Abstract:
Electron-positron pair production must be included when considering the hard X-ray spectra of AGN's and \(\gamma\)-ray bursters. We investigate thermal plasmas with temperatures \(kT \simeq m_e c^2\) and optical depths \(1 \lesssim \tau \lesssim 5\), including pair processes, Comptonization and bremsstrahlung. Analytic and numerical results are presented for equilibrium and impulsively heated plasmas.
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@inproceedings(SS-XUVAGN-84, author = "Susan Stepney and Paul W. Guilbert", title = "Pair production at moderate optical depths", crossref = "XUVAGN-84" ) @proceedings(XUVAGN-84, title = "X-Ray and {UV} Emission from {A}ctive {G}alactic {N}uclei", booktitle = "X-Ray and {UV} Emission from {A}ctive {G}alactic {N}uclei", editor = "W. Brinkmann and J. Trumper", address = "Max-Planck Institut fur extraterrestrische Physik, Garching", year = 1984 )