12.1. Spectroscopy of Photons 681
NEXAFS EXAFSX−ray EnergyX−ray IntensityFigure 12.1.7: Typical x-ray
absorption spectrum. The spec-
trum is divided into two regions
of near-edge and extended fine
structures.relation between the wavelength of an electronλeand its momentuampe,thatis
λe=h
pe, (12.1.3)
wherehis the Planck’s constant. Using non-relativistic consideration, we can write
the momentum of the electron as
pe = meve
=√
2 meEe, (12.1.4)wheremeis the mass of the electron,veis its velocity, andEeis its kinetic energy
given byEe=mev^2 e/2. Substitutingpe=
√
2 meEein the above equation givesλe=h
√
2 meEe. (12.1.5)
The kinetic energyEeof a photoelectron is relation to the energy of the incident
photonEγthrough
Ee=Eγ−Eb, (12.1.6)
whereEbis the binding energy o f the atom. Hence the wavelength of a photoelectron
can be evaluated from
λe=h
√
2 me(Eγ−Eb). (12.1.7)
Now, the wavenumber of a particle having wavelengthλis given byk=2π/λ.The
above equation can then also be written as
2 π
k=
h
√
2 me(Eγ−Eb)⇒k =[
2 me(Eγ−Eb)
^2] 1 / 2
, (12.1.8)
where≡=h/ 2 π. Using this expression the attenuation coefficient of the material
for x-rays can be scaled tok.Atypicalplotofμ(k) with respect tokis shown in
Fig.12.1.8. Note that the scaling ofμwith respect tokdoes not affect its shape.