Answers are grounded in this paper and cite their sources.
We present an astrophysical extended X-ray absorption fine-structure (EXAFS) analysis (AEA) tool. The AEA tool is designed to generate a numerical model of the modification to the X-ray absorption coefficient due to the EXAFS phenomenon. We have constructed a complete database (elements up to the atomic number 92) of EXAFS parameters: central atom phase shift (2δ 1 ), backscattering phase shift (ϕ b ), and backscattering amplitude ( F ). Using the EXAFS parameter data base, the AEA tool can generate a numerical model of any compound when the atomic numbers of neighboring atoms and their distances to the central X-ray-absorbing atom are given.
No takes yet. Share an insight, caveat, or question.
Woo et al. (1997) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: