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Numerical fits to important rates in high temperature astrophysical plasmas

Stepney, S., Guilbert, P. W.·1983·Monthly Notices of the Royal Astronomical Society

Abstract

We give simple but accurate numerical fits to various two-body rates in relativistic thermal plasmas, in the temperature range |$kT_\text e \sim 50\enspace \text{keV}-1\enspace\text{MeV}$|⁠. The processes we discuss are bremsstrahlung, Coulomb heating and electron–positron pair production and annihilation. In particular we present a fit to the thermal electron–electron bremsstrahlung spectrum which is accurate to better than 5 per cent. We also include the results of some other workers, for completeness. Our results are suitable for semi-analytic or computer modelling of hot plasmas.

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Metadata

Authors
Stepney, S., & Guilbert, P. W.
Venue
Monthly Notices of the Royal Astronomical Society
Published
1983-10-01
Volume
204
Issue
4
Pages
1269-1277
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2000302353
Cited by
178
References
0
FWCI
1.12
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Numerical fits to important rates in high temperature astrophysical plasmas. https://app.cochat.ai/papers/10.1093/mnras/204.4.1269
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Stepney, S., & Guilbert, P. W. (1983). Numerical fits to important rates in high temperature astrophysical plasmas. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/204.4.1269

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