg cos θ 1

∑ Fx = mgsin θ 1 − fk = max 1

mg sin θ 1 − μ k mg cos θ 1 = max 1

ax 1 =^ g(sin θ 1 −^ μ k cos θ 1 )

= (9.8 m / s^2 )(sin 30°−0.6 cos30°) = −0.19 m / s^2 x = x 0 + v (^0) x t 1 + 12 ax 1 t 12

2 =^0 +^1 ×^ t 1 −^12 (0.19)t 12

0.092t 12 − t 1 + 2 = 0

t 1 = 1.6 or −12.1 s

v =^ v 0 +^ ax 1 t 1

= 1 − 0.19 ×1. = 0.70 m / s

∑ Fy = N^ − mg^ cos θ 2 = 0 N (^) = mg cos θ 2 ∑ Fx = − f^ k − mgsin^ θ 2 = max 2 − μ k 2 mg^ cos θ 2 − mgsin^ θ 2 = max 2 μ k 2 gcos θ 2 = −gsin θ 2 − ax 2

μ k 2 =

−gsin^ θ 2 − ax 2 g cos θ 2 = 0.^15

H We solve this complicated problem one piece at a time. v^2 =^ v 02 +^2 a(x −^ x 0 ) 0 =^ v 02 +^2 ax 2 (d −^ 0)

d = −^ v 02 2 ax 2

2 2(−2.33) = (^) 0.11 m

Centripetal Force: The force directed toward the center that provides the acceleration for an object in a circular motion:

Fc = ma = m v^2 r e.g. gravity, tension, normal force.

  • Centripetal force provides the centripetal acceleration.
  • Centripetal acceleration is not a force.

Example: A 2 kg ball on a string of length L = 1 m has a period of 0.5 s. Ignoring the gravitational force, what is the speed, centripetal acceleration, and tension?

Problem 5 7 (p.128) A mass m on a frictionless table is attached to a hanging mass M by a cord through a hole in the table. Find the speed with which m must move in order for M to stay at rest for a radius r.

M

m

r T

Mg

T

T = mac = m v^2 r T − Mg = 0

Mg =^ m v^2 r

v =^ Mgr m

Conceptual Question:

Determine the source of the centripetal force that causes the object to move in a circle:

  1. A ball on a string:
  2. A car going around a banked curve:
  3. A satellite orbiting the earth:
  4. A car going over a rounded hill:

r

Conceptual Question:

(a) v (^) = 2 π r T

=

2 π r π 3 = 6 r = 0.3 m s

a (^) = v^2 r = 1.82 m s^2 (b) f (^) = ma

= 3.^64 × 10 −^3 N

(c) At r = 10 cm, the friction is just enough to provide the centripetal force:

μ N (^) = mv^2 r

μ mg (^) = mv

2 r

μ (^) = v^2 gr

2 π r T

2

gr

= 4 π^2 r gT 2

=

4 π^2 r

g π 3

2

36 r g = 0.^37