Astrophysics (Index)About

scattering

(changing the direction of a particle's movement)

In physics, scattering means changing the direction of movement of a particle. The word is commonly used for the scattering of photons and electrons but applies to other particles as well. Photon scattering is considered one of the phenomena in radiative transfer (along with absorption and emission) and is sometimes equivalent to absorption followed by emission due to the energy gained from the absorption. The word scattering might be used if emission is immediately following the previous absorption, and the "scattering" concept might be stretched to include longer time intervals between if doing so does not affect the analysis. Some types of scattering:

Some types/models of photon scattering:

Note that some photon scattering phenomena follows the pattern of classical (wave) electromagnetic radiation theory, whereas some does not, and is only explained by light's quantum nature.

The more specific term, elastic scattering is used in particle physics for that in which kinetic energy is preserved (within an inertial reference frame), such that the same amount of energy comprises the kinetic energy of the particles on their new trajectory, none absorbed and converted some other form such as potential energy. Such scattering is analogous to a rubber ball so perfect that it bounces up to the same height it fell from. Thomson scattering is basically elastic, as is the scattering of atoms within monatomic gases. Inelastic scattering naturally means scattering in which some of the kinetic energy is absorbed, i.e., converted to some other form of energy.

Quantum theory includes theories to explain scattering, down at the particle-level.


The term scattering is also used regarding the dynamics of planetary systems, e.g., planets redirected from their orbits. The term may be similarly used for interactions between stars in "crowded" regions such as globular clusters and the centers of galaxies.


(physics,EMR,radiative transfer,photons)
Further reading:
https://en.wikipedia.org/wiki/Scattering
https://www.britannica.com/science/scattering
https://www.chemeurope.com/en/encyclopedia/Scattering.html
https://www.oceanopticsbook.info/view/scattering/physics-scattering
http://www.tcm.phy.cam.ac.uk/~bds10/aqp/lec20-21_compressed.pdf

Referenced by pages:
absorption
absorption coefficient
albedo
Compton scattering
cosmic dust
cross section
distance modulus (μ)
dust echo
electric dipole radiation
electron scattering
emission
epoch of reionization (EOR)
equation of radiative transfer (RTE)
extinction
free streaming
Klein-Nishina formula
light pollution
mean free path
Mie scattering
millimeter astronomy
neutron scattering
optical depth (τ)
Penrose Compton scattering (PCS)
photon
photosphere
PICASO
polarization
radiative transfer (RT)
radiative transfer code (RT code)
Rayleigh scattering
reddening
reflection nebula
relic
Sachs-Wolfe effect (SWE)
scintillometry
spectropolarimetry
stellar atmosphere
stellar encounter
surface of last scattering
synchrotron radiation
synchrotron self-Compton (SSC)
thermal bremsstrahlung
Thomson optical depth (τT)
Thomson scattering
tired light
weak interaction

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