Calculating opacity in hot, dense matter using second-order electron-photon and two-photon transitions to approximate line broadening
Calculations of the opacity of hot, dense matter require models for plasma line broadening. However, the most general theories are too complex to calculate directly and some approximation is inevitably required. The most widely used approaches focus on the line center, where a Lorentzian shape is ob...
Glavni autori: | Baggott, RA, Rose, SJ, Mangles, SPD |
---|---|
Format: | Journal article |
Jezik: | English |
Izdano: |
American Physical Society
2020
|
Slični predmeti
-
Temperature equilibration due to charge state fluctuations in dense plasmas
od: Baggott, RA, i dr.
Izdano: (2021) -
Photon–Photon Interactions and the Opacity of the Universe in Gamma Rays
od: Alberto Franceschini
Izdano: (2021-05-01) -
Quantum-statistical models of hot dense matter : methods for computation opacity and equation of state /
od: Nikiforov, Arnold F., i dr.
Izdano: (2005) -
Skyrme-RPA study of charged-current neutrino opacity in hot and dense supernova matter
od: Dzhioev Alan A., i dr.
Izdano: (2018-01-01) -
Jet broadening in the opacity and twist expansions
od: Hannah Clayton, i dr.
Izdano: (2022-05-01)