Electric field

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An electric field is a force field that surrounds electric charges that attracts or repels other electric charges. Mathematically the electric field is a vector field that associates to each point in space the force, called the Coulomb force, that would be experienced per unit of charge, by an infinitesimal test charge at that point. Electric fields are created by electric charges, and by time-varying magnetic fields. Electric fields are important in many areas of physics, and are exploited practically in electrical technology. On a microscopic scale, the electric field is responsible for the attractive force between the atomic nucleus and electrons that holds atoms together, and the forces between atoms that cause chemical bonding. The electric field and the magnetic field together form the electromagnetic force, one of the four fundamental forces of nature.

Video Electric field

Definition of an electric field

An electric charge, such as an electron, creates and is surrounded by an electric force field. This field will exert a force, either repulsive or attractive, on any other electric charge placed in its vicinity. The electric field ${\displaystyle \mathbf {E(x)} }$ at a point ${\displaystyle \mathbf {x} }$ is defined as the (vector) force, ${\displaystyle \mathbf {F} }$, that would be exerted on a stationary test particle of unit positive charge placed at that point. The force on a particle of charge ${\displaystyle q}$ will be, given by:${\displaystyle \mathbf {F} =q\mathbf {E} }$. with SI units of newtons per coulomb (N?C^-1) or, equivalently, volts per metre (V?m^-1), which in terms of SI base units are kg?m?s^-3?A^-1. If the charge is moving, there is a second force field to consider: the magnetic field. The force on a test charge from both fields combined is called the Lorentz force.

Maps Electric field

Sources of electric field

Causes and description

Electric fields are caused by electric charges, described by Gauss's law, or varying magnetic fields, described by Faraday's law of induction. Together, these laws are enough to define the behavior of the electric field as a function of charge repartition and magnetic field. However, since the magnetic field is described as a function of electric field, the equations of both fields are coupled and together form Maxwell's equations that describe both fields as a function of charges and currents.

In the special case of a steady state (stationary charges and currents), the Maxwell-Faraday inductive effect disappears. The resulting two equations (Gauss's law ${\displaystyle \nabla \cdot \mathbf {E} ={\frac {\rho }{\varepsilon _{0}}}}$ and Faraday's law with no induction term ${\displaystyle \nabla \times \mathbf {E} =0}$), taken together, are equivalent to Coulomb's law, written as ${\displaystyle {\boldsymbol {E}}({\boldsymbol {r}})={1 \over 4\pi \varepsilon _{0}}\int \rho ({\boldsymbol {r'}}){{\boldsymbol {r}}-{\boldsymbol {r'}} \over |{\boldsymbol {r}}-{\boldsymbol {r'}}|^{3}}d^{3}r'}$ for a charge density ${\displaystyle \mathbf {\rho } (\mathbf {r} )}$ (${\displaystyle \mathbf {r} }$ denotes the position in space). Notice that ${\displaystyle \varepsilon _{0}}$, the permitivity of vacuum, must be substituted if charges are considered in non-empty media.

Continuous vs. discrete charge representation

The equations of electromagnetism are best described in a continuous description. However, charges are sometimes best described as discrete points; for example, some models may describe electrons as point sources where charge density is infinite on an infinitesimal section of space.

A charge ${\displaystyle q}$ located at ${\displaystyle \mathbf {r_{0}} }$ can be described mathematically as a charge density ${\displaystyle \rho (\mathbf {r} )=q\delta (\mathbf {r-r_{0}} )}$, where the Dirac delta function (in three dimensions) is used. Conversely, a charge distribution can be approximated by many small point charges.

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Superposition principle

Electric fields satisfy the superposition principle, because Maxwell's equations are linear. As a result, if ${\displaystyle \mathbf {E} _{1}}$ and ${\displaystyle \mathbf {E} _{2}}$ are the electric fields resulting from distribution of charges ${\displaystyle \rho _{1}}$ and ${\displaystyle \rho _{2}}$, a distribution of charges ${\displaystyle \rho _{1}+\rho _{2}}$ will create an electric field ${\displaystyle \mathbf {E} _{1}+\mathbf {E} _{2}}$; for instance, Coulomb's law is linear in charge density as well.

This principle is useful to calculate the field created by multiple point charges. If charges ${\displaystyle q_{1},q_{2},...,q_{n}}$ are stationary in space at ${\displaystyle \mathbf {r} _{1},\mathbf {r} _{2},...\mathbf {r} _{n}}$, in the absence of currents, the superposition principle proves that the resulting field is the sum of fields generated by each particle as described by Coulomb's law:

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

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Electrostatic fields

Electrostatic fields are E-fields which do not change with time, which happens when charges and currents are stationary. In that case, Coulomb's law fully describes the field.

Electric potential

If a system is static, such that magnetic fields are not time-varying, then by Faraday's law, the electric field is curl-free. In this case, one can define an electric potential, that is, a function ${\displaystyle \Phi }$ such that ${\displaystyle \mathbf {E} =-\nabla \Phi }$. This is analogous to the gravitational potential.

Parallels between electrostatic and gravitational fields

Coulomb's law, which describes the interaction of electric charges:

${\displaystyle \mathbf {F} =q\left({\frac {Q}{4\pi \varepsilon _{0}}}{\frac {\mathbf {\hat {r}} }{|\mathbf {r} |^{2}}}\right)=q\mathbf {E} }$

is similar to Newton's law of universal gravitation:

${\displaystyle \mathbf {F} =m\left(-GM{\frac {\mathbf {\hat {r}} }{|\mathbf {r} |^{2}}}\right)=m\mathbf {g} }$

(where ${\displaystyle \mathbf {\hat {r}} =\mathbf {\frac {r}{|r|}} }$).

This suggests similarities between the electric field E and the gravitational field g, or their associated potentials. Mass is sometimes called "gravitational charge" because of that similarity.

Electrostatic and gravitational forces both are central, conservative and obey an inverse-square law.

Uniform fields

A uniform field is one in which the electric field is constant at every point. It can be approximated by placing two conducting plates parallel to each other and maintaining a voltage (potential difference) between them; it is only an approximation because of boundary effects (near the edge of the planes, electric field is distorted because the plane does not continue). Assuming infinite planes, the magnitude of the electric field E is:

${\displaystyle E=-{\frac {\Delta \phi }{d}}}$

where ?? is the potential difference between the plates and d is the distance separating the plates. The negative sign arises as positive charges repel, so a positive charge will experience a force away from the positively charged plate, in the opposite direction to that in which the voltage increases. In micro- and nano-applications, for instance in relation to semiconductors, a typical magnitude of an electric field is in the order of 10⁶ V?m^-1, achieved by applying a voltage of the order of 1 volt between conductors spaced 1 µm apart.

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Electrodynamic fields

Electrodynamic fields are E-fields which do change with time, for instance when charges are in motion.

The electric field cannot be described independently of the magnetic field in that case. If A is the magnetic vector potential, defined so that ${\displaystyle \mathbf {B} =\nabla \times \mathbf {A} }$, one can still define an electric potential ${\displaystyle \Phi }$ such that:

${\displaystyle \mathbf {E} =-\nabla \Phi -{\frac {\partial \mathbf {A} }{\partial t}}}$

One can recover Faraday's law of induction by taking the curl of that equation

${\displaystyle \nabla \times \mathbf {E} =-{\frac {\partial (\nabla \times \mathbf {A} )}{\partial t}}=-{\frac {\partial \mathbf {B} }{\partial t}}}$

which justifies, a posteriori, the previous form for E.

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Energy in the electric field

The total energy per unit volume stored by the electromagnetic field is

${\displaystyle u_{EM}={\frac {\varepsilon }{2}}|\mathbf {E} |^{2}+{\frac {1}{2\mu }}|\mathbf {B} |^{2}}$

where ? is the permittivity of the medium in which the field exists, ${\displaystyle \mu }$ its magnetic permeability, and E and B are the electric and magnetic field vectors.

As E and B fields are coupled, it would be misleading to split this expression into "electric" and "magnetic" contributions. However, in the steady-state case, the fields are no longer coupled (see Maxwell's equations). It makes sense in that case to compute the electrostatic energy per unit volume:

${\displaystyle u_{ES}={\frac {1}{2}}\varepsilon |\mathbf {E} |^{2}\,,}$

The total energy U stored in the electric field in a given volume V is therefore

${\displaystyle U_{ES}={\frac {1}{2}}\varepsilon \int _{V}|\mathbf {E} |^{2}\,\mathrm {d} V\,,}$

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Further extensions

Definitive equation of vector fields

In the presence of matter, it is helpful to extend the notion of the electric field into three vector fields:

${\displaystyle \mathbf {D} =\varepsilon _{0}\mathbf {E} +\mathbf {P} \!}$

where P is the electric polarization - the volume density of electric dipole moments, and D is the electric displacement field. Since E and P are defined separately, this equation can be used to define D. The physical interpretation of D is not as clear as E (effectively the field applied to the material) or P (induced field due to the dipoles in the material), but still serves as a convenient mathematical simplification, since Maxwell's equations can be simplified in terms of free charges and currents.

Constitutive relation

The E and D fields are related by the permittivity of the material, ?.

For linear, homogeneous, isotropic materials E and D are proportional and constant throughout the region, there is no position dependence: For inhomogeneous materials, there is a position dependence throughout the material:

${\displaystyle \mathbf {D(r)} =\varepsilon \mathbf {E(r)} }$

For anisotropic materials the E and D fields are not parallel, and so E and D are related by the permittivity tensor (a 2nd order tensor field), in component form:

${\displaystyle D_{i}=\varepsilon _{ij}E_{j}}$

For non-linear media, E and D are not proportional. Materials can have varying extents of linearity, homogeneity and isotropy.

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See also

• Classical electromagnetism
• Field strength
• Signal strength in telecommunications
• Magnetism
• Teltron tube
• Teledeltos, a conductive paper that may be used as a simple analog computer for modelling fields

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References

  *Purcell, Edward; Morin, David (2010). ELECTRICITY AND MAGNETISM (3rd ed.). Cambridge University Press, New York. ISBN 978-1-107-01402-2. CS1 maint: Multiple names: authors list (link)   *Browne, Michael (2011). PHYSICS FOR ENGINEERING AND SCIENCE (2nd ed.). McGraw-Hill, Schaum, New York. ISBN 978-0-07-161399-6.   

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External links

• Electric field in "Electricity and Magnetism", R Nave - Hyperphysics, Georgia State University
• 'Gauss's Law' - Chapter 24 of Frank Wolfs's lectures at University of Rochester
• 'The Electric Field' - Chapter 23 of Frank Wolfs's lectures at University of Rochester
• MovingCharge.html - An applet that shows the electric field of a moving point charge
• Fields - a chapter from an online textbook
• Learning by Simulations Interactive simulation of an electric field of up to four point charges
• Java simulations of electrostatics in 2-D and 3-D
• Interactive Flash simulation picturing the electric field of user-defined or preselected sets of point charges by field vectors, field lines, or equipotential lines. Author: David Chappell

Source of article : Wikipedia