Classical electromagnetism or classical electrodynamics

8 min readMay 29, 2021

Classical electromagnetism or classical electrodynamics is a branch of theoretical physics that studies the interactions between electric charges and currents using an extension of the classical Newtonian model. The theory provides a description of electromagnetic phenomena whenever the relevant length scales and field strengths are large enough that quantum mechanical effects are negligible. For small distances and low field strengths, such interactions are better described by quantum electrodynamics.

Fundamental physical aspects of classical electrodynamics are presented in many texts, such as those by Feynman, Leighton and Sands,[1] Griffiths,[2] Panofsky and Phillips,[3] and Jackson.[4]

History[edit]

Main article: History of electromagnetism

The physical phenomena that electromagnetism describes have been studied as separate fields since antiquity. For example, there were many advances in the field of optics centuries before light was understood to be an electromagnetic wave. However, the theory of electromagnetism, as it is currently understood, grew out of Michael Faraday’s experiments suggesting an electromagnetic field and James Clerk Maxwell’s use of differential equations to describe it in his A Treatise on Electricity and Magnetism (1873). For a detailed historical account, consult Pauli,[5] Whittaker,[6] Pais,[7] and Hunt.[8]

Lorentz force[edit]

Main article: Lorentz force

The electromagnetic field exerts the following force (often called the Lorentz force) on charged particles:

{\displaystyle \mathbf {F} =q\mathbf {E} +q\mathbf {v} \times \mathbf {B} }

where all boldfaced quantities are vectors: F is the force that a particle with charge q experiences, E is the electric field at the location of the particle, v is the velocity of the particle, B is the magnetic field at the location of the particle.

The above equation illustrates that the Lorentz force is the sum of two vectors. One is the cross product of the velocity and magnetic field vectors. Based on the properties of the cross product, this produces a vector that is perpendicular to both the velocity and magnetic field vectors. The other vector is in the same direction as the electric field. The sum of these two vectors is the Lorentz force.

Although the equation appears to suggest that the electric and magnetic fields are independent, the equation can be rewritten in term of four-current (instead of charge) and a single electromagnetic tensor that represents the combined field ({\displaystyle F^{\mu \nu }}

{\displaystyle f_{\alpha }=F_{\alpha \beta }J^{\beta }.\!}

Electric field[edit]

Main article: Electric field

The electric field E is defined such that, on a stationary charge:

{\displaystyle \mathbf {F} =q_{0}\mathbf {E} }

where q0 is what is known as a test charge and F is the force on that charge. The size of the charge doesn’t really matter, as long as it is small enough not to influence the electric field by its mere presence. What is plain from this definition, though, is that the unit of E is N/C (newtons per coulomb). This unit is equal to V/m (volts per meter); see below.

In electrostatics, where charges are not moving, around a distribution of point charges, the forces determined from Coulomb’s law may be summed. The result after dividing by q0 is:

{\displaystyle \mathbf {E(r)} ={\frac {1}{4\pi \varepsilon _{0}}}\sum _{i=1}^{n}{\frac {q_{i}\left(\mathbf {r} -\mathbf {r} _{i}\right)}{\left|\mathbf {r} -\mathbf {r} _{i}\right|^{3}}}}

where n is the number of charges, qi is the amount of charge associated with the ith charge, ri is the position of the ith charge, r is the position where the electric field is being determined, and ε0 is the electric constant.

If the field is instead produced by a continuous distribution of charge, the summation becomes an integral:

{\displaystyle \mathbf {E(r)} ={\frac {1}{4\pi \varepsilon _{0}}}\int {\frac {\rho (\mathbf {r’} )\left(\mathbf {r} -\mathbf {r’} \right)}{\left|\mathbf {r} -\mathbf {r’} \right|^{3}}}\mathrm {d^{3}} \mathbf {r’} }

where {\displaystyle \rho (\mathbf {r’} )}

is the charge density and {\displaystyle \mathbf {r} -\mathbf {r’} }

is the vector that points from the volume element {\displaystyle \mathrm {d^{3}} \mathbf {r’} }

to the point in space where E is being determined.

Both of the above equations are cumbersome, especially if one wants to determine E as a function of position. A scalar function called the electric potential can help. Electric potential, also called voltage (the units for which are the volt), is defined by the line integral

{\displaystyle \varphi \mathbf {(r)} =-\int _{C}\mathbf {E} \cdot \mathrm {d} \mathbf {l} }

where φ(r) is the electric potential, and C is the path over which the integral is being taken.

Unfortunately, this definition has a caveat. From Maxwell’s equations, it is clear that ∇ × E is not always zero, and hence the scalar potential alone is insufficient to define the electric field exactly. As a result, one must add a correction factor, which is generally done by subtracting the time derivative of the A vector potential described below. Whenever the charges are quasistatic, however, this condition will be essentially met.

From the definition of charge, one can easily show that the electric potential of a point charge as a function of position is:

{\displaystyle \varphi \mathbf {(r)} ={\frac {1}{4\pi \varepsilon _{0}}}\sum _{i=1}^{n}{\frac {q_{i}}{\left|\mathbf {r} -\mathbf {r} _{i}\right|}}}

where q is the point charge’s charge, r is the position at which the potential is being determined, and ri is the position of each point charge. The potential for a continuous distribution of charge is:

{\displaystyle \varphi \mathbf {(r)} ={\frac {1}{4\pi \varepsilon _{0}}}\int {\frac {\rho (\mathbf {r’} )}{|\mathbf {r} -\mathbf {r’} |}}\,\mathrm {d^{3}} \mathbf {r’} }

where {\displaystyle \rho (\mathbf {r’} )}

is the charge density, and {\displaystyle \mathbf {r} -\mathbf {r’} }

is the distance from the volume element {\displaystyle \mathrm {d^{3}} \mathbf {r’} }

to point in space where φ is being determined.

The scalar φ will add to other potentials as a scalar. This makes it relatively easy to break complex problems down in to simple parts and add their potentials. Taking the definition of φ backwards, we see that the electric field is just the negative gradient (the del operator) of the potential. Or:

{\displaystyle \mathbf {E(r)} =-\nabla \varphi \mathbf {(r)} .}

From this formula it is clear that E can be e[9] xpressed in V/m (volts per meter).

https://vexare4629.medium.com/martin-morocky-born-31-march-1983-known-by-his-902c97847c76
https://arrabble.medium.com/mshasho-clothing-is-a-namibian-clothing-brand-founded-db8543163031
https://arrabble.medium.com/martin-morocky-born-31-march-1983-known-by-his-stage-name-as-the-dogg-646979461508
https://vexare4629.medium.com/namibian-music-awards-441b2392403b
https://vexare4629.medium.com/namibia-n%C9%99%CB%88m%C9%AAbi%C9%99-about-this-soundlisten-n%C3%A6%CB%88-16-17-officially-the-republic-of-namibia-e21df090d8c8
https://arrabble.medium.com/an-electromagnetic-field-also-em-field-is-a-classical-i-e-non-quantum-6fc1a608d934

Classical electromagnetism or classical electrodynamics

Contents

History[edit]

Lorentz force[edit]

Electric field[edit]

Written by Dedecab