Physics Formulae/Electromagnetism Formulae

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Lead Article: Tables of Physics Formulae


This article is a summary of the laws, principles, defining quantities, and useful formulae in the analysis of Electromagnetism.


Laws of Electromagnetism

Maxwell's Equations

Below is the set in the differential and integral forms, each form is found to be equivalant by use of vector calculus. There are many ways to formulate the laws using scalar/vector potentails, tensors, geometric algebra, and numerous variations using different field vectors for the electric and magnetic fields.

Name Differential form Integral form
Gauss's law 𝐄=ρε0 V𝐄d𝐀=qencε0
Gauss's law for Magnetism 𝐁=𝟎 V𝐁d𝐀=0
Maxwell–Faraday Law
(Faraday's law of induction)
×𝐄=𝐁t V=S𝐄dπ₯=S𝐁td𝐀
Maxwell-Ampère Circuital law
(Ampere's Law with Maxwell's correction)
×𝐁=μ0(𝐉+ε0𝐄t)  S𝐁dπ₯=μ0S(𝐉+ε0𝐄t)d𝐀
Lorentz Electromagnetic

Force Law

𝐅=qe(𝐄+𝐯×𝐁)


The Field Vectors


Central to electromagnetism are the electric and magnetic field vectors. Often for free space (vacumm) only the familiar E and B fields need to be used; but for matter extra field vectors D, P, H, and M must be used to account for the electric and magnetic dipole incluences throughout the media (see below for mathematical definitions).


The electric field vectors are related by:
𝐃=ϵ0𝐄+𝐏
The magnetic field vectors are related by:
𝐁=μ0(𝐇+𝐌)


Interpretation of the Field Vectors


Intuitivley;

β€” the E and B (electric and magnetic flux densities) fields are the easiest to interpret; field strength is propotional to the amount of flux though cross sections of surface area, i.e. strength as a cross-section density.

β€” the P and M (electric polarization and magnetization respectivley) fields are related to the net polarization of the dipole moments thoughout the medium, i.e. how well they respond to an external field, and how the orientation of the dipoles can retain (or not) the field they set up in response to the external field.

β€” the D and H (electric displacement and magnetic intensity field) fields are the least clear to understand physically; they are introduced for convenient thoretical simplifications, but one could imagine they relate to the strength of the field along the flux lines, strength as a linear density along flux lines.


Hypothical Magnetic Monopoles


β€” As far as is known, there are no magnetic monopoles in nature, though some theories predict they could exist.

β€” The approach to introduce monopoles in equations is to define a magnetic pole strength, magnetic charge, or monopole charge (all synonomous), treating poles analogously to the electric charges.

β€” One pole would be north N (numerically positive by convention), the other south S (numerically negative). There are two units which can be used from the SI system for pole strength.

β€” Pole srength can be quantified into densities, currents and current densities, as electric charge is in the previous table, exactly in the same way.

Maxwell's Equations would become one of the columns in the table below, at least theoretically. Subscripts e are electric charge quantities; subscripts m are magnetic charge quantities.


Name Weber (Wb) Convention Ampere meter (A m) Convention
Gauss's Law 𝐄=ρe/ϵ0 𝐄=ρe/ϵ0
Gauss's Law for magnetism 𝐁=ρm 𝐁=μ0ρm
Faraday's Law of induction ×𝐄=𝐁t+𝐣m ×𝐄=𝐁t+μ0𝐣m
AmpΓ¨re's Law ×𝐁=μ0ϵ0𝐄t+μ0𝐣e ×𝐁=μ0ϵ0𝐄t+μ0𝐣e
Lorentz force equation 𝐅=qe(𝐄+𝐯×𝐁)+
+qmμ0(𝐁𝐯×(𝐄/c2))
𝐅=qe(𝐄+𝐯×𝐁)+
+qm(𝐁𝐯×(𝐄/c2))


They are consistent if no magnetic monopoles, since monopole quantities are then zero and the equations reduce to the original form of Maxwell's equations.

Pre-Maxwell Laws

These laws are not fundamental anymore, since they can be derived from Maxwell's Equations. Coulomb's Law can be found from Gauss' Law (electrostatic form) and the Biot-Savart Law can be deduced from Ampere's Law (magnetostatic form). Lenz' Law and Faraday's Law can be incorperated into the Maxwell-Faraday equation. Nonetheless they are still very effective for simple calculations, especially for highly symmetrical problems.


Coulomb's Law 𝐄=𝐅Q=q4πϵ0|𝐫|2𝐫^

For a non uniform charge distribution, this becomes:

𝐄=14πϵ0Vn𝐫ρndVn|𝐫|3

Biot-Savart Law 𝐁=μ04πCI(dπ₯×𝐫)|𝐫|3,
Lenz's law Induced current always opposes its cause.

Electric Quantities

Electric Charge and Current


Quantity (Common Name/s) (Common) Symbol/s Defining Equation SI Units Dimension
Elementary Charge Quantum e C = A s [I][T]
Quantized Electric Charge q q=ne C = A s [I][T]
Electric Charge (any amount) q C = A s [I][T]
Electric charge density of dimension n

(Vn = n-space)

n = 1 for linear mass density,

n = 2 for surface mass density,

n = 3 for volume mass density,

etc

linear charge density λ,

surface charge density σ,

volume charge density ρ,


no general symbol for

any dimension


n-space charge density:

ρn=nmxnx2x1=mVn

special cases are:

λ=mx

σ=2mx2x1=2mS

ρ=3mx3x2x1=mV

C m-n [I][T][L]-n
Total descrete charge Q Q=iqi C [I][T]
Total continuum charge Q

n-space charge density

Q=ρndnx=ρndx1dx2dxn

special cases are:

Q=λdx

Q=σdA=σdx1dx2

Q=ρdV=ρdx1dx2dx3


C [I][T]
Capacitance C C=qV F = C V-1
Electric Current I I=dqdt A [I]
Current Density 𝐉 𝐉=𝐀^IA A m-2 [I][L]-2
Displacement current Id Id=ϵ0ΦEt A [I]
Charge Carrier Drift Speed 𝐯d m s-1 [L][T]-1


Electric Fields


Quantity (Common Name/s) (Common) Symbol/s Defining Equation SI Units Dimension
Electric Field, Field Strength,

Flux Density, Potential Gradient

𝐄 𝐄=𝐅/q N C-1 = V m-1 [M][L][T]-3[I]-1
Electric Flux ΦE ΦE=S𝐄d𝐀 N m2 C-1 [M][L]3[T]-3[I]-1
Electric Permittivity ϵ ϵ=ϵrϵ0 F m-1
Dielectric constant,

Relative Permittivity

ϵr F m-1
Electric Displacement Field 𝐃 𝐃=𝐄ϵ C m-2 [I][T][L]-2
Electric Displacement Flux ΦD ΦD=S𝐃d𝐀 C [I][T]
Electric Dipole Moment vector 𝐩 𝐩=2q𝐚

𝐚 is the charge separation

directed from -ve to +ve charge

C m [I][T][L]
Electric Polarization 𝐏 𝐏=𝐩V C m-2 [I][T][L]-2
Absolute Electric Potential

relative to point r0

Theoretical: r0=

Practical: R0=Rearth

(Earth's radius)

ϕ,V V=Wrq=1qr𝐅d𝐫=r1r2𝐄d𝐫 V = J C-1
Electric Potential Difference ΔV ΔV=ΔWq=1qr1r2𝐅d𝐫=r1r2𝐄d𝐫
Electric Potential Energy U U=W J [M][L]2[T]2

Magnetic Quantities

Quantity (Common Name/s) (Common) Symbol/s Defining Equation SI Units Dimension
Magnetic Field, Field Strength,

Flux Density, Induction Field

𝐁 𝐅=q(𝐯×𝐁) T = N A-1 m-1
Magnetic Flux ΦB ΦB=S𝐁d𝐀 Wb = T m-2
Magnetic Permeability μ μ=μrμ0 H m-1
Relative Permeability μr H m-1
Magnetic Field Intensity,

(also confusingly the field strength)

𝐇 𝐇=𝐁μ
Magnetic Dipole Moment vector 𝐦 𝐦=NI𝐀

N is the number of turns of conductor

A m2 [I][L]2
Magnetization 𝐌 𝐌=𝐦V
Self Inductance L Two equivalent definitions are in fact possible:

L=NΦI

LIt=NV

H = Wb A-1
Mutual Inductance M Again two equivalent definitions are in fact possible:

MX=NΦYIX

MIYt=NVX

X,Y subscripts refer to two conductors mutually inducing

voltage/ linking magnetic flux though each other

H = Wb A-1


Electric Fields

Electrostatic Fields

Common corolaries from Couloumb's and Gauss' Law (in turn corolaries of Maxwell's Equations) for uniform charge distributions are summarized in the table below.


Uniform Electric Field accelerating a charged mass a=qEm
Point Charge 𝐄=q4πϵ0|𝐫|2𝐫^
At a point in a local

array of Point Charges

𝐄=𝐄i=14πϵ0iqi|𝐫i𝐫|2𝐫^i
Electric Dipole 𝐄|𝐩|2πϵ0z3𝐳^

|𝐫|>>|𝐚|

Line of a Charge 𝐄=λ2πϵ0|𝐫|𝐫^
Charged Ring 𝐄=qz4πϵ0(z2+R2)3/2𝐳^
Charged Conducting Surface 𝐄=σϵ0𝐧^
Charged Insulating Surface 𝐄=σ2ϵ0𝐧^
Charged Disk 𝐄=σ(1z)2ϵ0z2+R2𝐳^
Outside Spherical Shell r>=R 𝐄=q4πϵ0|𝐫|2𝐫^
Inside Spherical Shell r<R 𝐄=𝟎
Uniform Charge r<=R 𝐄=q|𝐫|4πϵ0R3𝐫^
Electric Dipole Potential Energy

in a uniform Electric Eield

U=𝐩𝐄
Torque on an Electric Dipole

in a uniform Electric Eield

τ=𝐩×𝐄
Electric Field Energy Density

Linear media (constant ϵ throughout)

u=ϵE22

For non-uniform fields and electric dipole moments, the electrostatic torque and potential energy are:

U=(𝐄d𝐩+𝐩d𝐄)


τ=(d𝐩×𝐄+𝐩×d𝐄)


Electric Potential and Electric Field


ΔV=r1r1𝐄d𝐫

V=𝐄

Electrostatic Potentials

Point Charge V=q4πϵ0r
Pair of Point Charges V=q1q24πϵ0r


Electrostatic Capacitances

Parallel Plates C=ϵ0Ad
Cylinder C=ϵ02πLln|ba|
Sphere C=4πϵ0baba
Isolated Sphere C=4πϵ0R
Capacitors Connected in Parallel Cnet=iCi
Capacitors Connected in Series 1Cnet=i1Ci
Capacitor Potential Energy U=q22C=CV22

Magnetic Fields

Magnetic Forces

Force on a Moving Charge

𝐅=q𝐯×𝐁


Force on a Current-Carrying Conductor

𝐅=Iπ₯×𝐁


Magnetostatic Fields

Common corolaries from the Biot-Savart Law and Ampere's Law (again corolaries of Maxwell's Equations) for steady (constant) current-carrying configerations are summarized in the table below.


For these types of current configerations, the magnetic field is easily evaluated using the Biot-Savart Law, containing the vector dπ₯×𝐫, which is also the direction of the magnetic field at the point evaluated.

For conveinence in the results below, let 𝐛=dπ₯×𝐫 be a unit binormal vector to π₯ and 𝐫, so that


𝐛^=dπ₯×𝐫|dπ₯×𝐫|


then 𝐛^ also the unit vector for the direction of the magnetic field at the point evaluated.

Hall Effect n=BIVle
Circulating Charged Particle q𝐯×𝐁=m|𝐯|2|𝐫|𝐫^
Infinite Line of Current 𝐁=μ0I2π|𝐫|𝐛^
Magnetic Field of a Ray 𝐁=μ0I4π|𝐫|
Center of a Circular Arc 𝐁=μ0Iϕ4π|𝐫|𝐛^
Infinitley Long Solenoid 𝐁=μ0nI𝐛^
Toroidal Inductors and Transformers 𝐁=μ0IN2π|𝐫|𝐛^
Current Carrying Coil 𝐁=μ2πz3𝐛^
Magnetic Dipole Potential Energy

in a uniform Magnetic Eield

U=𝐦𝐁
Torque on a Magnetic Dipole

in a uniform Magnetic Eield

τ=𝐦×𝐁

For non-uniform fields and magnetic moments, the magnetic potential energy and torque are:

U=(𝐁d𝐦+𝐦d𝐁)


τ=(d𝐦×𝐁+𝐦×d𝐁)

Magnetic Energy

Magnetic Energy for Linear Media

(μ constant at all points in meduim)

U=LI22
Magnetic Energy Density for Linear

Media (μ constant at all points in meduim)

u=B22μ

EM Induction

Self Induction of emf β„°L=LdIdt
Mutual Induction β„°1=MdI2dt,β„°2=MdI1dt
transformation of voltage VsNp=VpNs

IsNs=IpNp

Req=(NpNs)2R

Induced Magnetic Field

inside a circular capacitor

B=(μ0Id/2πR2)r
Induced Magnetic Field

outside a circular capacitor

B=μ0Id/2πrr

Maxwell's Equations

Electric Field

Magnetic Field

Electric Charge

Magnetic Monopoles

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