We demonstrate the possibilities of classical integral equations (HNC approach) and ab initio quantum simulations (DFT-MD) to yield structural properties of warm dense matter needed to model and interpret X-ray scattering signals. For that goal, the electronic as well as the ionic structure is neede
Resonant scattering of X-rays by the warm intergalactic medium
β Scribed by E. Churazov; M. Haehnelt; O. Kotov; R. Sunyaev
- Publisher
- John Wiley and Sons
- Year
- 2001
- Tongue
- English
- Weight
- 355 KB
- Volume
- 323
- Category
- Article
- ISSN
- 0035-8711
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