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  2. Thomson scattering - Wikipedia

    en.wikipedia.org/wiki/Thomson_scattering

    Thomson scattering is a model for the effect of electromagnetic fields on electrons when the field energy is much less than the rest mass of the electron .In the model the electric field of the incident wave accelerates the charged particle, causing it, in turn, to emit radiation at the same frequency as the incident wave, and thus the wave is scattered.

  3. Classical electron radius - Wikipedia

    en.wikipedia.org/wiki/Classical_electron_radius

    The classical electron radius appears in the classical limit of modern theories as well, including non-relativistic Thomson scattering and the relativistic Klein–Nishina formula. Also, is roughly the length scale at which renormalization becomes important in quantum electrodynamics. That is, at short-enough distances, quantum fluctuations ...

  4. Klein–Nishina formula - Wikipedia

    en.wikipedia.org/wiki/Klein–Nishina_formula

    In some cases it is convenient to express the classical electron radius in terms of the Compton wavelength: = ¯ = /, where is the fine structure constant (~1/137) and ¯ = / is the reduced Compton wavelength of the electron (~0.386 pm), so that the constant in the cross section may be given as:

  5. Mean free path - Wikipedia

    en.wikipedia.org/wiki/Mean_free_path

    In practice, the diameter of gas molecules is not well defined. In fact, the kinetic diameter of a molecule is defined in terms of the mean free path. Typically, gas molecules do not behave like hard spheres, but rather attract each other at larger distances and repel each other at shorter distances, as can be described with a Lennard-Jones ...

  6. Structure factor - Wikipedia

    en.wikipedia.org/wiki/Structure_factor

    The units of the structure-factor amplitude depend on the incident radiation. For X-ray crystallography they are multiples of the unit of scattering by a single electron (2.82 m); for neutron scattering by atomic nuclei the unit of scattering length of m is commonly used.

  7. Gas constant - Wikipedia

    en.wikipedia.org/wiki/Gas_constant

    In any case, the context and/or unit of the gas constant should make it clear as to whether the universal or specific gas constant is being referred to. [ 10 ] In case of air, using the perfect gas law and the standard sea-level conditions (SSL) (air density ρ 0 = 1.225 kg/m 3 , temperature T 0 = 288.15 K and pressure p 0 = 101 325 Pa ), we ...

  8. Plasma diagnostics - Wikipedia

    en.wikipedia.org/wiki/Plasma_diagnostics

    Scattering of laser light from the electrons in a plasma is known as Thomson scattering. The electron temperature can be determined very reliably from the Doppler broadening of the laser line. The electron density can be determined from the intensity of the scattered light, but a careful absolute calibration is required.

  9. Eddington luminosity - Wikipedia

    en.wikipedia.org/wiki/Eddington_luminosity

    For ionized hydrogen, = /, where is the Thomson scattering cross-section for the electron and is the mass of a proton. Note that F r a d = d 2 E / d A d t {\displaystyle F_{\rm {rad}}=d^{2}E/dAdt} is defined as the energy flux over a surface, which can be expressed with the momentum flux using E = p c {\displaystyle E=pc} for radiation.