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PHY354H1
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Erich Poppitz
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Lecture

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Physics

PHY354H1

Erich Poppitz

Winter

Description

PHY254 Lecture 3
▯ Readings: Morin 3.2-3.4. Continue reading compwiki website.
▯ In this lecture we cover an example of F=ma that is not static, then
consider F=ma problems in a more general format using ODEs (Ordi-
nary Di▯erential Equations).
Setting up F = ma problems: dynamics
▯ When the sum of the forces on a system do not balance, we get a net
acceleration according to Newton’s second law:
~ dv
F = m~ a = m dt (1)
▯ Like in statics, we ▯rst need to draw an FBD and decompose the forces
into components. We also have to use information about constraints
like string. We will not do dynamical torque problems until later in the
course.
▯ Question: Consider the pulley system with masses m 1nd m (2orin,
p. 59)
Find the acceleration of the masses and the tension in the string.
▯ Partial Answer: The force equations are:
1 For m 2 T ▯2m g =2m a 2 2
For P 2the pulley attached to m ): 22 = T 1since2the mass of the
pulley is 0).
For m 1 T ▯1m g =1a . 1
Plugging in the second equation into the ▯rst equation we get the fol-
lowing 2 equations:
T 1 m g 1 m a ;1 1 ▯ m 1 = m 2 2 2 (2)
How many equations in how many unknowns? 2 equations and 3 un-
knowns. How do we close the system: we use "conservation of string",
which we assume is inextensible. If m moves down 2d, m moves up
1 2
d. So
a 1 ▯2a ; 2
which is the third equation we need. See the book for the rest of the
solution. The ▯nal answers are:
(2m 1 m )g2 2(m 2 2m )g1 2m (1 ▯ 2m )g 1
a2= ; a1= ; T = +m g1
(4m +1m ) 2 (4m 1 m ) 2 (4m 1 m ) 2
▯ This is an example of how using constraints provides required extra
information. There are lots of examples in the book.
F=ma as an ODE
▯ In the previous examples, forces were usually constant which made
them easy to deal with. You will notice that the accelerations were
always constants. This meant it would then be easy to ▯nd the velocity
and position by using constant acceleration kinematics.
▯ In general, forces can depend on variables such as time, position and
velocity. We want to develop a way of solving an F=ma problem for a
general F. Lets consider the one-dimensional case (or you can consider
this as a single component of the vector case). In one dimension, we
can write
F = F(t;x;v) (3)
2 ▯ Newton’s second law states that
dv
m = F(t;x;v) (4)
dt
To get to a solution for v(t) and x(t), we are going to need to do
2 integrations, which means we will have 2 constants of integration.
These can be solved for using initial conditions on the initial position
and/or the initial velocity. Let’s assume the initial conditions to our
above problem are given by
x(t0) = x 0 v(t0) = v 0
▯ Equation (4) has no general solution, but we can consider three rela-
tively simple cases: a time dependent force, a position dependent force,
and a velocity dependent force.
Case 1: Time dependent force F=F(t)
▯ In this case we have:
dv
m = F(t) (5)
dt
We can separate variables
mdv = F(t)dt (6)
Then we can integrate the equation.
Z v(t) Z t
0 0 0
m v dv = m(v(t) ▯ v ) 0 t F(t )dt )
0 0
Z t
v(t) = v + 1 F(t )dt 0 (7)
0 m t0
This gives us v = v(t). But since v(t) = dx, we can integrate again:

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