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AS Physics

Practical Equipment

Apparatus Resolution
Meter rule 1mm
Vernier calipers 0.05mm
Micrometer screw gauge 1µm

Momentum

The product of mass and velocity.

p=mvp = mv

The Principle of Conservation of Momentum

The total linear momentum before a collision is equal to the total linear momentum after a collision unless the system is acted on by a resultant external force

Force

The rate of change of momentum

F=ΔpΔtF = \dfrac{\Delta p}{\Delta t}

Collisions

Elastic Collisions

The collision in which the total kinetic energy of the system is conserved

  • The relative speed of approach = the relative speed of separation

Inelastic Collisions

The collision in which the total kinetic energy is not conserved

  • Occurs when objects crumple and deform

Center of Gravity

The point at which the weight of the object may be considered to act

Moment

The turning effect of a force

moment=Fdmoment = Fd

Couple

A pair of forces that acts to produce rotation only

  • Equal in magnitude
  • Opposite in direction
  • Perpendicular to the distance between them

Torque

The moment of a couple

τ=Fd\tau = Fd

The Principle of Moments

For a system to be in equilibrium, the sum of clockwise moments about a point must be equal to the sum of the anticlockwise moments (about the same point)

Archimedes' Principle

An object submerged in a fluid at rest has an upward buoyancy force (upthrust) equal to the weight of the fluid displaced by the object

F=ρgVF = \rho g V

Energy

The Principle of Conservation of Energy

Energy cannot be created or destroyed, it can only be transferred from one energy store to another

Gravitational Energy

Energy stored in a mass due to its position in a uniform gravitational field

Kinetic Energy

Energy an object has due to its motion

Deformation

Hooke's Law

Extension is directly proportional to the applied force

F=kxF = kx

The Spring Constant

A measure of the stiffness of a spring

k=FXk = \dfrac FX

Stress

Applied force per unit cross sectional area

  • The ultimate tensile stress is the maximum tensile stress before breaking

σ=FA\sigma = \dfrac FA

Strain

Extension per unit length

ϵ=XL\epsilon = \dfrac XL

Young Modulus

The ratio of stress and strain

  • A measure of how stiff or elastic a material

E=σϵ=FLAxE = \dfrac \sigma \epsilon = \dfrac{FL}{Ax}

Wave

The Wave Equation

v=fλv = f \lambda

Wave Intensity

I=PAI = \dfrac PA

IA2I \propto A^2

If2I \propto f^2

Progressive Waves

Waves that transfer energy without transfer of matter

Transverse Waves

A wave in which the particles oscillate perpendicular to the direction of motion and energy

  • Peaks and troughs
  • Electromagnetic waves, visible light, UV, vibrations on strings
  • Can be polarized

Longitudinal Waves

A wave in which the particles oscillate parallel to the direction of motion and energy transfer

  • A rarefaction is an area of low pressure, with the particles being further apart from each other
  • A compression is an area of high pressure, with the particles being closer to each other
  • Cannot travel through a vacuum
  • Sound waves

Doppler Effect

fo=fs(vv±vS)f_o = f_s (\dfrac{v}{v \pm v_S})

  • vv: wave velocity
  • vsv_s: velocity of the source relative to the observer

  • Source moving towards: vvsv - v_s

  • Source moving away: v+vsv + v_s

  • Source is moving

  • Observer is stationary

Electromagnetic Spectrum

Radiation Wavelength/m
Gamma Rays 1e-16, 4e-13
X Rays 4e-13, 1e-8
Ultraviolet 1e-8, 4e-7
Visible 4e-7, 7e-7
Infrared 7e-7, 1e-3
Microwaves 1e-3, 1e-1
Radio 1e-1, \infty
  • Memorization:
    • 1 4 1 4 7 1 1
    • 6 3 8 7 7 3 1

Malus's Law

If unpolarized electromagnetic waves of intensity I0I_0 pass through a polarizer, the intensity of the transmitted polarized waves falls by a half

I=I02I = \dfrac{I_0}2

If the analyzer is rotated by an angle θ with respect to the polarizer, the intensity of the waves transmitted by the analyzer is given by the equation

I=I0cos2(θ)I = I_0 \cos^2(\theta)

Superposition

The Principle of Superposition

When two or more waves overlap at a point, the displacement at that point is equal to the sum of the displacements of the individual waves

Wavelength of Stationary Waves

Waves that do not transfer energy and matter

Fundamental Mode of Vibration / First Harmonic

The simplest wave pattern of a wave fixed at both ends is a single loop made up two nodes and an antinode.

  • Nodes are locations of zero amplitude
  • Antinodes are locations of maximum amplitude

Zero Open Ends

L=nλ2,n[1,3]L = \dfrac{n \lambda}2, n \in [1, 3]

One Open End

L=nλ4,n is oddL = \dfrac{n \lambda}{4}, n\ is\ odd

Two Open Ends

L=nλ2,nNL = \dfrac{n \lambda}2, n \in \mathbb{N}^*

Diffraction

The spreading out of waves when they pass an obstruction

Conditions for Constructive & Destructive Interference

  • Constructive interference: path difference = nλ,nNn \lambda, n \in \mathbb{N}
  • Destructive interference: path difference = (n+12)λ,nN(n+\dfrac12) \lambda, n \in \mathbb{N}

Coherence

Waves have the same frequency and constant phase difference

Double Slit

λ=axD\lambda = \dfrac{ax}D

  • λ\lambda: wave length of source
  • aa: distance between the centers of the slit
  • xx: fringe width (distance between successive bright fringes)
  • DD: distance between the slits and the screen

The Diffraction Grating

  • Use monochromatic light: one wavelength
  • From a laser to ensure that the light beams are coherent
  • Better than Young's double slit

asin(θ)=nλa \sin(\theta) = n \lambda

  • aa: spacing between adjacent silts
  • θ\theta: angular separation between the order of maxima
  • nNn \in \mathbb{N}: order or maxima
  • λ\lambda: wavelength of source

To calculate the orders of maxima, θ=90,sin(θ)=1\theta = 90^\circ, \sin(\theta) = 1

Silt Spacing

Diffraction gratings come in different sizes measured by lines/m, represented by NN

d=1Nd = \dfrac1N

Atomic Structure and Particle Physics

Nuclear Force

Strong Nuclear Force: A fundamental force that acts between particles such as protons and neutrons, but which does not affect particles like electrons

Radiation

Radiation Nature Charge Penetrating ability in air Affected by magnetic fields
α\alpha 24He2+^4_2He^{2+} +2e+2e 6cm a little
β\beta^- electron 1e-1e 2m a lot
β+\beta^+ positron +1e+1e 2m a lot
γ\gamma electromagnetic ray 00 never completely stop none
  • α:ZAXZ2A4Y+24α\alpha: ^A_Z X \rightarrow ^{A-4}_{Z-2}Y + ^4_2 \alpha
  • β:np+10β+ve\beta^-: n \rightarrow p + ^0_{-1}\beta^- + \overline{v_e}
  • β+:pn++10β++ve\beta^+: p \rightarrow n + ^0_{+1}\beta^+ + v_e

Particles

Leptons: subatomic fundamental particles that are not affected by strong nuclear force

Hadrons: subatomic particles made up of quarks that are affected by strong nuclear force

Baryon: three quarks

Meson: one quark and one antiquark

Quark Charge Antiquark Charge
Up +23e+\dfrac{2}{3}e Antiup 23e-\dfrac{2}{3}e
Down 13e-\dfrac{1}{3}e Antidown +13e+\dfrac{1}{3}e
Charm +23e+\dfrac{2}{3}e Anticharm 23e-\dfrac{2}{3}e
Strange 13e-\dfrac{1}{3}e Antistrange +13e+\dfrac{1}{3}e
Top +23e+\dfrac{2}{3}e Antitop 23e-\dfrac{2}{3}e
Bottom 13e-\dfrac{1}{3}e Antibottom +13e+\dfrac{1}{3}e