Physics equations/Equations
Physics equationsEdit
00Mathematics for this courseEdit
Measured in radians, defines angle (in radians), where s is arclength and r is radius. The circumference of a circle is and the circle's area is is its area. The surface area of a sphere is and sphere's volume is
A vector can be expressed as, , where , and are the x and y components. Alternative notation for the unit vectors include and . An important vector is the displacement from the origin, with components are typically written without subscripts: . The magnitude (or absolute value or norm) of a vector is is , where the angle (or phase), , obeys , or (almost) equivalently, . As with any function/inverse function pair, the tangent and arctangent are related by where . The arctangent is not a true function because it is multivalued, with .
The geometric interpretations of and are shown in the figure. Vector addition and subtraction can also be defined through the components: AND
01IntroductionEdit

 1 kilometer = .621 miles and 1 MPH = 1 mi/hr ≈ .447 m/s
 Typically air density is 1.2kg/m^{3}, with pressure 10^{5}Pa. The density of water is 1000kg/m^{3}.
 Earth's mean radius ≈ 6371km, mass ≈ 6×10^{24}
_{} kg, and gravitational acceleration = g ≈ 9.8m/s^{2}  Universal gravitational constant = G ≈ 6.67×10^{−11}
_{} m^{3}·kg^{−1}·s^{−2}  Speed of sound ≈ 340m/s and the speed of light = c ≈ 3×10^{8}m/s
 One lightyear ≈ 9.5×10^{15}m ≈ 63240AU (Astronomical unit)
 The electron has charge, e ≈ 1.6 × 10^{−19}C and mass ≈ 9.11 × 10^{31}kg. 1eV = 1.602 × 10^{19}J is a unit of energy, defined as the work associated with moving one electron through a potential difference of one volt.
 1 amu = 1 u ≈ 1.66 × 10^{27} kg is the approximate mass of a proton or neutron.
 Boltzmann's constant = k_{B}≈ 1.38 × 10^{23} J K^{−1} , and the gas constant is R = N_{A}k_{B}≈8.314 J K^{−1} mol^{−1}, where N_{A}≈ 6.02 × 10^{23} is the Avogadro number.
 ≈ 8.987× 10^{9} N·m²·C^{−2} is a fundamental constant of electricity; also ≈ 8.854 × 10^{−12} F·m^{−1} is the vacuum permittivity or the electric constant.
 = 4π × 10^{−7} NA ≈ 1.257 × 10^{−6} N A (magnetic permeability) is the fundamental constant of magnetism: .
 = h/(2π) ≈ 1.054×10^{−34} J·s the reduced Planck constant, and ≈ .526 × 10^{−10} m is the Bohr radius.
02One dimensional kinematicsEdit
Difference is denoted by , , or the Delta. or . Average, or mean, is denoted by , where is number and are probabilities. The average velocity is , and the average acceleration is , where denotes position. In CALCULUS, instantaneous values are denoted by v(t)=dx/dt and a=dv/dt=d^{2}x/dt^{2}.
The equations of motion for uniform acceleration are: , and, . Also, , and, . Note that only if the acceleration is uniform.
03TwoDimensional KinematicsEdit
...in advanced notation this becomes .
In free fall we often set, a_{x}=0 and a_{y}= g. If angle is measured with respect to the x axis:
The figure shows a Man moving relative to Train with velocity, , where the velocity of the train relative to Earth is, is the velocity of the Train relative to Earth. The velocity of the Man relative to Earth is,
If the speeds are relativistic, define u=v/c where c is the speed of light, and this formula must be modified to:
04Dynamics: Force and Newton's LawsEdit
Newton's laws of motion, can be expressed with two equations, and . The second represents the fact that the force that the ith object exerts one object exerts on the jth object is equal and opposite the force that the jth exerts on the ith object. Three nonfundamental forces are:
 The normal force, , is a contact forces that is perpendicular to the surface,
 The force of friction, , is a contact force that is parallel to the surface.
 Tension, , is often associated with ropes and strings. If the rope has sufficiently low weight and of all external forces act at the two ends, then this tension is distributed uniformly along the rope.
 The fourth force is fundamental: Weight equals , and is the force of gravity acting on an object of mass, . At Earth's surface, .
The x and y components of the three forces of tension on the small grey circle where the three "massless" ropes meet are:
 ,
 ,
 ,
05Friction, Drag, and ElasticityEdit
 is an approximation for the force friction when an object is sliding on a surface, where μ_{k} ("mewsubk") is the kinetic coefficient of friction, and N is the normal force.
 approximates the maximum possible friction (called static friction) that can occur before the object begins to slide. Usually μ_{s} > μ_{k}. Also, air drag often depends on speed, an effect this model fails to capture.
06Uniform Circular Motion and GravitationEdit
 relates the radian, degree, and revolution.
 is the number of revolutions per second, called frequency.
 is the number of seconds per revolution, called period. Obviously .
 is called angular frequency (ω is called omega, and θ is measured in radians). Obviously
 is the acceleration of uniform circular motion, where v is speed, and r is radius.
 , where T is period.
 is the force of gravity between two objects, where the universal constant of gravity is G ≈ 6.674 × 10^{11} m^{3}·kg^{−1}·s^{−2}.
07Work and EnergyEdit
 is kinetic energy, where m is mass and v is speed..
 is gravitational potential energy,where y is height, and is the gravitational acceleration at Earth's surface.
 is the potential energy stored in a spring with spring constant .
 relates the final energy to the initial energy. If energy is lost to heat or other nonconservative force, then Q>0.
 (measured in Joules) is the work done by a force as it moves an object a distance . The angle between the force and the displacement is θ.
 describes the work if the force is not uniform. The steps, , taken by the particle are assumed small enough that the force is approximately uniform over the small step. If force and displacement are parallel, then the work becomes the area under a curve of F(x) versus x.
 is the power (measured in Watts) is the rate at which work is done. (v is velocity.)
08Linear Momentum and CollisionsEdit
 is momentum, where m is mass and is velocity. The net momemtum is conserved if all forces between a system of particles are internal (i.e., come equal and opposite pairs):
 .
 is the impulse, or change in momentum associated with a brief force acting over a time interval . (Strictly speaking, is a timeaveraged force defined by integrating over the time interval.)
09Statics and TorqueEdit
 is the torque caused by a force, F, exerted at a distance ,r, from the axis. The angle between r and F is θ.
The SI units for torque is the newton metre (N·m). It would be inadvisable to call this a Joule, even though a Joule is also a (N·m). The symbol for torque is typically τ, the Greek letter tau. When it is called moment, it is commonly denoted M.^{[1]} The lever arm is defined as either r, or r_{⊥}. Labeling r as the lever arm allows moment arm to be reserved for r_{⊥}.
10Rotational Motion and Angular MomentumEdit
Linear motion  Angular motion 

The following table refers to rotation of a rigid body about a fixed axis: is arclength, is the distance from the axis to any point, and is the tangential acceleration, which is the component of the acceleration that is parallel to the motion. In contrast, the centripetal acceleration, , is perpendicular to the motion. The component of the force parallel to the motion, or equivalently, perpendicular, to the line connecting the point of application to the axis is . The sum is over particles or points of application.
Linear motion  Rotational motion  Defining equation 

Displacement =  Angular displacement =  
Velocity =  Angular velocity =  
Acceleration =  Angular acceleration =  
Mass =  Moment of Inertia =  
Force =  Torque =  
Momentum=  Angular momentum=  
Kinetic energy =  Kinetic energy = 
Description^{[3]}  Figure  Moment(s) of inertia 

Rod of length L and mass m (Axis of rotation at the end of the rod) 

Solid cylinder of radius r, height h and mass m   
Sphere (hollow) of radius r and mass m  
Ball (solid) of radius r and mass m 
11Fluid staticsEdit
Pressure versus Depth: A fluid's pressure is F/A where F is force and A is a (flat) area. The pressure at depth, below the surface is the weight (per area) of the fluid above that point. As shown in the figure, this implies:
where is the pressure at the top surface, is the depth, and is the mass density of the fluid. In many cases, only the difference between two pressures appears in the final answer to a question, and in such cases it is permissible to set the pressure at the top surface of the fluid equal to zero. In many applications, it is possible to artificially set equal to zero, for example at atmospheric pressure. The resulting pressure is called the gauge pressure, for below the surface of a body of water.
Buoyancy and Archimedes' principle Pascal's principle does not hold if two fluids are separated by a seal that prohibits fluid flow (as in the case of the piston of an internal combustion engine). Suppose the upper and lower fluids shown in the figure are not sealed, so that a fluid of mass density comes to equilibrium above and below an object. Let the object have a mass density of and a volume of , as shown in the figure. The net (bottom minus top) force on the object due to the fluid is called the buoyant force:
 ,
and is directed upward. The volume in this formula, AΔh, is called the volume of the displaced fluid, since placing the volume into a fluid at that location requires the removal of that amount of fluid. Archimedes principle states:
 A body wholly or partially submerged in a fluid is buoyed up by a force equal to the weight of the displaced fluid.
Note that if , the buoyant force exactly cancels the force of gravity. A fluid element within a stationary fluid will remain stationary. But if the two densities are not equal, a third force (in addition to weight and the buoyant force) is required to hold the object at that depth. If an object is floating or partially submerged, the volume of the displaced fluid equals the volume of that portion of the object which is below the waterline.
12Fluid dynamicsEdit
 the volume flow for incompressible fluid flow if viscosity and turbulence are both neglected. The average velocity is and is the cross sectional area of the pipe. As shown in the figure, because is constant along the developed flow. To see this, note that the volume of pipe is along a distance . And, is the volume of fluid that passes a given point in the pipe during a time .
 is Bernoulli's equation, where is pressure, is density, and is height. This holds for inviscid flow.
13Temperature, Kinetic Theory, and Gas LawsEdit
 converts from Celsius to Kelvins, and converts from Celsius to Fahrenheit.
 is the ideal gas law, where P is pressure, V is volume, n is the number of moles and N is the number of atoms or molecules. Temperature must be measured on an absolute scale (e.g. Kelvins).
 N_{A}k_{B}=R where N_{A}= 6.02 × 10^{23} is the Avogadro number. Boltzmann's constant can also be written in eV and Kelvins: k_{B} ≈8.6 × 10^{5} eV/deg.
 is the average translational kinetic energy per "atom" of a 3dimensional ideal gas.
 is the rootmeansquare speed of atoms in an ideal gas.
 is the total energy of an ideal gas, where
14Heat and Heat TransferEdit
Here it is convenient to define heat as energy that passes between two objects of different temperature The SI unit is the Joule. The rate of heat trasfer, or is "power": 1 Watt = 1 W = 1J/s
 is the heat required to change the temperature of a substance of mass, m. The change in temperature is ΔT. The specific heat, c_{S}, depends on the substance (and to some extent, its temperature and other factors such as pressure). Heat is the transfer of energy, usually from a hotter object to a colder one. The units of specfic heat are energy/mass/degree, or J/(kgdegree).
 is the heat required to change the phase of a a mass, m, of a substance (with no change in temperature). The latent heat, L, depends not only on the substance, but on the nature of the phase change for any given substance. L_{F} is called the latent heat of fusion, and refers to the melting or freezing of the substance. L_{V} is called the latent heat of vaporization, and refers to evaporation or condensation of a substance.
 is rate of heat transfer for a material of area, A. The difference in temperature between two sides separated by a distance, d, is . The thermal conductivity, k_{c}, is a property of the substance used to insulate, or subdue, the flow of heat.
 is the power radiated by a surface of area, A, at a temperature, T, measured on an absolute scale such as Kelvins. The emissivity, , is 1 for a black body, and 0 for a perfectly reflecting surface. The StefanBoltzmann constant is .
15ThermodynamicsEdit
 Pressure (P), Energy (E), Volume (V), and Temperature (T) are state variables (state functionscalled state functions). The number of particles (N) can also be viewed as a state variable.
 Work (W), Heat (Q) are not state variables.
 , is the entropy of an ideal , monatomic gas. The constant is arbitrary only in classical (nonquantum) thermodynamics. Since it is a function of state variables, entropy is also a state function.
A point on a PV diagram define's the system's pressure (P) and volume (V). Energy (E) and pressure (P) can be deduced from equations of state: E=E(V,P) and T=T(V,P). If the piston moves, or if heat is added or taken from the substance, energy (in the form of work and/or heat) is added or subtracted. If the path returns to its original point on the PVdiagram (e.g., 12341 along the rectantular path shown), and if the process is quasistatic, all state variables (P, V, E, T) return to their original values, and the final system is indistinguishable from its original state.
The net work done per cycle is area enclosed by the loop. This work equals the net heat flow into the system, (valid only for closed loops).
Remember: Area "under" is the work associated with a path; Area "inside" is the total work per cycle.
 is the work done on a system of pressure P by a piston of voulume V. If ΔV>0 the substance is expanding as it exerts an outward force, so that ΔW<0 and the substance is doing work on the universe; ΔW>0 whenever the universe is doing work on the system.
 is the amount of heat (energy) that flows into a system. It is positive if the system is placed in a heat bath of higher temperature. If this process is reversible, then the heat bath is at an infinitesimally higher temperature and a finite ΔQ takes an infinite amount of time.
 is the change in energy (First Law of Thermodynamics).
CALCULUS: .
 In an isothermal expansion (contraction), temperature, T, is constant. Hence P=nRT/V and substitution yields,
16Oscillatory Motion and WavesEdit
 describes oscillatory motion with period (here we use the zerosubscript to denote constants that do not vary with time).
 . For example, .
 for a massspring system with mass, m, and spring constant, k_{s}.
 for a low amplitude pendulum of length, L, in a gravitational field, g.
 is the potential energy of a mass spring system.
Let describe position:
 , where is maximum velocity.
 , where , is maximum acceleration.
 , relates maximum force to maximum acceleration.
 is the total energy.
 CALCULUS: x(t) obeys the linear homogeneous differential equation (ODE),
 relates the frequency, f, wavelength, λ,and the the phase speed, v_{p} of the wave (also written as v_{w}) This phase speed is the speed of individual crests, which for sound and light waves also equals the speed at which a wave packet travels.
 describes the nth normal mode vibrating wave on a string that is fixed at both ends (i.e. has a node at both ends). The mode number, n = 1, 2, 3,..., as shown in the figure.
 Beat frequency: The frequency of beats heard if two closely space frequencies, and , are played is .
 Musical acoustics: Frequency ratios of 2/1, 3/2, 4/3, 5/3, 5/4, 6/5, 8/5 are called the (just) "octave", "fifth", "fourth", "majorsixth", "majorthird", "minorthird", and "minorsixth", respectively.
17Physics of HearingEdit
 is the the approximate speed near Earth's surface, where the temperature, T, is measured in Kelvins. A theoretical calculation is where for a semiclassical gas with degrees of freedom. For a diatomic gas such as Nitrogen, γ = 1.4.
 is the speed of a wave in a stretched string if is the tension and is the linear mass density (kilograms per meter).
18Electric charge and fieldEdit
 is Coulomb's law for the force between two charged particles separated by a distance r: k_{e}≈8.987×10^{9}N·m²·C^{−2}, and ε_{0}≈8.854×10^{−12} F·m^{−1}.
 is the electric force on a "test charge", q, where is the magnitude of the electric field situated a distance r from a charge, Q.
Consider a collection of particles of charge , located at points (called source points), the electric field at (called the field point) is:
 is the electric field at the field point, , due to point charges at the source points, , and points from source points to the field point.
CALCULUS supplement:
is the electric field due to distributed charge, where , and denote linear, surface, and volume density (or charge density), respectively.
Cartesian coordinates (x, y, z). Volume element: . Line element: . Three basic area elements: , or, , or, .
Cylindrical coordinates (ρ, φ, z): Volume element: . Line element: . Basic area elements: (side), and, (top end).
Spherical coordinates (r, θ, φ): Volume element: (if symmetry holds). Line element: . Basic area element of a sphere: , where dΩ is a solid angle.
19Electric Potential and Electric FieldEdit
 is the potential energy of a particle of charge, q, in the presence of an electric potential V.
 (measured in Volts) is the variation in electric potential as one moves through an electric field . The angle between the field and the displacement is θ. The electric potential, V, decreases as one moves parallel to the electric field.
 describes the electric potential if the field is not uniform.
 due to a set of charges at where .
 is the (equal and opposite) charge on the two terminals of a capacitor of capicitance, C, that has a voltage drop, V, across the two terminals.
 is the capacitance of a parallel plate capacitor with surface area, A, and plate separation, d. This formula is valid only in the limit that d^{2}/A vanishes. If a dielectric is between the plates, then ε>ε_{0}≈ 8.85 × 10^{−12} due to shielding of the applied electric field by dielectric polarization effects.
 is the energy stored in a capacitor.
 is the energy density (energy per unit volume, or Joules per cubic meter) of an electric field.
CALCULUS supplement
 is the gradient theorem.
 is the divergence theorem
Here, Ω is a (3dimensional) volume and ∂Ω is the boundary of the volume, which is a (twodimensional) surface. Also a surface is Σ, which, if open, has the boundary ∂Σ, which is a (onedimensional) curve.
 in the limit that the Riemann sum becomes an integral.
 where is the del operator.
 is Gauss's law for the surface integral of the electric field over any closed surface, and is the total charge inside that surface.
 is a useful variant if the medium is dielectric. D=εE is the electric displacement field. The permittivity, ε = (1+χ)ε_{0}, where ε_{0}≈ 8.85 × 10^{−12}, and the electric susceptibility, χ, represents the degree to which the medium can be polarized by an electric field. The free charge, Q_{free}, represents all charges except those represented by the susceptibility, χ.
20Electric Current, Resistance, and Ohm's LawEdit
 defines the electric current as the rate at which charge flows past a given point on a wire. The direction of the current matches the flow of positive charge (which is opposite the flow of electrons if electrons are the carriers.)
 is Ohm's Law relating current, I, and resistance, R, to the difference in voltage, V, between the terminals. The resistance, R, is positive in virtually all cases, and if R > 0, the current flows from larger to smaller voltage. Any device or substance that obeys this linear relation between I and V is called ohmic.
 relates the density (n), the charge(q), and the average drift velocity (v_{drift}) of the carriers. The area (A) is measured by imagining a cut across the wire oriented such that the drift velocity is perpendicular to the surface of the (imaginary) cut.
 expresses the resistance of a sample of ohmic material with a length (L) and area (A). The 'resistivity', ρ ("row"), is an intensive property of matter.
 Power is energy/time, measured in joules/second or J/s. Often called P (never p). It is measured in watts (W)
 Current is charge/time, measured in coulombs/second or C/s. Often called I or i. It is measured in amps or ampheres (A)
 Electric potential (or voltage) is energy/charge, measured in joules/coulomb or J/C. Often called V (sometimes E, emf, ). It is measured in volts (V)
 Resistance is voltage/current , measured in volts/amp or V/A. Often called R (sometimes r, Z) It is measured in Ohms (Ω).
 is the power dissipated as current flows through a resistor
21Circuits, Bioelectricity, and DC InstrumentsEdit
 and are Kirchoff's Laws^{[4]}
 for the voltage divider shown.
 Simple RC circuit^{[5]} The figure to the right depicts a capacitor being charged by an ideal voltage source. If, at t=0, the switch is thrown to the other side, the capacitor will discharge, with the voltage, V , undergoing exponential decay:
where V_{0} is the capacitor voltage at time t = 0 (when the switch was closed). The time required for the voltage to fall to is called the RC time constant and is given by
22MagnetismEdit
 is the force on a particle with charge q moving at velocity v with in the presence of a magnetic field B. The angle between velocity and magnetic field is θ and the force is perpeduclar to both velocity and magnetic field by the right hand rule.
 expresses this result as a cross product.
 is the force a straight wire segment of length carrying a current, I.
 expresses thus sum over many segments to model a wire.
 CALCULUS: In the limit that we have the integral, .
 Defining magnetic force and field without calculus:
 is the magnetic field at a distance r from an infinitely long wire carrying a current, where μ_{0} = 4π × 10^{−7} N A. This field points azimuthally around the wire in a direction defined by the right hand rule. Application of the force law on a current element, we have
 is the force between two long wires of length separated by a short distance . The currents are I_{1} and I_{2}, with the force being attractive if the currents are flowing in the same direction.
Cyclotron motion: For a particle moving perpendicular to B, we have cyclotron motion. Recall that for uniform circular motion, the acceleration is a=v^{2}/r, where r is the radius. Since sin θ =1, Newton's second law of motion (F=ma) yields,
Since, sin θ =0, for motion parallel to a magnetic field, particles in a uniform magnetic field move in spirals at a radius which is determined by the perpendicular component of the velocity:
Hall effect: The Hall effect occurs when the magnetic field, velocity, and electric field are mutually perpendicular. In this case, the electric and magnetic forces are aligned, and can cancel if qE=qvB (since sinθ = 1). Since both terms are porportional to charge, q, the appropriate ratio of electric to magnetic field for null net force depends only on velocity:
 ,
where we have used the fact that voltage (i.e. emf or potential) is related to the electric field and a displacement parallel to that field: ΔV = E Δs cosθ
CALCULUS supplement:
 and the volume integral , where is current density.
 is Ampere's law relating a closed integral involving magnetic field to the total current enclosed by that path.
23Electromagnetic Induction, AC Circuits, and Electrical TechnologiesEdit
 is a consequence of the magnetic force law as seen in the reference frame of a moving charged object, where E is the electric field perceived by an observer moving at velocity v in the presence of a magnetic vield, B. Also written as, E = vBsinθ, this can be used to derive Faraday's law of induction. (Here, θ is the angle between the velocity and the magnetic field.)
 is the magnetic flux, where θ is the angle between the magnetic field and the normal to a surface of area, A.
 is Faraday's law where t is time and N is the number of turns. The minus sign reminds us that the emf, or electromotive force, acts as a "voltage" that opposes the change in the magnetic field or flux.
24Electromagnetic WavesEdit
 is called the displacement current because it replaces the current density when using Ampère's circuital law to calculate the line integral of the magnetic field around a closed loop.
Maxwell's equations hold for all volumes and closed surfaces. In vacuum, electromagnetic waves travel at the speed, .
25Geometric OpticsEdit
relates the focal length f of the lens, the image distance S_{1}, and the object distance S_{2}. The figure depicts the situation for which (S_{1}, S_{2}, f) are all positive: (1)The lens is converging (convex); (2) The real image is to the right of the lens; and (3) the object is to the left of the lens. If the lens is diverging (concave), then f < 0. If the image is to the left of the lens (virtual image), then S_{2} < 0 .
27Wave OpticsEdit
 where describes the constructive interference associated with two slits in the Fraunhoffer (far field) approximation.
 where is the high frequency carrier and is the slowly varying envelope. Here,
 and . Consequently, the beat frequency heard when two tones of frequency and is .
 models the addition of two waves of equal amplitude but different path length, .
AstronomyEdit
MassRadiusDistanceEarthSunMoonEdit
 Earth's Radius: R_{⊕} ≈ 6.37x10^{6}m
 Earth's Mass: M_{⊕} ≈ 5.97×10^{24}kg
 Solar and Lunar radius and mass:
 Solar radius and mass: R_{☉}≈110R_{⊕} and M_{☉} ≈ 330,000M_{⊕}.
 Lunar radius and mass: R_{L} ≈ 0.273R_{⊕} and M_{L} ≈ 0.0123M_{⊕}
 Earthmoon distance ≈ 60R_{⊕}
 EarthSun distance = 1AU ≈ 1.496x10^{11}m ≈ 23481R_{⊕}
 One lightyear ≈ 9.5×10^{15} m = 63240 AU
 One parsec ≈ 3.26 lightyears
^{[6]}
KeplerNewtonMassPeriodDistanceNormEdit
 , where P is the period of orbit in years, and a is the semimajor axis measured in AU. The net mass, , is the sum of the mass of both bodies, and is normalized to the mass of the Sun. For a planet of mass, , orbiting a star of much larger mass, , the normalized net mass is . The mass of the Sun, , is 1.99×10^{30} kilograms. If for some object, then that object is twice as massive as the Sun. One year is 3.15×10^{7} seconds.
AstrParallaxEdit
 , where D is the distance to the object in parsecs, θ is the parallax angle in arcseconds, and b is the baseline in AU; b=1 for observations taken from Earth. One degree is 60 arcminutes and one arcminute is 60 arseconds. One AU ≈ 1.5x10^{11} meters, and one parsec ≈ 3.26 lightyears, and one lightyear ≈ 9.5×10^{15} meters.
AstrInverseSquareEdit
 is a "normalized intensity", closely related to relative magnitude, that allows students to combine equations and solve problems without resorting to the logarithmic magnitude scale. If the distance to the stellar object, D, is measured in parsecs, it is the power per square parsec that enters a telescope on Earth. The luminosity, , (in solar units) is a measure of the absolute magnitude. In general, is the inversesquare law.
PhotonsWavesParticlesEdit
 is the energy of a photon, where f is frequency and h ≈6.6×10^{34}m^{2}kg/s is Plank's constant, and c ≈3×10^{8}m/s is the speed of light. Also, E=ℏ ω where ℏ ≈1.05×10m^{2}kg/s and ω =2π f.
 relates frequency, wavelength, and the speed (or phase velocity). Using wavenumber, k =2π/λ, this can also be represented as ω =ck.
AstrBlackbodyEdit
 is Wein's law that relates the peak emission wavelength, λ_{max}, of a black body to temperature, T measured in Kelvins. Peak wavelength, λ_{max}, is measured in nanometers (1nm=10^{9}m). If temperature is measured in units normalized to the Sun's temperature, , then
 where is the temperature normalized to the Sun's temperature.
The StefanBoltzmann law is usually written as P=σAT^{4}, where A is surface area, T is temperature (in Kelvins), and σ is the StefanBoltzmann constant. The power, P, can be written as normalized luminosity, , where L_{☉} =3.85×10^{26}W is the power output (or luminosity) of the Sun. In these normalized units, the StefanBoltzmann law is:
 , where is the radius and temperature normalized to the Sun's radius and is the temperature normalized to the Sun's temperature.
Hidden chapters from openstax PhysicsEdit
===28Special Relativity=== <section begin=28Special_Relativity/> *foo <section end=28Special_Relativity/> ===29Introduction to Quantum Physics=== <section begin=29Introduction_to_Quantum_Physics/> *foo <section end=29Introduction_to_Quantum_Physics/> ===30Atomic Physics=== <section begin=30Atomic_Physics/> *foo <section end=30Atomic_Physics/> ===31Radioactivity and Nuclear Physics=== <section begin=31Radioactivity_and_Nuclear_Physics/> *foo <section end=31Radioactivity_and_Nuclear_Physics/> ===32Medical Applications of Nuclear Physics=== <section begin=32Medical_Applications_of_Nuclear_Physics/> *foo <section end=32Medical_Applications_of_Nuclear_Physics/> ===33Particle Physics=== <section begin=33Particle_Physics/> *foo <section end=33Particle_Physics/> ===34Frontiers of Physics=== <section begin=34Frontiers_of_Physics/> *foo <section end=34Frontiers_of_Physics/>
 ↑ https://en.wikipedia.org/w/index.php?title=Torque&oldid=582917749
 ↑ "Linear Motion vs Rotational motion" (PDF).
 ↑ https://en.wikipedia.org/w/index.php?title=List_of_moments_of_inertia&oldid=582953751
 ↑ https //en.wikipedia.org/w/index.php?title=Kirchhoff%27s_circuit_laws&oldid=579357795
 ↑ From https://en.wikipedia.org/w/index.php?title=RC_circuit&oldid=598786790
 ↑ Taken from Google, Orbit of the Moon.