Cross section (physics)
A cross section is the effective area that governs the probability of some scattering or absorption event. Together with particle density and path length, it can be used to predict the total scattering probability via the Beer–Lambert law.
In nuclear and particle physics, the concept of a cross section is used to express the likelihood of interaction between particles.
When particles in a beam are thrown against a foil made of a certain substance, the cross section \sigma is a hypothetical area measure around the target particles of the substance (usually its atoms) that represents a surface. If a particle of the beam crosses this surface, there will be some kind of interaction.
The term is derived from the purely classical picture of (a large number of) pointlike projectiles directed to an area that includes a solid target. Assuming that an interaction will occur (with 100% probability) if the projectile hits the solid, and not at all (0% probability) if it misses, the total interaction probability for the single projectile will be the ratio of the area of the section of the solid (the cross section, represented by \sigma) to the total targeted area.
This basic concept is then extended to the cases where the interaction probability in the targeted area assumes intermediate values  because the target itself is not homogeneous, or because the interaction is mediated by a nonuniform field. A particular case is scattering.
Contents
 Scattering 1
 Nuclear physics 2

3 Rate (particle physics)
 Partial cross section 3.1
 Total cross section 3.2
 Differential cross section 3.3
 See also 4
 References 5
 External links 6
Scattering
The scattering crosssection, σ_{scat}, is a hypothetical area which describes the likelihood of light (or other radiation) being scattered by a particle. In general, the scattering crosssection is different from the geometrical crosssection of a particle, and it depends upon the wavelength of light and the permittivity, shape and size of the particle. The total amount of scattering in a sparse medium is determined by the product of the scattering crosssection and the number of particles present. In terms of area, the total crosssection (σ) is the sum of the crosssections due to absorption, scattering and luminescence
 \sigma = \sigma_\text{A} + \sigma_\text{S} + \sigma_\text{L}.\
The total crosssection is related to the absorbance of the light intensity through BeerLambert's law, which says absorbance is proportional to concentration: A_\lambda = C \,\ell\, \sigma, where C is the concentration as a number density, A_{λ} is the absorbance at a given wavelength λ, and \ell is the path length. The extinction or absorbance of the radiation is the logarithm (decadic or, more usually, natural) of the reciprocal of the transmittance:^{[1]}
 A_\lambda =  \log \mathcal{T}.\
Nuclear physics
In nuclear physics, it is convenient to express the probability of a particular event by a cross section. Statistically, the centers of the atoms in a thin foil can be considered as points evenly distributed over a plane. The center of an atomic projectile striking this plane has geometrically a definite probability of passing within a certain distance r of one of these points. In fact, if there are n atomic centers in an area A of the plane, this probability is (n \pi r^2)/A, which is simply the ratio of the aggregate area of circles of radius r drawn around the points to the whole area. If we think of the atoms as impenetrable steel discs and the impinging particle as a bullet of negligible diameter, this ratio is the probability that the bullet will strike a steel disc, i.e., that the atomic projectile will be stopped by the foil. If it is the fraction of impinging atoms getting through the foil which is measured, the result can still be expressed in terms of the equivalent stopping cross section of the atoms. This notion can be extended to any interaction between the impinging particle and the atoms in the target. For example, the probability that an alpha particle striking a beryllium target will produce a neutron can be expressed as the equivalent cross section of beryllium for this type of reaction.
Rate (particle physics)
In scattering theory, particle physics and nuclear physics, the rate at which a specific subatomic particle reaction occurs is a physical quantity measuring the number of reactions per unit time.
Partial cross section
For a particle beam (say of neutrons, pions) incident on a target (liquid hydrogen), for each type of reaction in the scattering process labelled by an index r = 1, 2, 3..., it is calculated from:^{[2]}
 W_r = JN\sigma_r
where N is the number of target particles, illuminated by the beam containing n particles per unit volume in the beam (number density of particles) traveling with average velocity v in the rest frame of the target, and these two quantities combine into the flux of the beam J = nv. The cross section of the reaction is σ_{r}. Since the beam flux has dimensions of [length]^{−2}·[time]^{−1} and σ_{r} has dimensions of [length]^{2} while N is a dimensionless number, the rate W has the dimensions of reciprocal time  which intuitively represents a frequency of recurring events.
The above formula assumes the following:
 the beam particles all have the same kinetic energy,
 the number density of the beam particles is sufficiently low: allowing the interactions between the particles within the beam to be neglected,
 the number density of target particles is sufficiently low: so that only one scattering event per particle occurs as soon as the beam is incident with the target, and multiple scattering events within the target can be neglected,
 the de Broglie wavelength of the beam is much smaller than the interparticle separations within the target, so that diffraction effects through the target can be neglected,
 the collision energy is sufficiently high allowing the binding energies in the target particles to be neglected.
These conditions are usually met in experiments, which allows for a very simple calculation of rate.
Sometimes the rate per unit target particle, or rate density, is more useful. For reaction r:^{[3]}
 W_r/N = J\sigma_r
Total cross section
The cross section σ_{r} is specifically for one type of reaction, and is called the partial cross section. The total cross section, and corresponding total rate of the reaction, can be found by summing over the cross sections and rates for each reaction:^{[2]}
 W = \sum_r W_r = JN \sum_r \sigma_r = JN \sigma
Differential cross section
In terms of the differential cross section dσ_{r}(θ, φ) as a function of spherical polar angles θ and φ for reaction r, the differential rate is:^{[2]}
 dW_r = JN d\sigma_r = JN \frac{d\sigma_r}{d\Omega} d\Omega
where dΩ = d(cosθ)dφ is the solid angle element in the vicinity of the event with vertex at the point of scattering. Integrating over θ and φ returns the rate for reaction r:
 W_r = JN \int_0^{2\pi} d\varphi \int_{1}^{+1} d(\cos\theta) \frac{d\sigma_r}{d\Omega}
See also
 Cross sectional area
 Differential cross section
 Luminosity (scattering theory)
 Neutron cross section
 Particle detector
 Radar: The (monostatic) radar cross section is defined as 4 π times the radio differential cross section at 180 degrees.
 Rutherford scattering
 Scattering amplitude
References
 J.D.Bjorken, S.D.Drell, Relativistic Quantum Mechanics, 1964
 P.Roman, Introduction to Quantum Theory, 1969
 W.Greiner, J.Reinhardt, Quantum Electrodynamics, 1994
 R.G. Newton. Scattering Theory of Waves and Particles. McGraw Hill, 1966.
 R.C. Fernow (1989). Introduction to Experimental Particle Physics. Cambridge University Press.
External links
 Nuclear Cross Section
 Scattering Cross Section
 IAEA  Nuclear Data Services
 BNL  National Nuclear Data Center
 Particle Data Group  The Review of Particle Physics
 IUPAC Goldbook  Definition: Reaction Cross Section
 IUPAC Goldbook  Definition: Collision Cross Section