Encyclopedia
In
optics,
stimulated emission is the process by which, when perturbed by a
photon, matter may lose
energy resulting in the creation of another photon. The perturbing photon is
not destroyed in the process , and the second photon is created with the same phase,
frequency,
polarization, and direction of travel as the original. Stimulated emission is really a
quantum mechanical phenomenon but it can be understood in terms of a classical field and a quantum mechanical atom. The process can be thought of as
optical amplification, and it forms the basis of the
laser and
maser.
Overview
Electrons and how they interact with each other and electromagnetic fields form the basis for most of our understanding of
chemistry and
physics. Electrons have energy in proportion to how far they are on average from the
nucleus of an
atom. Thus, electrons are found in specific energy levels, of an atom, as shown below:
The Pauli exclusion principle forces some electrons to be farther from the nucleus than others, which is why all the electrons in an atom do not simply occupy the 1
s orbital. When electrons absorb energy either from
light or from
heat , they move farther away from the
atomic nuclei but they are only allowed to absorb energy that will land them into specific energy levels. This leads to
emission lines and
absorption lines.
When an
electron is
excited, it will not stay that way forever. On average there is a lifetime for any particular energy level after which half of the electrons initially in that state will have
decayed into a lower state. When such a decay occurs, the
energy difference between the level the electron was at and the new level must be released either as a photon or a phonon. When an electron decays due to "timeout" it is said to be due to "
spontaneous emission." The phase associated with the photon that is emitted is random and has to do with some
quantum mechanical ideas concerning the atom's internal state. If a bunch of electrons were put into an excited state somehow and then left to relax, the resulting radiation would be very spectrally limited but the individual photons would not be in phase with one another. This is also called
fluorescence.
Other photons will affect an atom's state. The quantum mechanical variables mentioned above are changed. Specifically the atom will act like a small electric
dipole which will oscillate with the external field. One of the consequences of this oscillation is it encourages electrons to decay to the lower energy state. When it does this due to the presence of other photons, the released photon is
in phase with the other photons and in the same direction as the other photons. This is known as stimulated emission.
Stimulated emission can be modelled mathematically by considering an
atom which may be in two
electronic
energy states, the
ground state and the
excited state , with energies
E1 and
E2 respectively.
If the atom is in the excited state, it may decay into the ground state by the process of
spontaneous emission, releasing the difference in energies between the two states as a photon. The photon will have
frequency ν and
energy hν, given by:
,
where
h is Planck's constant.
Alternatively, if the excited-state atom is perturbed by the electric field of a photon with frequency ν, it may release a
second photon of the same frequency, in phase with the first photon. The atom will again decay into the ground state. This process is known as
stimulated emission.
In a group of such atoms, if the number of atoms in the excited state is given by
N, the rate at which stimulated emission occurs is given by:
,
where
B21 is a proportionality constant for this particular transition in this particular atom , and ρ is the radiation density of photons of frequency ν. The rate of emission is thus proportional to the number of atoms in the excited state,
N, and the density of the perturbing photons.
The critical detail of stimulated emission is that the emitted photon is identical to the stimulating photon in that it has the same
frequency, phase,
polarization, and direction of propagation. The two photons, as a result, are totally coherent. It is this property that allows optical amplification to take place.
Although most directly related to the discussion of how
lasers work, stimulated emission touches on some of the most basic concepts in physics and the interaction of light and matter. It is a very important and key understanding to the understanding of optics specifically and physics in general.
Spectral line shape function
Although there are many possible line shapes, it is common to model the
spectral line shape function as a
Lorentzian distribution:
where
is the
full width at half maximum, or FWHM, in hertz.
This model is generally valid as long as
and
The line shape function, regardless of the form that it takes, must satisfy the normalization condition of any probability distribution:
which the Lorentzian satisfies.
The peak value of the Lorentzian line shape occurs at the line center:
It is also convenient to define the
normalized line shape function:
which is dimensionless, and which has a peak value, also at the line center, of
Stimulated emission cross section
The stimulated emission cross section is
where
- A21 is the Einstein A coefficient ,
- λ is the wavelength ,
- n is the refractive index of the medium , and
- g is the spectral line shape function .
Optical amplification
Under certain conditions, stimulated emission can provide a physical mechanism for
optical amplification. An external source of energy stimulates atoms in the ground state to transition to the excited state, creating what is called a
population inversion. When light of the appropriate frequency passes through the inverted medium, the photons stimulate the excited atoms to emit additional photons of the same frequency, phase, and direction, resulting in an amplification of the input intensity.
The population inversion, in units of atoms per
cubic meter, is
where
g1 and
g2 are the degeneracies of energy levels 1 and 2, respectively.
Small signal gain equation
The intensity of the stimulated emission is governed by the following differential equation:
as long as the intensity
I is small enough so that it does not have a significant effect on the magnitude of the population inversion. Grouping the first two factors together, this equation simplifies as
where
is the
small-signal gain coefficient . We can solve the differential equation using separation of variables:
Integrating, we find:
or
where
is the optical intensity of the input signal .
Saturation intensity
The saturation intensity
IS is defined as the input intensity at which the gain of the optical amplifier drops to exactly half of the small-signal gain. We can compute the saturation intensity as
where
- h is Planck's constant, and
- τS is the saturation time constant, which depends on the spontaneous emission lifetimes of the various transitions between the energy levels related to the amplification.
General gain equation
The general form of the gain equation, which applies regardless of the input intensity, derives from the general differential equation for the intensity
I as a function of position
z in the gain medium:
where is the saturation intensity. To solve, we first rearrange the equation in order to separate the variables, intensity
I and position
z:
Integrating both sides, we obtain
or
The gain
G of the amplifier is defined as the optical intensity
I at position
z divided by the input intensity:
Substituting this definition into the prior equation, we find the
general gain equation:
Small signal approximation
In the special case where the input signal is small compared to the saturation intensity, in other words,
then the general gain equation gives the small signal gain as
or
which is identical to the small signal gain equation .
Large signal asymptotic behavior
For large input signals, where
the gain approaches unity
and the general gain equation approaches a linear
asymptote:
References
See also
