Electromagnetic radiation
The
electromagnetic waves that compose electromagnetic radiation can be imagined as
a self-propagating transverse oscillating wave of electric and magnetic fields.
This diagram shows a plane linearly polarized EMR wave propagating from left to
right. The electric field is in a vertical plane and the magnetic field in a
horizontal plane. The two types of fields in EMR waves are always in phase with
each other, and no matter how powerful, have a ratio of electric to magnetic intensity
which is fixed and never varies.
Electromagnetic radiation (EM
radiation or EMR) is a form of energy emitted and absorbed by charged
particles, which exhibits wave-like behavior as it travels through space. EMR
has both electric
and magnetic field components,
which stand in a fixed ratio of intensity to each other, and which oscillate in phase
perpendicular to each other and perpendicular to the direction of energy and wave propagation. In vacuum, electromagnetic radiation
propagates at a characteristic speed, the speed of light.
Electromagnetic radiation is a particular form of the
more general electromagnetic
field (EM field), which is produced by moving charges.
Electromagnetic radiation is associated with EM fields that are far enough away
from the moving charges that produced them, that absorption of the EM radiation
no longer affects the behavior of these moving charges. These two types or
behaviors of EM field are sometimes referred to as the near
and far field. In this language, EMR is merely another name for the
far-field. Charges and currents directly produce the near-field. However,
charges and currents produce EMR only indirectly—rather, in EMR, both the
magnetic and electric fields are produced by changes in the other type of
field, not directly by charges and currents. This close relationship causes the
electric and magnetic fields in EMR to stand in a fixed ratio of strengths to
each other, and to be found in phase, with maxima and nodes in each found at
the same places in space.
EMR carries energy—sometimes
called radiant
energy—through space continuously away from the source (this is not
true of the near-field part of the EM field). EMR also carries both momentum and angular momentum. These
properties may all be imparted to matter
with which it interacts. EMR is produced from other types of energy when
created, and it is converted to other types of energy when it is destroyed. The
photon is the quantum of the
electromagnetic interaction, and is the basic "unit" or constituent
of all forms of EMR. The quantum nature of light becomes more apparent at high
frequencies (or high photon energy). Such photons behave more like particles
than lower-frequency photons do.
EMR is classified according to the frequency of its wave. The electromagnetic
spectrum, in order of increasing frequency and decreasing wavelength, consists of radio waves, microwaves, infrared
radiation, visible
light, ultraviolet
radiation, X-rays and gamma rays. The eyes of various organisms sense a small and
somewhat variable window of frequencies of EMR called the visible spectrum.
The effects of EMR upon biological systems (and also to
many other chemical systems, under standard conditions)
depends both upon the radiation's power and frequency. For lower frequencies of
EMR up to those of visible light (i.e., radio, microwave, infrared), the damage
done to cells and also to many ordinary materials under such conditions is
determined mainly by heating effects, and thus by the radiation power. By
contrast, for higher frequency radiations at ultraviolet frequencies and above
(i.e., X-rays and gamma rays) the damage to chemical materials and living cells
by EMR is far larger than that done by simple heating, due to the ability of
single photons in such high frequency EMR to damage individual molecules
chemically.
Properties of EM radiation
Electromagnetic waves can be imagined as a
self-propagating transverse oscillating wave of electric and magnetic fields.
This 3D diagram shows a plane linearly polarized wave propagating from left to
right
This 3D diagram shows a plane linearly
polarized wave propagating from left to right. Note that the electric and
magnetic fields in such a wave are in-phase with each other, reaching minima
and maxima together
The physics of electromagnetic
radiation is electrodynamics.
Electromagnetism is the physical
phenomenon associated with the theory of electrodynamics. Electric and magnetic
fields obey the properties of superposition.
Thus, a field due to any particular particle or time-varying electric or
magnetic field contributes to the fields present in the same space due to other
causes. Further, as they are vector
fields, all magnetic and electric field vectors add together according to
vector addition. For example, in optics two or more coherent lightwaves may
interact and by constructive or destructive interference yield a resultant
irradiance deviating from the sum of the component irradiances of the
individual lightwaves.Since light is an oscillation it is not affected by travelling through static electric or magnetic fields in a linear medium such as a vacuum. However in nonlinear media, such as some crystals, interactions can occur between light and static electric and magnetic fields — these interactions include the Faraday effect and the Kerr effect.
In refraction, a wave crossing from one medium to another of different density alters its speed and direction upon entering the new medium. The ratio of the refractive indices of the media determines the degree of refraction, and is summarized by Snell's law. Light of composite wavelengths (natural sunlight) disperses into a visible spectrum passing through a prism, because of the wavelength dependent refractive index of the prism material (dispersion); that is, each component wave within the composite light is bent a different amount.
EM radiation exhibits both wave properties and particle properties at the same time (see wave-particle duality). Both wave and particle characteristics have been confirmed in a large number of experiments. Wave characteristics are more apparent when EM radiation is measured over relatively large timescales and over large distances while particle characteristics are more evident when measuring small timescales and distances. For example, when electromagnetic radiation is absorbed by matter, particle-like properties will be more obvious when the average number of photons in the cube of the relevant wavelength is much smaller than 1. It is not too difficult to experimentally observe non-uniform deposition of energy when light is absorbed, however this alone is not evidence of "particulate" behavior of light. Rather, it reflects the quantum nature of matter.[1] Demonstrating that the light itself is quantized, not merely its interaction with matter, is a more subtle problem.A quantum theory of the interaction between electromagnetic radiation and matter such as electrons is described by the theory of quantum electrodynamics.
Wave model
Electromagnetic radiation is a transverse wave, meaning that the oscillations of the waves are perpendicular to the direction of energy transfer and travel. The electric and magnetic parts of the field stand in a fixed ratio of strengths in order to satisfy the two Maxwell equations that specify how one is produced from the other. These E and B fields are also in phase, with both reaching maxima and minima at the same points in space (see illustrations). A common misconception is that the E and B fields in electromagnetic radiation are out of phase because a change in one produces the other, and this would produce a phase difference between them as sinusoidal functions (as indeed happens in electromagnetic induction, and in the near-field close to antennas). However, in the far-field EM radiation which is described by the two source-free Maxwell curl operator equations, a more correct description is that a time-change in one type of field is proportional to a space-change in the other. These derivatives require that the E and B fields in EMR are in-phase (see math section below).An important aspect of the nature of light is frequency. The frequency of a wave is its rate of oscillation and is measured in hertz, the SI unit of frequency, where one hertz is equal to one oscillation per second. Light usually has a spectrum of frequencies that sum to form the resultant wave. Different frequencies undergo different angles of refraction.
A wave consists of successive troughs and crests, and the distance between two adjacent crests or troughs is called the wavelength. Waves of the electromagnetic spectrum vary in size, from very long radio waves the size of buildings to very short gamma rays smaller than atom nuclei. Frequency is inversely proportional to wavelength, according to the equation:
Interference is the superposition of two or more waves resulting in a new wave pattern. If the fields have components in the same direction, they constructively interfere, while opposite directions cause destructive interference.The energy in electromagnetic waves is sometimes called radiant energy.
Particle model and quantum theory
See also: Quantization
(physics) and Quantum optics
An anomaly that arose in the
late 19th century involved a contradiction between the wave theory of light and
measurements of the electromagnetic spectrum emitted by thermal radiators, or
so-called black bodies. Physicists struggled
with this problem, which later became known as the ultraviolet
catastrophe, unsuccessfully for many years. In 1900, Max Planck developed a new theory
of black-body radiation that explained the observed spectrum.
Planck's theory was based on the idea that black bodies emit light (and other
electromagnetic radiation) only as discrete bundles or packets of energy. These packets were called quanta. Later, Albert Einstein proposed that the
quanta of light might be regarded as real particles, and (still later) the
particle of light was given the name photon, to correspond with other particles being described
around this time, such as the electron
and proton. A photon has an energy, E,
proportional to its frequency, f, byLikewise, the momentum p of a photon is also proportional to its frequency and inversely proportional to its wavelength:
As a photon is absorbed by an atom, it excites the atom, elevating an electron to a higher energy level (on average, one that is farther from the nucleus). When an electron in an excited molecule or atom descends to a lower energy level, it emits a photon of light equal to the energy difference. Since the energy levels of electrons in atoms are discrete, each element and each molecule emits and absorbs its own characteristic frequencies. When the emission of the photon is immediate, this phenomenon is called fluorescence, a type of photoluminescence. An example is visible light emitted from fluorescent paints, in response to ultraviolet (blacklight). Many other fluorescent emissions in other spectral bands than visible, are known. When the emission of the photon is delayed, the phenomenon is called phosphorescence.
Speed of propagation
Main article: Speed of light
Any electric charge that
accelerates, or any changing magnetic field, produces electromagnetic
radiation. Electromagnetic information about the charge travels at the speed of
light. Accurate treatment thus incorporates a concept known as retarded time (as opposed to
advanced time, which is not physically possible in light of causality), which adds to the
expressions for the electrodynamic electric field and magnetic field. These extra terms
are responsible for electromagnetic radiation.When any wire (or other conducting object such as an antenna) conducts alternating current, electromagnetic radiation is propagated at the same frequency as the electric current. In many such situations it is possible to identify an electrical dipole moment that arises from separation of charges due to the exciting electrical potential, and this dipole moment oscillates in time, as the charges move back and forth. This oscillation at a given frequency gives rise to changing electric and magnetic fields, which then set the electromagnetic radiation in motion.
At the quantum level, electromagnetic radiation is produced when the wavepacket of a charged particle oscillates or otherwise accelerates. Charged particles in a stationary state do not move, but a superposition of such states may result in transition state which has an electric dipole moment that oscillates in time. This oscillating dipole moment is responsible for the phenomenon of radiative transition between quantum states of a charged particle. Such states occur (for example) in atoms when photons are radiated as the atom shifts from one stationary state to another.
Depending on the circumstances, electromagnetic radiation may behave as a wave or as particles. As a wave, it is characterized by a velocity (the speed of light), wavelength, and frequency. When considered as particles, they are known as photons, and each has an energy related to the frequency of the wave given by Planck's relation E = hν, where E is the energy of the photon, h = 6.626 × 10−34 J·s is Planck's constant, and ν is the frequency of the wave.
One rule is always obeyed regardless of the circumstances: EM radiation in a vacuum always travels at the speed of light, relative to the observer, regardless of the observer's velocity. (This observation led to Albert Einstein's development of the theory of special relativity.)
In a medium (other than vacuum), velocity factor or refractive index are considered, depending on frequency and application. Both of these are ratios of the speed in a medium to speed in a vacuum.
Derivation from electromagnetic theory
Main article: electromagnetic wave equation
Electromagnetic waves as a
general phenomenon were predicted by the classical laws of electricity and magnetism, known
as Maxwell's
equations. Inspection of Maxwell's equations without sources
(charges or currents) results in, along with the possibility of nothing
happening, nontrivial solutions of changing electric and magnetic fields.
Beginning with Maxwell's equations in free space:
where
is
a vector differential operator (see Del).
One solution,For a more useful solution, we utilize vector identities, which work for any vector, as follows:
where we simplified the above by
using equation (1).
Evaluate the right hand side:
|
|
where
c0 is the speed
of the wave in free space and
f describes a displacement
Or more simply:
where is d'Alembertian:
But these are only two equations and we started with four, so there is still more information pertaining to these waves hidden within Maxwell's equations. Let's consider a generic vector wave for the electric field.
This form will satisfy the wave equation, but will it satisfy all of Maxwell's equations, and with what corresponding magnetic field?
Not only are the electric and magnetic field waves in the far-field traveling at the speed of light, but they always have a special restricted orientation and proportional magnitudes, , which can be seen immediately from the Poynting vector. The electric field, magnetic field, and direction of wave propagation are all orthogonal, and the wave propagates in the same direction as . Also, E and B far-fields in free space, which as wave solutions depend primarily on these two Maxwell equations, are always in-phase with each other. This is guaranteed since the generic wave solution is first order in both space and time, and the curl operator on one side of these equations results in first-order spacial derivatives of the wave solution, while the time-derivative on the other side of the equations, which gives the other field, is first order in time, resulting in the same phase shift for both fields in each mathematical operation.
From the viewpoint of an electromagnetic wave traveling forward, the electric field might be oscillating up and down, while the magnetic field oscillates right and left; but this picture can be rotated with the electric field oscillating right and left and the magnetic field oscillating down and up. This is a different solution that is traveling in the same direction. This arbitrariness in the orientation with respect to propagation direction is known as polarization. On a quantum level, it is described as photon polarization. The direction of the polarization is defined as the direction of the electric field.