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Physics 111 Semester Review

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Title: Physics 111 Semester Review


1
Physics 111Semester Review
  • Kinematics
  • Dynamics
  • Work, Kinetic Energy, Potential Energy
  • Momentum, Collisions
  • Gravity
  • Oscillations
  • Waves
  • Fluids/Kinetic Theory
  • Thermodynamics

2
Kinematics, Constant Acceleration
  • Position x x0 v0,x t (1/2) ax t2
  • The x-coordinate at time t is equal to the
    initial x-coordinate x0 plus the initial velocity
    v0,x times t plus one-half the acceleration ax
    times t -squared.
  • Velocity vx v0,x ax t
  • Velocity equals initial velocity plus
    acceleration times time
  • Solve velocity equation for t, plug into position
    equation
  • (x- x0) ax (1/2) (vx 2- v0,x 2)
  • An equation of position and velocity, without
    explicit reference to time.
  • Measure acceleration from a velocity vs time
    graph
  • a (v2-v1) / (t2-t1)
  • Acceleration equals change in velocity divided by
    time to achieve the change.

3
Vectors trigonometry
C
A
  • Vector components add separately
  • A B C
  • Ax Bx Cx
  • Ay By Cy
  • If you put the origin of a coordinate system at
    the tail of vector A, and figure out the angle q
    between the x-axis and A, then
  • Ax A cos q
  • Ay A sin q

B
x
A
Ay
q
Ax
x
4
Motion in 2 (or more) dimensions
  • If the motion is in two dimensions,
  • each coordinate can be analysed separately.
  • Just replace x ??y in equations
  • Example Trajectory motion, free fall
  • Launch projectile at an angle q from horizontal
  • with initial speed v0
  • v0,x v0 cos(q) v0,y v0 sin(q)
  • ax 0 ay -g
  • x x0 v0,x t y y0 v0,y t - (1/2) g t2
  • 0 (vx 2- v0,x 2) -(y- y0) g (1/2) (vy 2-
    v0,y 2)

5
Dynamics
  • Inertia resistance of object to change in state
    of motion.
  • Mass measure of inertia
  • Forces act to change the state of motion of an
    object
  • Net Force Sum of all forces acting on a mass m
  • This is statement that forces simply add
  • Net Force mass times acceleration
  • This is Newtons 2nd law, linking the force with
    motion
  • Notice that individual forces do not separately
    acceleration, only the sum of all forces
  • Fnet m a
  • Fnet 0 if and only if acceleration is zero
  • If acceleration is zero, then velocity does not
    change.

6
Examples of Forces
  • Gravity (near surface) F mg (down)
  • Gravity acting on a mass m a distance r from
    center of mass M
  • Earth radius RE, Mass ME, mass m at height h
    above surface, h ltlt RE,
  • Tension Pulls object only in direction of
    string
  • Spring force F - k (x-x0)
  • x0 equilibrium position (often x0 0).

7
Forces of contact
  • The force at the contact between two objects
  • separated into its components parallel and
  • perpendicular to the surface
  • Force parallel Friction force
  • Force Perpendicular normal force N
  • Normal force acting on m points into m
  • (this is the no glue hypothesis).
  • Normal force has whatever magnitude necessary to
    keep v_perp0
  • (this is the no walking through walls
    hypothesis).
  • If a block slides on an incline, or a cart rolls
    on a track, v? 0
  • Even for a ball bouncing on floor, v ? 0 at
    moment of contact (even though v ? ? 0)
  • Normal force is NOT mg. Sometimes N has same
    value as Gravitymg.

Ff
N
8
Apparent Weight Weightnessless
  • If you stand on a scale, the force of the scale
    pushing up on you (the force N) is your APPARENT
    WEIGHT.
  • This force is bigger than mg (the force of
    gravity acting on you) if you are standing in an
    elevator accelerating upwards
  • N - mg ma
  • This force is smaller than mg if you are standing
    in an elevator accelerating downwards.
  • This force is zero if you are an astronaut in the
    space-station in free-fall.
  • Weightnessless does not mean force of gravity 0.

a
mg
N
9
Static Friction force
  • Static Friction,
  • Mass m is not moving relative to surface of
    contact
  • FS lt mSN
  • The force of static friction takes on whatever
    magnitude or direction (but parallel to surface)
    necessary to keep v?? 0 (component of velocity
    parallel to surface).
  • Note if v?? 0 and constant, then a?? 0.
  • But FS cannot exceed the numerical value mSN.

Fs
N
mg
10
Kinetic Friction
v
  • Magnitude of the force of kinetic friction is
    fixed
  • FK mKN
  • Direction of force of kinetic friction on mass m
    opposes the slipping of mass m on the surface.
  • Acceleration can be positive, negative, or zero.

FK
N
mg
11
Free Body Diagramswww.physics.odu.edu/hyde/Teach
ing/Lectures/FreeBodyDiagrams.html
  • Draw a sketch
  • Draw a separate sketch of just the mass m.
  • Draw all forces acting on mass m
  • Give each force a unique label N, mg, fs
  • Do not give the same force more than one label.
  • Draw all forces again with all tails at the
    origin of a coordinate system.
  • Evaluate x- and y-components of forces
  • Nx0 NxN, Fk,x -FK, Fk,y 0
  • Wx mgcos(270-q) Wymg sin(270º-q)
  • Identify all constraints
  • FK mK N
  • Action-Reaction partners.
  • Apply Newton 2nd Law Sum of all forces acting
    on mass m equals m times acceleration a of mass
    m.
  • Fnet ma

v
q
FK
N
mg
N
x
FK
mg
12
Work, Kinetic Energy, Mechanical Energy,
Potential Energy
  • In kinematics of freefall, we already got a hint
    of the role of energy
  • -(y- y0) g (1/2) (vy 2- v0,y 2) 0 (vx 2-
    v0,x 2)
  • Gravity is a conservative force. Near surface of
    earth, gravitational potential energy mgy.
  • Free Fall, Mechanical energy is conserved E K
    U constant, or DK DU 0, or -DU DK
  • -DU -(mgy mg y0) DK (1/2) m v 2- (1/2)m v2

13
Work
d
q
F
  • A force F acts on a mass m while the force moves
    through a displacement d (there may be other
    forces also).
  • The Work W done by force F is W F d cosq
  • q is the angle between the force and the
    displacement.
  • The total Work WTotal is just the work done by
    the net force. This is also the sum of the works
    done by each force.
  • WTotal Fnet d cosq
  • q is the angle between net force Fnet and
    displacement d
  • WTotal F1 d cosq1 F2 d cosq2
  • q1 is the angle between force F1 and
    displacement d.
  • Example A frictionless stationary track does no
    work on a sliding/rolling object The normal
    force is perpendicular to the motion (by
    definition).
  • Use work to analyze motion on track without every
    worrying about that confusing Normal-force!!

14
Work Energy Theorem
  • Total Work done on mass m equals change in
    kinetic energy of m.
  • Wtotal Kf Ki DK
  • K (1/2) m v2

15
Conservative Forces
  • A conservative force is a force that depends only
    on position
  • Gravity
  • Spring force F -kx
  • Electrostatics (next semester).
  • A non-conservative force depends also upon the
    present (or past) state of motion.
  • Friction

16
Potential Energy
  • A conservative force depends only on position.
  • A particle therefore has the ability to change
    its state of motion, just by virtue of its
    position. This is the potential to do work, or
    potential energy.
  • If the conservative force F does work W on a
    particle of mass m (other forces may also be
    present), define the potential energy U
    associated with the conservative force F as
    follows
  • W -DU - (Uf -Ui)
  • This only defines changes in potential energy,
    the location x0 such that U(x0)0 is yours to
    choose at will.

17
Examples of Potential Energy
  • Ideal Hookes Law Force
  • U (1/2) k x2
  • Gravity (a mass m a distance r from center of
    mass M). We choose U?0 as r??.
  • Gravity a distance h above surface of Earth
    (radius RE, mass ME)

For motion near earth surface, use U(RE h)-U(RE)
mgh
18
Mechanical Energy E
  • E K U kinetic potential energy
  • WNC Work done on mass m by non-conservative
    forces.
  • WNC Ef Ei DE
  • If WNC 0, then mechanical energy is conserved
  • DE 0 ? Ef Ei

19
Thermal Energy
  • Total energy includes internal Thermal Energy Uth
  • The work done by nonconservative forces is
    converted into heat (some goes into system, some
    into surroundings).
  • Change in Thermal energy Uth Heat into system
    minus work done by system
  • D Uth Q - W

20
Momentum Collisions
  • Momentum p mv
  • Fnet m a or Fnet rate of change of momentum
  • If there are no external forces, then momentum is
    conserved (e.g. collisions)
  • p1,i p2,i p1,f p2,f
  • Good way to analyze motion without worrying about
    details of forces
  • Elastic collision, Total kinetic energy is
    conserved
  • Inelastic collision, Total momentum conserved,
    but kinetic energy decreases (splatheat) or
    increases (explosion).

21
Oscillations
  • Mass m on a spring with ideal Hookes law spring
    constant k
  • F - k x
  • E (1/2) m v2 (1/2) k x2 constant.
  • Motion is periodic with period 2p/w
  • w k/m1/2
  • X(t) A cosw(t-t0)

22
Waves
  • Waves on string, velocity v F/s1/2
  • F tension in string
  • s M/L mass per unit length
  • Wavelength, frequency, velocity
  • v f l

23
Fluids, Kinetic Theory, Thermodynamics
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