IntroductionMeter: distance light travels in vacuum during time interval of 1/299,792,458sSecond: time for 9,192,631,770 wavelengths of radiation to be emitted by a cesium atomKilogram: mass of a sphere carved from a single crystal of silicon-28

Prefix Symbol Sci. Not.Pico p 10-12

Nano n 10-9

Micro µ 10-6

Milli m 10-3

Centi c 10-2

Deci d 10-1

Kilo k 103

Mega M 106

Giga G 109

Tera T 1012

Parallax: apparent shift in the position of an object when it is viewed from different angles

Graphing: (dependent variable; x) as a function of (independent variable; y)

Quadratic: y=ax2+bx+cInverse: y=a/x

contact force objects touchlong range force gravity, magnetsagents source of the force

Period & FrequencyPeriod (T): time needed to repeat one complete cycle of motionFrequency (f): number of cycles that take place in one second; 1 cycle/s = 1 Hz

Period of mass oscillating on a spring is T=2π√(m/k)m: mass of the oscillating objectk: spring constant (if not known, can be found using k=F/x)

F: force applied to springx: distance the spring extends

Period of pendulum is T=2π√(l/g)

l: length of pendulumg: acceleration due to gravity (9.80 m/s2)

Force of compressed or stretched spring F = kxF: forcek: spring constantx: amount spring has been stretched or compressed

Scalar and Vector quantitiesScalar Quantity: quantity that tells you only magnitude (mass, distance and temperature)Vector Quantity: quantity that has magnitude and direction (displacement and velocity)

Distance and DisplacementDistance is the total length an object has moved and has no direction associated with it. Displacement is the straight-line distance between two points, and is a vector which points from an object's initial position towards its final position. (If you end where you started, displacement is 0)

Speed and VelocityAverage Speed: amount of distance a moving object covers divided by the amount of time to cover that distance.

v=∆d/∆t

AccelerationAverage acceleration: rate of change of velocity between t0 and t1

a=v1-v0/t1-t0

Equations of motionVelocity with constant acceleration v1=v0+atFinal position with constant acceleration d=do+1/2(v0+v1)t; d=do+vot+1/2at2

Final velocity with constant acceleration v12=v0

2+2a(d1-d0)

Projectile motionIgnoring air resistance, horizontal velocity of a projectile is constant

vx=∆d/t=constantInitial vertical velocity of a projectile launched horizontally is zero

voy=0Final velocity found using

vfy=-gt

Gravitational Field StrengthA gravitational field exists for all objects that have mass. At the Earth's surface Earth’s GFS is g=9.80m/s2.

Weight is the force of gravity acting on a body. Weight is the product of the mass of an object and the acceleration due to gravity that is acting on an object w=mg. Mass is a constant that does not change with location. Weight is not a constant and does change depending on the location of the object

Newton’s Law of Universal GravitationStates that every particle in the universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

F=G(m1m2/r2)F: gravitational force in NewtonsG: universal gravitational constant 6.67x10-11 N·m2/kg2

m1, m2: the 2 massesr: the distance between the centres of the 2 masses

Newton’s Laws of Motion

1. Newton’s First Law of Motion (“Law of Inertia”)A body at rest stays at rest, and a body in motion stays in motion, unless it is acted on by an external forceInertia: tendency of an object to resist changeEquilibrium: when the net force on an object is at 0; occurs in state of rest or constant velocity

2. Newton’s Second Law of Motion (“Law of Force and Acceleration”)A force acting on a mass causes that mass to accelerate in the direction of the force. The acceleration is directly proportional to the force and inversely proportional to the mass.

3. Newton’s Third Law of Motion (“Law of Action and Reaction”)For every action force, there is an equal and opposite reaction force. Action-reaction pairs act on different bodies, and they do not cancel each other. (Force a book exerts on a table and the force a table exerts on a book). [Whenever one body exerts a force on a second body, the second body exerts an oppositely directed force of equal magnitude on the first body]

FrictionKinetic Friction: The friction between two surfaces when one surface is moving relative to the other

fK: force of kinetic frictionStatic Friction: The friction between two surfaces when the surfaces are not moving relative to each other

fs: force of static friction

Force of friction = fx = µFN

µ: coefficient of frictionFN: normal force (the reaction force to an object's weight)

µ = fx/FN

fx = µ(FN)

Dynamics in One DimensionMomentumThe momentum of an objects is the product of its mass and its velocity

p=mvp: momentum in kgm/s,m: mass in kgv: velocity in m/s.

Change in momentum: ∆p=∆(mv)

ImpulseThe product of the average net force exerted on an object and the time interval over which the force acts.

Impulse = F∆TF: average force in Newtonst: time that the force is applied.

Impulse and MomentumThe impulse given to an object is equal to the object's change in momentum.

F∆t=∆(mv)

The law of conservation of momentumMomentum for any closed system upon which there is no net external force remains the same.

pi=pf

Pai+Pbi=Paf+Pbf

mava+mbvb=mavaf+mbvbf

Elastic ForcesHooke’s LawThe force needed to compress or stretch a string is directly proportional to the product of the spring constant, k, and the amount the spring has been stretched or compressed.

F=k∆xF: applied (or restoring) force in Newtonsk: spring constant in N/m∆x: distortion of the spring in m

Work, Energy, & PowerWorkWork is equal to the component of a force that is in the direction of the motion of an object & the displacement of the object

W=Fcosθd

PowerPower is the rate of doing work or the rate at which energy is transferred; measured in watts; 1 W = 1 J/s

Power = work/timeP = Fcosθd/t

Energy: property of an object that allows it to produce change in the environment or in itself. The work-energy theorem states that the change in energy of an object is exactly equal to the work done on it. W=∆E

Kinetic Energy = KE = ½(mv2)Gravitational Potential Energy = PE = mgh

where m is the mass, g the acceleration due to gravity, h is the height the object is above a reference plane.

Gravitational Potential Energy (PE or Ug): PE is the stored energy in a system resulting from the gravitational interaction between masses. When we state an object’s PE we must say which plane we are using as the reference plane.PE=mgh

Mechanical Energy: sum of the kinetic and potential energyEi = Ef

mghi + ½(mvi2) = mghf + ½(mvf

2)

Efficiency = (work output/work input) x 100%

Collisions & ExplosionsInelastic Collisions

Objects deform or stick together Kinetic energy is converted to heat Less kinetic energy after the collision Momentum is conserved

mava+mbvb=mava’+mbvb

’

Elastic Collisions No deformation Kinetic energy is conserved

mava+mbvb=mava’+mbvb

’

½mava2+½mbvb

2=½mava’2+½mbvb

’2

Explosions Object is at rest or moving at a constant velocity It breaks into 2 or more pieces The kinetic energy of the system increases

Temperature and Thermal EnergyThermal Energy(heat)-total amount of energy of all the particles.

Kinetic Molecular TheoryAll matter is made up of tiny particles that are in constant motion. Particles moving faster have more kinetic energy.

Thermal Energy: The overall energy of motion of the particles that make up an object

Conduction: heat energy is transferred to the lower temperature; when the two are at the same temperature, thermal equilibrium is reached.

Convection: transfer of heat by the process of motion in a fluid.

Radiation: transfer of energy by electromagnetic waves; does not require presence of matter.

Kelvin: 0.0 K is absolute zero, and equal to -273 oC

Specific heatAmount of energy that must be added to a material to raise its temperature 1.0 K (1.0 oC)Q=mC∆T where m is the mass, C is the specific heat and ∆T is the change in temperature.

Change of stateMelting Point: temperature at which a substance changes from a solid to a liquidBoiling Point: temperature at which a substance changes from a liquid to a gas

All of the energy added goes to overcoming the forces that hold the molecules together.The temperature does not change.

Heat of Fusion: amount of energy needed to melt one kilogram of a substanceQ=mHf where m is the mass of the substance and Hf is the heat of fusion

Heat of Vaporization: amount of energy needed to vaporize one kilogram of liquidQ=mHv where m is the mass of the substance and Hv is the heat of vaporization.

CalorimetryCalorimeter is a carefully insulated container that does not allow heat to leave or enter

Tf = (mACATAi + mBCBTBi) / mACA+mBCB

First Law of ThermodynamicsThe total increase in the thermal energy of a system is equal to the work done plus the heat added.

QTOTAL = W + Q

Heat engine: device that can convert thermal energy into mechanical energy

Heat pump

Second Law of ThermodynamicsEntropy: the state of disorderNatural processes go in a direction that maintains or increases entropy.

Wave propertiesWave: rhythmic disturbance that carries energy through matter or space

Mechanical waves carry energy through matter1. Transverse wave: a mechanical wave in which the medium moves perpendicular to the direction on the wave. Transverse

waves cannot occur in gases.2. Longitudinal wave: a mechanical wave in which the medium moves in the same direction as the wave. Longitudinal

waves can occur in solids, liquids and gases.

All waves can be represented using a sine wave:

Below the surface, ocean waves are transverse waves. At the surface they have characteristics of both transverse and longitudinal waves.

The speed of a wave is calculated by either:a. dividing the distance the wave travels by the time taken. v=∆d/∆t.b. multiplying its wavelength by its frequency. v= λf

The period of a wave is the time for one complete cycle and it is equal to T=1/f

Waves at boundaries

heat reservoir

work

QH = W + QL

QH

QL

heat engine

cold reservoir

heat reservoir

work

QH = W + QL

heat engine

cold reservoir

QH

QL

λ wavelength

When a wave hits a boundary some of the energy is transmitted through the boundary and some is reflected back. The incident wave is the wave that hits the boundary; the reflected wave is the wave that comes back. If the incident wave hits a more dense medium (one in which the wave travels faster), the reflected wave will be inverted.

Superposition of wavesThe principle of superposition states that the displacement of a medium caused by two or more waves is equal to the algebraic sum of the two individual waves

When the displacement of the waves is in the same direction, they produce constructive interferenceWhen the displacement of the waves is in the opposite direction, they cause destructive interference

If waves travel through a medium at just the right speed they appear to be stationary. These are called standing waves. The part of the medium that does not move is called the node. The part that has the maximum deflection is called the antinode.

Waves in two dimensionsθi = angle of incidenceθr = angle of reflectionθi=θr (law of reflection)

Diffraction and interference of waves: the spreading of waves around a barrier

Doppler EffectWhen objects travel towards you the sounds they make seem to have a higher pitch & when objects travel away from you the sounds they make seem to have a lower pitch

The frequency of the sound produced by an object moving toward an observer appears to be fo = fs[1-(vs/v)] where fs is the frequency of the source, vs is the velocity of the source, and v is the velocity of sound

If the object is moving away from the observer the frequency appears to be fo = fs[1+(vs/v)]

Light fundamentalsLight is the range of frequencies of electromagnetic waves that stimulate the retina of the eye. They range from about 4.00x10-7m to 7.00x10-7m. Shortest is violet, longest is red. Light travels in a vacuum at 3.00x108m/s and is represented by c.

Sources of light: An object that emits light is called luminous; an object that reflects light is illuminated

Luminous Flux (P): rate at which visible light is emitted from a source. Unit: lumen (lm)

Illuminance (E): amount of light falling on a surface; measured in lux (lx): lm/m2 E=P/4πd2

Luminous intensity: Some light sources are specified in candela (cd), or candle power. A candela is not a measure of luminous flux, but of luminous intensity. The luminous intensity of a point source is the luminous flux that falls on 1.0m2 of a sphere of one meter radius. Thus, luminus intensity is luminous flux divided by 4π; P/4π

Light and matterLight: wave, particle, or electromagnetic radiation

Transparent: materials that transmit light rays without distorting themTranslucent: materials that transmit light rays but do not allow objects to be seen clearlyOpaque: light cannot pass through

Spectrum: the ordered arrangement of colours from violet to red

Colours by additionwhite light can formed by combining red, green, & blue light

Colours by SubtractionDye: a molecule that absorbs certain wavelengths of light & transmits or reflects others; form solutionPigment: a coloured particle that absorbs certain colours & transmits or reflects others; form suspension

Primary Pigment: a pigment that absorbs only 1 primary colour from white lighto Yellow, cyan, & magenta are primary colours of pigments

Secondary Pigment: absorbs 2 primary colours & reflects 1

red

greenblue cyan

magenta yellow

white

o Red, green, blue

Wave Motion and Geometrical Optics

Index of refraction is the rate of the speed of light in a vacuum to its speed in a materialnsubstance = c/vsubstance

Snell’s LawStates that the ratio of the sine of the angle of incidence to the sine of the angle of reflection is a constant

n = sinθi/sinθr

nisinθi = nrsinθr

Critical Angle and Total Internal Reflection

Total internal reflection occurs when light passes from a more optically dense medium to a less optically dense medium, at an angle so great that there is no refracted ray

The critical angle is the angle at which the refracted ray lies along the boundary of the 2 materials

MirageWhen light rays pass through at different temperatures the light is bent away from the normal. When the air temperature at the surface of the Earth is much hotter than the air temperature in the sky, light coming from the sky is bent.

Regular & Irregular ReflectionRegular reflection mirror; you can see an imageIrregular reflection wall; you can’t see an image

Lenses & MirrorsImage orientation: an image is erect when it has same orientation as object, otherwise it is invertedVirtual image: light does not converge; cannot be projected on a screen

Mirror Shape ObjectImage

OrientationVirtual or

RealSize

Plane any upright virtual same as object

Concave

more than 2 focal lengths away from mirror

upside-down real smaller than object

b/w 1 and 2 focal lengths upside-down real larger than objectat the focal point none none none

b/w mirror and focal point upright virtual larger than objectconvex any upright virtual smaller than object

Lens/mirror equation1/f = 1/di + 1/do

Magnificationm = hi/ho = di/do

Lenses 2 focal points f is pos. for convex & neg. for concave lenses di is pos. on the image side of the lens where images are real do is pos. on the object side of the lens concave lens: image on the same side as the object

Special RelativityEinstein’s Theory of Special Relativity describes motion of particles moving at close to the speed of light

2 postulates1. the speed of light is the same for all observers, no matter what their relative speeds

2. laws of physics are the same in any inertial (non-accelerated) frame of reference; this means the laws of physics observed by a hypothetical observer travelling with a relativistic particle must be the same as those observed by an observer who is stationary

Time Dilation

∆t = ∆to / √ [1-(v2/c2)]

∆to dilated time measured by an observer who is at rest with respect to the eventv relative speed between the 2 observersc speed of light

Length ContractionLengths in the direction of relative motion are shorter for the observer who is moving the amount of length

L = Lo √ [1-(v2/c2)]

L is the length measured by the observer who is in motionLo is the proper length as measured by the observer who is at rest relative to the object

Relativistic Momentum

P = mv / √ [1-(v2/c2)]

Relativistic Addition of Velocities

U = (v + U ’) / [1+(v2/c2)]

U is the speed of the missile relative to the observer who is in motion relative to the rocketv is the velocity of the rocket relative to the moving observerU ’ is the velocity of the missile relative to the rocket

Mass Energy Equivalency

E = mc2 / √ [1-(v2/c2)]

Eo = mc2 m = Eo/c2

Radioactivity: the remission of energy or particles from an unstable nucleus; can omit:1. alpha particles ά

helium nuclei 24He

2. beta particles βhigh speed electrons -1

0e-

3. gamma rays γelectromagnetic radiation; highest frequency

Nuclear Fission/FusionWhen nuclear fission occurs, a nucleus splits into smaller nuclei; a chain reaction can occur. Nuclear fusion occurs when light nuclei collide at high temperature & form heavier nuclei, releasing a high amount of energy

(not in motion)