Compton scattering
Encyclopedia : C : CO : COM : Compton scattering
In physics, Compton scattering or the Compton effect, is the decrease in energy (increase in wavelength) of an X-ray or gamma ray photon, when it interacts with matter. The amount the wavelength increases by is called the Compton shift. Although nuclear compton scattering exists, what is meant by Compton scattering usually is the interaction involving only the electrons of an atom. Compton effect was observed by Arthur Holly Compton in 1923, for which he earned the 1927 Nobel Prize in Physics.
The effect is important because it demonstrates that light cannot be explained purely as a wave phenomenon. Thomson scattering, the classical theory of charged particles scattered by an electromagnetic wave, cannot explain any shift in wavelength. Light must behave as if it consists of particles in order to explain the Compton scattering. Compton's experiment convinced physicists that light can behave as a stream of particles whose energy is proportional to the frequency.
The interaction between high energy photons and electrons results in the electron being given part of the energy (making it recoil), and a photon containing the remaining energy being emitted in a different direction from the original, so that the overall momentum of the system is conserved. If the photon still has enough energy left, the process may be repeated.
Compton scattering occurs in all materials and predominantly with photons of medium energy, i.e. about 0.5 to 3.5 MeV. It is also observed that high-energy photons; photons of visible light or higher frequency, for example, have sufficient energy to even eject the bound electrons from the atom (Photoelectric effect).
The Compton shift formula
For differential cross section of Compton scattering, see Klein-Nishina formula.
Compton used a combination of three fundamental formulas representing the various aspects of classical and modern physics, combining them to describe the quantum behavior of light.
- Light as a particle, as noted previously in the photoelectric effect.
- Relativistic dynamics Special Theory of Relativity
- Trigonometry - Law of cosines
- [ \lambda_2 = \frac(1-\cos) + \lambda_1 ]
- [\lambda_1 ] is the wavelength of the photon before scattering,
- [\lambda_2 ] is the wavelength of the photon after scattering,
- me is the mass of the electron,
- h/(mec) is known as the Compton wavelength,
- θ is the angle by which the photon's heading changes,
- h is Planck's constant, and
- c is the speed of light.
Derivation
We use that:- [E_ + E_ = E_ + E_\,]
And:
- [\vec p_ + \vec} = \vec} + \vec}\,]
We then use [E = hf = pc]:
- [\vec} = \vec} - \vec}\,]
- [}}^2 = } - \vec})}^2]
- [}}^2 = \vec}^2 - 2\cdot\vec}\cdot\vec} + \vec}^2]
- [\vec} \cdot \vec} = \vec} \cdot \vec}- 2\cdot\vec}\cdot\vec} + \vec} \cdot \vec}]
- [}^2 \cdot \cos(0) = p_^2 \cdot \cos(0) - 2 \cdot p_ \cdot p_ \cdot \cos(\theta) + p_^2\cdot \cos(0)]
substituting [p_] with [\frac] and [p_] with [\frac], we derive
- [p_^2 = \frac + \frac - \frac}]
- [E_ + E_ = E_ + E_\,]
- [hf + mc^2 = hf' + \sqrtc)^2 + (mc^2)^2}\,]
- [(hf + mc^2-hf')^2 = (p_c)^2 + (mc^2)^2\,]
- [\frac= p_^2\,]
- [\frac = \frac + \frac - \frac}]
- [h^2f^2+h^2f'^2-2h^2ff'+2h(f-f')mc^2 = h^2f^2+h^2f'^2-2h^2ff'\cos\,]
- [-2h^2ff'+2h(f-f')mc^2 = -2h^2ff'\cos\,]
- [hff'-(f-f')mc^2 = hff'\cos\,]
- [hff'(1-\cos) = (f-f')mc^2\,]
- [h\frac\frac(1-\cos) =\left(\frac-\frac\right)mc^2]
- [h\frac\frac(1-\cos) = \left(\frac-\frac\right)mc^2]
- [ h(1-\cos) = \frac\frac\left(\frac-\frac\right)mc^2]
- [h(1-\cos) = \left(\frac-\frac\right)mc^2]
- [\frac(1-\cos) =\lambda'-\lambda]
Applications
Compton scattering is of prime importance to radiobiology, as it happens to be the most probable interaction of high energy X rays with atomic nuclei in living beings and is applied in radiation therapy.
Compton scattering has on occasion been proposed as an alternative explanation for the phenomenon of the redshift by opponents of the Big Bang theory, although this is not generally accepted because the influence of the Compton scattering would be noticeable in the spectral lines of distant objects and this is not observed.
In material physics, Compton scattering can be used to probe the wave function of the electrons in matter in the momentum representation.
Compton Scatter is an important effect in Gamma spectroscopy, as it is possible for the gamma rays to scatter out of the detectors used. Compton suppression is used to detect stray scatter gamma rays to counteract this effect.
See also
- Thomson scattering
- Photoelectric effect
- Timeline of cosmic microwave background astronomy
- Peter Debye
- Sunyaev Zel'dovich effect
- Walther Bothe
- List of astronomical topics
- List of physics topics
External links
- [Compton Effect] (PDF file) by Michael Brandl for [Project PHYSNET].
From Wikipedia, the Free Encyclopedia. Original article here. Support Wikipedia by contributing or donating.
All text is available under the terms of the GNU Free Documentation License See Wikipedia Copyrights for details.

