Relativistic corrections to collective photon scattering in plasmas

V N Tsytovich, R Bingham, U de Angelis, A Forlani

Research output: Contribution to journalArticle

3 Citations (Scopus)

Abstract

Relativistic corrections to Thomson scattering of photons in plasmas are well known [D. H. Sampson, Ap. J. 129, 734 (1959); J. R. Buchler and W. R. Yueh, Ap. J. 210, 440 (1976) (Ref. 1)]. Here we consider the case when collective effects also have to be taken into account and find the relativistic corrections to collective scattering in plasmas. Collective effects are due to the shielding clouds and are important when the wavelength of the scattering radiation is of the same size or larger than the Debye wavelength. This is the case, for instance, in the solar interior where relativistic corrections to Thomson scattering of photons have recently been taken into account in the calculation of the solar opacity [S. Rose, J. Phys. B: Atom. Molec. Phys. 26, L29 (1993); Iglesias and Rogers, Ap. J. 371, 408 (1991) (Ref. 2)] with the result of a few percent decrease. As an application of our results we show that when the relativistic corrections to collective scattering are included, the decrease in the opacity is 0.2%.
LanguageEnglish
Pages797-807
Number of pages11
JournalJournal of Quantitative Spectroscopy and Radiative Transfer
Volume55
Issue number6
DOIs
Publication statusPublished - 30 Jun 1996

Fingerprint

Photons
Scattering
Plasmas
Thomson scattering
photons
opacity
scattering
Opacity
solar interior
Wavelength
wavelengths
shielding
Shielding
radiation
Radiation
Atoms
atoms

Keywords

  • relativistic corrections
  • photon scattering
  • plasmas
  • Thomson scattering

Cite this

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title = "Relativistic corrections to collective photon scattering in plasmas",
abstract = "Relativistic corrections to Thomson scattering of photons in plasmas are well known [D. H. Sampson, Ap. J. 129, 734 (1959); J. R. Buchler and W. R. Yueh, Ap. J. 210, 440 (1976) (Ref. 1)]. Here we consider the case when collective effects also have to be taken into account and find the relativistic corrections to collective scattering in plasmas. Collective effects are due to the shielding clouds and are important when the wavelength of the scattering radiation is of the same size or larger than the Debye wavelength. This is the case, for instance, in the solar interior where relativistic corrections to Thomson scattering of photons have recently been taken into account in the calculation of the solar opacity [S. Rose, J. Phys. B: Atom. Molec. Phys. 26, L29 (1993); Iglesias and Rogers, Ap. J. 371, 408 (1991) (Ref. 2)] with the result of a few percent decrease. As an application of our results we show that when the relativistic corrections to collective scattering are included, the decrease in the opacity is 0.2{\%}.",
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Relativistic corrections to collective photon scattering in plasmas. / Tsytovich, V N; Bingham, R; Angelis, U de; Forlani, A.

In: Journal of Quantitative Spectroscopy and Radiative Transfer, Vol. 55, No. 6, 30.06.1996, p. 797-807.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Relativistic corrections to collective photon scattering in plasmas

AU - Tsytovich, V N

AU - Bingham, R

AU - Angelis, U de

AU - Forlani, A

PY - 1996/6/30

Y1 - 1996/6/30

N2 - Relativistic corrections to Thomson scattering of photons in plasmas are well known [D. H. Sampson, Ap. J. 129, 734 (1959); J. R. Buchler and W. R. Yueh, Ap. J. 210, 440 (1976) (Ref. 1)]. Here we consider the case when collective effects also have to be taken into account and find the relativistic corrections to collective scattering in plasmas. Collective effects are due to the shielding clouds and are important when the wavelength of the scattering radiation is of the same size or larger than the Debye wavelength. This is the case, for instance, in the solar interior where relativistic corrections to Thomson scattering of photons have recently been taken into account in the calculation of the solar opacity [S. Rose, J. Phys. B: Atom. Molec. Phys. 26, L29 (1993); Iglesias and Rogers, Ap. J. 371, 408 (1991) (Ref. 2)] with the result of a few percent decrease. As an application of our results we show that when the relativistic corrections to collective scattering are included, the decrease in the opacity is 0.2%.

AB - Relativistic corrections to Thomson scattering of photons in plasmas are well known [D. H. Sampson, Ap. J. 129, 734 (1959); J. R. Buchler and W. R. Yueh, Ap. J. 210, 440 (1976) (Ref. 1)]. Here we consider the case when collective effects also have to be taken into account and find the relativistic corrections to collective scattering in plasmas. Collective effects are due to the shielding clouds and are important when the wavelength of the scattering radiation is of the same size or larger than the Debye wavelength. This is the case, for instance, in the solar interior where relativistic corrections to Thomson scattering of photons have recently been taken into account in the calculation of the solar opacity [S. Rose, J. Phys. B: Atom. Molec. Phys. 26, L29 (1993); Iglesias and Rogers, Ap. J. 371, 408 (1991) (Ref. 2)] with the result of a few percent decrease. As an application of our results we show that when the relativistic corrections to collective scattering are included, the decrease in the opacity is 0.2%.

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KW - Thomson scattering

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