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SUVAT
(A.1 Kinematics)
S= displacement (m)
u= initial velocity (m/s)
v= final velocity (m/s)
a= acceleration (m/s²)
t= time (s)
Ff≤μsFN
(A.2 Forces and Momentum)
Body is stationary
Ff: Frictional force (N)
μs: Coefficient of static friction
FN= Normal reaction force (N)
Ff=μdFN
(A.2 Forces and Momentum)
Body is in motion
Ff: Kinetic friction force (N)
μd: Coefficient of dynamic (kinetic) friction
FN: Normal force (N)
F=−kx
(A.2 Forces and Momentum)
Spring
F: Restoring force (N)
k: Spring constant (N/m)
x: Displacement from equilibrium (m)
Fd=6πηrv
(A.2 Forces and Momentum)
F: Drag force (N)
η: Viscosity of the fluid (Pa·s)
r: Radius of the object (m)
v: Velocity of the object (m/s)
Fb=ρVg
(A.2 Forces and Momentum)
F: Buoyant force (N)
ρ: Density of the fluid (kg/m³)
V: Volume of the object submerged (m³)
g: Gravitational field strength (9.8 m/s²)
F = ma= Δp/Δt
(A.2 Forces and Momentum)
F: Resultant force (N)
m: mass (kg)
a: acceleration (m/s²)
Δp: Change in momentum (kg·m/s)
Δt: Time interval (s)
J = F∆t = ∆p
(A.2 Forces and Momentum)
J: Impulse (N·s)
F: Force (N)
Δt: Time duration (s)
p = mv
(A.2 Forces and Momentum)
p: Momentum (kg·m/s)
m: Mass (kg)
v: Velocity (m/s)
a= v²/r
a=ω²r
a=4πr²/T²
(A.2 Forces and Momentum)
a: Centripetal acceleration (m/s²)
v: Velocity (m/s)
r: Radius of circular path (m)
ω: Angular velocity (rad/s)
T: Period (s)
v=2πr/T
v=ωr
(A.2 Forces and Momentum)
Velocity of a body traveling in a circle
v: Linear velocity (m/s)
ω: Angular velocity (rad/s)
r: Radius of circular motion (m)
T: Period (s)
W = Fscosθ
(A.3 Work, Energy, and Power)
Work done (Nm) = Force (N) x displacement (m) x cos (angle to the force (°))
- When θ=90° No work is done
Ek=½mv²
Ek= p²/2m
(A.3 Work, Energy, and Power)
Body in motion
Ek: Kinetic energy (J)
m: Mass (kg)
v: Velocity (m/s)
p= momentum
ΔEp=mgh
(A.3 Work, Energy, and Power)
Gravitational potential energy changes when an object's height changes in a gravitational field.
ΔEp: Change in gravitational potential energy (J)
m: Mass (kg)
g: Gravitational field strength (9.8 m/s²)
Δh: Change in height (m)
EH=½k(Δx)²
(A.3 Work, Energy, and Power)
Elastic potential energy is stored in a stretched or compressed spring.
E: Elastic potential energy (J)
k: Spring constant (N/m)
Δx: Displacement from equilibrium (m)
P=W/Δt=Fv
(A.3 Work, Energy, and Power)
Power: rate of energy transfer
P: Power (W)
W: Work done (J)
Δt: Time interval (s)
F: Force (N)
v: Velocity (m/s)
η
(A.3 Work, Energy, and Power)
η: Efficiency
ρ=m/V
(B.1 Thermal Energy Transfers)
ρ: Density (kg/m³)
m: Mass (kg)
V: Volume (m³)
Ek=3/2× kB×T
(B.1 Thermal Energy Transfers)
Ek: Average kinetic energy of a particle (J)
kB: Boltzmann constant
T: Absolute temperature (K)
Q=mcΔT
(B.1 Thermal Energy Transfers)
Material changing temperature
Q: Heat transferred (J)
m: Mass (kg)
c: Specific heat capacity (J/kg°C)
ΔT: Change in temperature (K or °C)
Q=mL
(B.1 Thermal Energy Transfers)
Material changing phase
Q: Heat transferred (J)
m: Mass (kg)
L: Specific latent heat (J/kg)
ΔQ/Δt=(kA) ΔT/Δx
(B.1 Thermal Energy Transfers)
Heat conduction through a material
ΔQ/Δt: Rate of heat transfer (W)
k: Thermal conductivity (W/mK)
A: Cross-sectional area (m²)
ΔT: Temperature difference (K)
Δx: Thickness of the material (m)
ΔT/Δx: Temperature gradient (K/m)
L=σT⁴A
(B.1 Thermal Energy Transfers)
L: Total power radiated/Luminosity (W)
σ: Stefan-Boltzmann constant
T: Absolute temperature (K)
A: Surface area (m²)
b=L/4πd²
(B.1 Thermal Energy Transfers)
b: Intensity/apparent brightness (W/m²)
L: Luminosity (W)
d: Distance from the source (m)
λmaxT=2.9×10−3mK
(B.1 Thermal Energy Transfers)
Wein's Law
λmax: Wavelength of maximum intensity (m)
T: Absolute temperature (K)
P=F/A
(B.3 Gas Laws)
P: Pressure (Pa)
F: Force (N)
A: Area (m²)
n=N/NΑ
(B.3 Gas Laws)
n: Amount of substance (mol)
N: Number of particles
NA: Avogadro's constant
PV/T=constant
(B.3 Gas Laws)
P: Pressure (Pa)
V: Volume (m³)
T: Absolute temperature (K)
PV=nRT
PV=NkBT
(B.3 Gas Laws)
IDEAL GAS LAW
P: Pressure (Pa)
V: Volume (m³)
n: Number of moles (mol)
R: Gas constant
T: Absolute temperature (K)
N: Number of particles
kB: Boltzmann constant
P=1/3×ρv²
(B.3 Gas Laws)
P: Pressure (Pa)
ρ: Density of the gas (kg/m³)
v: Velocity of gas particles (m/s)
U=3/2×nRT
U= 3/2×NkBT
(B.3 Gas Laws)
U: Internal energy (J)
n: Number of moles (mol)
R: Gas constant
T: Absolute temperature (K)
N: Number of particles
kB: Boltzmann constant
Q=ΔU+W
(B.4 Thermodynamics)
Q: Heat added to the system (J)
ΔU Change in internal energy (J)
W: Work done by the system (J)
W=PΔV
(B.4 Thermodynamics)
W: Work done (J)
P: Pressure (Pa)
ΔV: Change in volume (m³)
ΔU=(3/2)×nRΔT
ΔU=(3/2)×NkBΔT
(B.4 Thermodynamics)
ΔU: Change in internal energy (J)
n: Number of moles (mol)
R: Gas constant
ΔT: Change in temperature (K)
N: Number of particles
kB: Boltzmann constant
ΔS=ΔQ/T
(B.4 Thermodynamics)
ΔS: Change in entropy (J/K)
ΔQ: Heat transfer (J)
T: Absolute temperature (K)
S=kBlnΩ
(B.4 Thermodynamics)
S: Entropy (J/K)
kB: Boltzmann constant
Ω: Number of microstates
PV⁵/₃=constant
(B.4 Thermodynamics)
For adiabatic processes in a monatomic ideal gas
P: Pressure (Pa)
V: Volume (m³)
ηCarnot=1−Th/Tc
(B.4 Thermodynamics)
Carnot efficiency is the maximum efficiency of a heat engine.
ηCarnot: Carnot efficiency
Tc: Temperature of the cold reservoir (K)
Th: Temperature of the hot reservoir (K)
I=Δq/Δt
(B.5 Current and Circuits)
I: Electric current (A)
Δq: Electric charge (C)
Δt: Time interval (s)
V=W/q
(B.5 Current and Circuits)
V: Electric potential difference (V)
W: Work done or energy transferred (J)
q: Charge (C)
R=V/I
(B.5 Current and Circuits)
R: Resistance (Ω)
V: Voltage (V)
I: Current (A)
ρ=RA/L
(B.5 Current and Circuits)
resistivity of a material
ρ: Resistivity (Ωm)
R: Resistance (Ω)
A: Cross-sectional area (m²)
L: Length of the conductor (m)
P=VI=I²R=V²/R
(B.5 Current and Circuits)
Electrical power
P: Power (W)
V: Voltage (V)
I: Current (A)
R: Resistance (Ω)
ε=I(R+r)
(B.5 Current and Circuits)
ε: Electromotive force (e.m.f) (V)
I: Current (A)
R: External resistance (Ω)
r: Internal resistance of the source (Ω)
a=−ω²/x
(C.1 Simple Harmonic Motion)
a: Acceleration (m/s²)
ω: Angular frequency (rad/s)
x: Displacement from equilibrium (m)
T=1/f
T=2π/ω
(C.1 Simple Harmonic Motion)
The period of oscillation
T: Period (s)
f: Frequency (Hz)
ω: Angular frequency (rad/s)
T=2π√m/k
(C.1 Simple Harmonic Motion)
The period of a mass-spring system
T: Period (s)
m: Mass (kg)
k: Spring constant (N/m)
T=2π√l/g
(C.1 Simple Harmonic Motion)
The period of a simple pendulum
T: Period (s)
l: Length of the pendulum (m)
g: Gravitational field strengt (m/s²)
x=x₀sin(ωt+ϕ)
(C.1 Simple Harmonic Motion)
The displacement in SHM
x: Displacement (m)
x₀: Amplitude (m)
ω: Angular frequency (rad/s)
t: Time (s)
ϕ: Phase constant (rad)
v=ωx₀cos(ωt+ϕ)
(C.1 Simple Harmonic Motion)
v: Velocity (m/s)
x₀: Amplitude (m)
ω: Angular frequency (rad/s)
t: Time (s)
ϕ: Phase constant (rad)
v=±ω√x₀²−x²
(C.1 Simple Harmonic Motion)
Velocity in SHM
v: Velocity (m/s)
x: Displacement (m)
x₀: Amplitude (m)
ω: Angular frequency (rad/s)
Ep=½mω²x²
(C.1 Simple Harmonic Motion)
Ep: Potential energy (J)
m: Mass (kg)
ω: Angular frequency (rad/s)
x: Displacement (m)
Et=½mω²x₀²
(C.1 Simple Harmonic Motion)
E: Total energy (J)
m: Mass (kg)
ω: Angular frequency (rad/s)
x₀: Amplitude (m)
v=fλ
v=λ/T
(C.2 Wave model)
v: wave speed (m/s)
λ: wavelength (m)
f: frequency (Hz)
T: time period (s)
n₁/n₂=v₁/v₂=sinθ₁/sinθ₂
(C.3 Wave Phenomena)
n1,n2: Refractive indices of media
v1,v2: Wave velocities in media (m/s)
θ1: Angles of incidence
θ2: Angle of refraction
Constructive Interference:
Path difference = nλ
Destructive Interference: Path difference = (n+½)λ
(C.3 Wave Phenomena)
n: Integer (0, 1, 2, ...)
λ: Wavelength (m)
s=λD/d
(C.3 Wave Phenomena)
Double slit
s: Fringe separation (m)
λ: Wavelength (m)
D: Distance to the screen (m)
d: Slit separation (m)
θ=λ/b
(C.3 Wave Phenomena)
Single slit
θ: Angle between central max and first min (radians)
λ: Wavelength (m)
b: Width of the slit (m)
nλ=dsinθ
(C.3 Wave Phenomena)
Multiple slits
n: Order of maxima (integer)
λ: Wavelength (m)
d: Spacing between adjacent slits (m)
θ: angular separation between order of maxima (degrees or radians)
Δf/f=λΔ/λ≈v/c
(C.5 Doppler Effect)
Doppler effect in light
Δf: Change in frequency (Hz)
f: Source frequency (Hz)
Δλ: Change in wavelength (m)
λ: Wavelength (m)
v: Relative velocity of source and observer (m/s)
c: Speed of the wave (m/s)
Moving Source:
f′=f×(v/v±us)
Moving Observer:
f′=f×(v±u)/v
(C.5 Doppler Effect)
Doppler effect in sound
f′: Observed frequency (Hz)
f: Source frequency (Hz)
v: Speed of the wave in the medium (m/s)
us: Speed of the source relative to the medium (m/s)
u₀: Speed of the observer relative to the medium (m/s)
v+us: Source moving away from observer
v- us: Source moving towards observer
v+uo: observer moves TOWARD the source
v-uo= Observer moves AWAY from the source
F=Gm₁m₂/r²
(D.1 Gravitational fields)
Gravitational force between two bodies
F: Gravitational force (N)
G: Gravitational constant,
m₂m₁: Masses of the two objects (kg)
r: Distance between the centers of the masses (m)
g=F/m=GM/r²
(D.1 Gravitational fields)
This gives the gravitational field strength at a point due to a mass M
g: Gravitational field strength
F: Gravitational force (N)
m: Mass experiencing the force
G: Gravitational constant
M: Mass creating the field (kg)
r: Distance from the center of M (m)
Ep=−Gm₁m₂/r
(D.1 Gravitational fields)
Gravitational potential energy
Ep: Gravitational potential energy (J)
G: Gravitational constant
m1,m2: Masses of the two objects (kg)
r: Distance between the centers of the masses (m)
Vg=−GM/r
(D.1 Gravitational fields)
Gravitational potential
Vg: Gravitational potential (J/kg)
G: Gravitational constant
M: Mass creating the potential (kg)
r: Distance from the center of M (m)
g=−ΔVg/Δr
(D.1 Gravitational fields)
Gravitational potential gradient
g: Gravitational field strength (N/kg)
ΔVg: Change in gravitational potential (J/kg)
Δr: Change in distance (m)
W=mΔVg
(D.1 Gravitational fields)
Work done in moving a mass
W: Work done (J)
m: Mass being moved (kg)
ΔVg: Change in gravitational potential (J/kg)
vesc=√(2GM/r)
(D.1 Gravitational fields)
The speed needed to escape the gravitational pull of a mass
vesc: Escape velocity (m/s)
G: Gravitational constant
M: Mass being escaped from (kg)
r: Distance from the center of M (m)
vorbital=√(GM/r)
(D.1 Gravitational fields)
Obrital speed of smaller mass/speed required to maintain a stable circular orbit.
vorbital: Orbital velocity (m/s)
G: Gravitational constant
M: Mass being orbited (kg)
r: Orbital radius (m)
F=k×(q₁q₂/r²)
(D.2 Electric and Magnetic Fields)
Electric force between two charges
F: Electric force between charges (N)
k: Coulomb's constant
q1,q2: Magnitudes of the charges (C)
r: Distance between the charges (m)
E=F/q
(D.2 Electric and Magnetic Fields)
electric field strength of a charge
E: Electric field strength (N/C)
F: Electric force on the charge (N)
q: Magnitude of the charge (C)
E=V/d
(D.2 Electric and Magnetic Fields)
Electric field strength between plates
E: Electric field strength (N/C)
V: Electric potential difference (V)
d: Separation between the plates (m)
Ep=k×(q₁q₂/r)
(D.2 Electric and Magnetic Fields)
potential energy
between two point charges.
Ep: Electric potential energy (J)
k: Coulomb's constant
q1,q2: Magnitudes of the charges (C)
r: Distance between the charges (m)
Ve=k×(Q/r)
(D.2 Electric and Magnetic Fields)
calculates the electric potential at a distance r from a point charge.
Ve: Electric potential (V)
k: Coulomb's constant
Q: Charge creating the potential (C)
r: Distance from the charge (m)
E=−ΔVe/Δr
(D.2 Electric and Magnetic Fields)
Electric potential gradient
E: Electric potential gradient (V/m)
ΔVe: Change in electric potential (V)
Δr: Change in distance (m)
W=qΔVe
(D.2 Electric and Magnetic Fields)
work done in moving a charge.
W: Work done on the charge (J)
q: Magnitude of the charge (C)
ΔVe: Change in electric potential (V)
F=qvBsinθ
(D.3 Motion in electromagnetic fields)
magnetic force acting on a charged particle moving through a magnetic field.
F: Magnetic force on the charge (N)
q: Magnitude of the charge (C)
v: Velocity of the charge (m/s)
B: Magnetic field strength (T)
θ: Angle between v and B (degrees or radians)
F=BILsinθ
(D.3 Motion in electromagnetic fields)
The force on a current-carrying conductor in a magnetic field.
F: Magnetic force on the wire (N)
B: Magnetic field strength (T)
I: Current through the wire (A)
L: Length of the wire in the field (m)
θ: Angle between the wire and magnetic field (degrees or radians)
F/L=μ₀×(I₁I₂/2πr)
(D.3 Motion in electromagnetic fields)
Force between two parallel wires carrying currents.
F: Magnetic force between two parallel current-carrying wires (N)
μ0: Permeability of free space
I1,I2: Currents in the two wires (A)
r: Distance between the wires (m)
L: Length of the wires (m)
E=hf
(E.1 Structure of the Atom)
E: Energy of a photon (J)
h: Planck's constant
f: Frequency of the photon (Hz)
E=mc²
(E.3 Radioactive Decay)
mass-energy equivalence
E: Energy released (J)
m: Mass lost (kg)
c: Speed of light in a vacuum
R=R₀A¹/³
(E.1 Structure of the Atom)
the radius of a nucleus
R: Radius of a nucleus (m)
R0: Fermi radius constant
A: Mass number (number of nucleons)
En=−13.6/n² eV
(E.1 Structure of the Atom)
Photon energy at a energy level
En: Energy of an electron in the nth energy level (eV)
n: number of level (1,2,3..)
mvr=nh/2π
(E.1 Structure of the Atom)
Angular momentum for an electron in an atom
Angular momentum: mvr
m: Mass of the electron (kg)
v: Speed of the electron (m/s)
r: Radius of the orbit (m)
n: Principal quantum number (integer): energy level or shell an electron is in around an atom
h: Planck's constant
N=N₀e (to the power of) −λt
(E.3 Radioactive Decay)
Number of undecayed nuclei
N: Number of undecayed nuclei at time t
N0: Initial number of nuclei
λ: Decay constant (s-1)
t: Time (s)
A=λN
A=λN₀ (to the power of) −λt
(E.3 Radioactive Decay)
Activity of a radioactive sample
A: Activity of the sample (Bq)
λ: Decay constant (s−1)
N: Number of undecayed nuclei
N0: Initial number of nuclei
t: Time (s)
T½=ln2/λ
(E.3 Radioactive Decay)
Half-life of a sample
T½: Half-life (s)
λ: Decay constant (s−1)
Emax=hf−Φ
(E.2 Quantum Physics)
Kinetic energy of freed electron (photoelectric effect)
Emax: Maximum kinetic energy of emitted photoelectron (J)
h: Planck's constant (Js)
f: Frequency of incident radiation (Hz)
Φ: Work function of the material (J)
hf: Energy of photon
λ=h/p
(E.2 Quantum Physics)
λ: De Broglie wavelength (m)
h: Planck's constant (Js)
p: Momentum of the particle (kg·m/s)
λf−λi=h/mc(1−cosθ)
The change in wavelength of a photon due to Compton scattering— when a photon collides with and transfers energy to an electron.
λf: Final wavelength of the photon (m)
λi: Initial wavelength (m)
h: Planck's constant (Js)
me: Electron mass (kg)
c: Speed of light (m/s)
θ: Scattering angle (radians or degrees)
d(parsec)=1/p(arc-second)
(E.5 Fusion and Star)
The distance to a star in parsecs
d: distance to star
p: parallax angle
Φ=BAcosθ
(D.4 Induction)
Calculates Magnetic flux, or the amount of magnetic field passing through an area.
Φ: Magnetic flux (Wb)
B: Magnetic field strength (T)
A: Area perpendicular to the field (m²)
θ: Angle between the magnetic field and the normal to the surface
ε=−N×ΔΦ/Δt
(D.4 Induction)
The induced EMF (electromotive force) in a coil of wire.
ε: Induced EMF (V)
N: Number of turns in the coil
ΔΦ: Change in magnetic flux (Wb)
Δt: Time interval (s)
ε=BvL
The induced EMF in a straight conductor moving in a magnetic field.
ε: Induced EMF (V)
B: Magnetic field strength (T)
v: Speed of the conductor (m/s)
L: Length of conductor within the field (m)
τ=Frsinθ
(A.4 Rigid Body Mechanics)
The torque applied by a force around a pivot point.
τ: Torque (N·m)
F: Applied force (N)
r: Distance from axis to point of force application (m)
θ: Angle between force and lever arm
Δθ=((ωf+ωi)/2)×t
ωf=ωi+αt
Δθ=ωi×t+½αt²
ωf²=ωi²+2αΔθ
Angular version of SUVAT equations
(A.4 Rigid Body Mechanics)
Δθ: Angular displacement (rad)
ωi: Initial angular velocity (rad/s)
ωf: Final angular velocity (rad/s)
α: Angular acceleration (rad/s²)
t: Time (s)
I=∑mr²
(A.4 Rigid Body Mechanics)
Moment of inertia
I: Moment of inertia (kg·m²)
m: Mass of each particle (kg)
r: Distance from rotation axis (m)
τ=Iα
(A.4 Rigid Body Mechanics)
Torque required to produce angular acceleration.
τ: Torque (N·m)
I: Moment of inertia (kg·m²)
α: Angular acceleration (rad/s²)
L=Iω
(A.4 Rigid Body Mechanics)
Angular momentum of a rotating body.
L: Angular momentum (kg·m²/s)
I: Moment of inertia (kg·m²)
ω: Angular velocity (rad/s)
ΔL=τΔt
(A.4 Rigid Body Mechanics)
Angular impulse
τ: Torque (N·m)
ΔL: Change in angular momentum (kg·m²/s)
Δt: Time interval (s)