Difference between revisions of "Absorption length"
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</math>  | </math>  | ||
where ''ρ'' is density, ''N<sub>a</sub>'' is the Avogadro constant, and ''m<sub>a</sub>'' is the atomic molar mass. Note that the '''mass attenuation coefficient''' is simply <math>\mu/\rho</math>.  | where ''ρ'' is density, ''N<sub>a</sub>'' is the Avogadro constant, and ''m<sub>a</sub>'' is the atomic molar mass. Note that the '''mass attenuation coefficient''' is simply <math>\mu/\rho</math>.  | ||
| + | |||
| + | ==Elemental dependence==  | ||
| + | |||
| + | [[Image:Elements-abs.png|400px]][[Image:Elements-mu.png|400px]]  | ||
| + | |||
| + | ==Energy dependence==  | ||
| + | Notice that the absorption undergoes sharp increases when passing through an absorption edge.  | ||
| + | |||
| + | ===Examples===  | ||
| + | |||
| + | ====[[Material:Silicon|silicon]]====  | ||
| + | |||
| + | [[Image:Silicon-AttLen.png|400px]][[Image:Silicon-mu.png|400px]]  | ||
| + | |||
| + | ====[[Material:Gold|gold]]====  | ||
| + | |||
| + | [[Image:Gold-AttLen.png|400px]][[Image:Gold-mu.png|400px]]  | ||
| + | |||
| + | ==Elemental/Energy dependence==  | ||
| + | [[Image:Elements2D-abs.png|400px]][[Image:Elements2D-mu.png|400px]]  | ||
==Related forms==  | ==Related forms==  | ||
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| <math>\epsilon = \frac{1}{\mu}</math>  | | <math>\epsilon = \frac{1}{\mu}</math>  | ||
| <math>\epsilon = \frac{\rho}{\mu/\rho}</math>  | | <math>\epsilon = \frac{\rho}{\mu/\rho}</math>  | ||
| − | | <math>\epsilon = \frac{  | + | | <math>\epsilon = \frac{M_a}{\rho N_a 2 r_e \lambda f_2 }</math>  | 
| − | | <math>\epsilon = \frac{  | + | | <math>\epsilon = \frac{M_a}{\rho N_a \sigma}</math>  | 
| − | |    | + | | <math>\epsilon = \frac{ \lambda }{4 \pi \beta}</math>  | 
| − | + | | <math>\epsilon = \frac{1}{2 \lambda \mathrm{Im}(\mathrm{SLD})} </math>  | |
|-  | |-  | ||
| <math>\mu = \frac{1}{\epsilon}</math>  | | <math>\mu = \frac{1}{\epsilon}</math>  | ||
| <math>\mu</math>  | | <math>\mu</math>  | ||
| <math>\mu = \frac{\mu/\rho}{\rho}</math>  | | <math>\mu = \frac{\mu/\rho}{\rho}</math>  | ||
| − | | <math>\mu = \frac{\rho N_a}{  | + | | <math>\mu = \frac{\rho N_a}{M_a} 2 r_e \lambda f_2</math>  | 
| − | | <math>\mu = \frac{\rho N_a}{  | + | | <math>\mu = \frac{\rho N_a}{M_a} \sigma</math>  | 
| − | |    | + | | <math>\mu = \frac{4 \pi }{ \lambda } \beta</math>  | 
| − | |    | + | | <math>\mu = 2 \lambda\mathrm{Im}(\mathrm{SLD})</math>  | 
|-  | |-  | ||
| <math>\frac{\mu}{\rho} = \frac{1}{\rho\epsilon}</math>  | | <math>\frac{\mu}{\rho} = \frac{1}{\rho\epsilon}</math>  | ||
| <math>\frac{\mu}{\rho} = \mu/\rho</math>  | | <math>\frac{\mu}{\rho} = \mu/\rho</math>  | ||
| <math>\frac{\mu}{\rho}</math>  | | <math>\frac{\mu}{\rho}</math>  | ||
| − | | <math>\frac{\mu}{\rho} = \frac{N_a}{  | + | | <math>\frac{\mu}{\rho} = \frac{N_a}{M_a} 2 r_e \lambda f_2</math>  | 
| − | | <math>\frac{\mu}{\rho} = \frac{N_a}{  | + | | <math>\frac{\mu}{\rho} = \frac{N_a}{M_a} \sigma</math>  | 
| − | | <math>\frac{\mu}{\rho} = </math>  | + | | <math>\frac{\mu}{\rho} = \frac{4 \pi}{ \rho \lambda  } \beta</math>  | 
| − | | <math>\frac{\mu}{\rho} = </math>  | + | | <math>\frac{\mu}{\rho} = \frac{2 \lambda}{\rho  } \mathrm{Im}(\mathrm{SLD})</math>  | 
|-  | |-  | ||
| − | | <math>f_2 = \frac{  | + | | <math>f_2 = \frac{M_a }{\rho N_a 2 r_e \lambda  \epsilon} </math>  | 
| − | | <math>f_2 = \frac{  | + | | <math>f_2 = \frac{M_a }{\rho N_a 2 r_e \lambda} \mu </math>  | 
| − | | <math>f_2 = \frac{  | + | | <math>f_2 = \frac{M_a }{ N_a 2 r_e \lambda} \frac{\mu}{\rho} </math>  | 
| <math>f_2</math>  | | <math>f_2</math>  | ||
| <math>f_2 = \frac{\sigma}{2 r_e \lambda}</math>  | | <math>f_2 = \frac{\sigma}{2 r_e \lambda}</math>  | ||
| Line 70: | Line 90: | ||
| <math>f_2 = \frac{M_a}{\rho N_a r_e } \mathrm{Im}(\mathrm{SLD})</math>  | | <math>f_2 = \frac{M_a}{\rho N_a r_e } \mathrm{Im}(\mathrm{SLD})</math>  | ||
|-  | |-  | ||
| − | | <math>\sigma = \frac{  | + | | <math>\sigma = \frac{M_a}{\rho N_a \epsilon} </math>  | 
| − | | <math>\sigma = \frac{  | + | | <math>\sigma = \frac{M_a}{\rho N_a} \mu</math>  | 
| − | | <math>\sigma = \frac{  | + | | <math>\sigma = \frac{M_a}{N_a} \frac{\mu}{\rho}</math>  | 
| <math>\sigma = 2 r_e \lambda f_2</math>  | | <math>\sigma = 2 r_e \lambda f_2</math>  | ||
| <math>\sigma</math>  | | <math>\sigma</math>  | ||
| Line 78: | Line 98: | ||
| <math>\sigma = \frac{2 \lambda M_a}{\rho N_a}\mathrm{Im}(\mathrm{SLD})</math>  | | <math>\sigma = \frac{2 \lambda M_a}{\rho N_a}\mathrm{Im}(\mathrm{SLD})</math>  | ||
|-  | |-  | ||
| − | |    | + | | <math>\beta = \frac{ \lambda }{4 \pi  \epsilon}</math>  | 
| − | |    | + | | <math>\beta = \frac{ \lambda  }{4 \pi } \mu</math>  | 
| − | |    | + | | <math>\beta = \frac{ \rho \lambda  }{4 \pi } \frac{\mu}{\rho}</math>  | 
| <math>\beta = \frac{ \rho N_a r_e \lambda^2 }{2 \pi M_a} f_2</math>  | | <math>\beta = \frac{ \rho N_a r_e \lambda^2 }{2 \pi M_a} f_2</math>  | ||
| <math>\beta = \frac{ \rho N_a \lambda }{4 \pi M_a} \sigma</math>  | | <math>\beta = \frac{ \rho N_a \lambda }{4 \pi M_a} \sigma</math>  | ||
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| <math>\beta = \frac{\lambda^2}{2 \pi} \mathrm{Im}(\mathrm{SLD})</math>  | | <math>\beta = \frac{\lambda^2}{2 \pi} \mathrm{Im}(\mathrm{SLD})</math>  | ||
|-  | |-  | ||
| − | |    | + | | <math>\mathrm{Im}(\mathrm{SLD}) = \frac{1 }{2 \lambda \epsilon} </math>  | 
| − | |    | + | | <math>\mathrm{Im}(\mathrm{SLD}) = \frac{\mu}{2 \lambda} </math>  | 
| − | |    | + | | <math>\mathrm{Im}(\mathrm{SLD}) = \frac{\rho }{2 \lambda} \frac{\mu}{\rho}</math>  | 
| <math>\mathrm{Im}(\mathrm{SLD}) = \frac{\rho N_a r_e }{M_a} f_2</math>  | | <math>\mathrm{Im}(\mathrm{SLD}) = \frac{\rho N_a r_e }{M_a} f_2</math>  | ||
| <math>\mathrm{Im}(\mathrm{SLD}) = \frac{\rho N_a}{2 \lambda M_a}\sigma</math>  | | <math>\mathrm{Im}(\mathrm{SLD}) = \frac{\rho N_a}{2 \lambda M_a}\sigma</math>  | ||
| − | | <math>\mathrm{Im}(\mathrm{SLD}) = \frac{2 \pi   | + | | <math>\mathrm{Im}(\mathrm{SLD}) = \frac{2 \pi }{\lambda^2} \beta</math>  | 
| <math>\mathrm{Im}(\mathrm{SLD})</math>  | | <math>\mathrm{Im}(\mathrm{SLD})</math>  | ||
|}  | |}  | ||
| + | |||
| + | |||
| + | See also '''[[Atomic_scattering_factors#Related_forms|scattering factors]]''' for a comparison of the quantities related to ''f''<sub>1</sub>.  | ||
==See Also==  | ==See Also==  | ||
| + | * [[Resonant scattering]]  | ||
| + | ** [[RSoXS]]  | ||
| + | ** [[Resonant reflectivity]]  | ||
* [http://henke.lbl.gov/optical_constants/atten2.html LBL X-Ray Attenuation Length calculator]  | * [http://henke.lbl.gov/optical_constants/atten2.html LBL X-Ray Attenuation Length calculator]  | ||
* [http://11bm.xray.aps.anl.gov/absorb/absorb.php APS absorption calculator]  | * [http://11bm.xray.aps.anl.gov/absorb/absorb.php APS absorption calculator]  | ||
| + | * [http://henke.lbl.gov/optical_constants/filter2.html CXRO transmission calculator]  | ||
* [http://en.wikipedia.org/wiki/Mass_attenuation_coefficient Wikipedia: Mass attenuation coefficient]  | * [http://en.wikipedia.org/wiki/Mass_attenuation_coefficient Wikipedia: Mass attenuation coefficient]  | ||
| + | * [http://en.wikipedia.org/wiki/Absorption_cross_section Wikipedia: Absorption cross sectio]  | ||
* [http://www.nist.gov/pml/data/xraycoef/ NIST tables of x-ray mass attenuation coefficient]  | * [http://www.nist.gov/pml/data/xraycoef/ NIST tables of x-ray mass attenuation coefficient]  | ||
Latest revision as of 15:43, 29 July 2015
The absorption length or attenuation length in x-ray scattering is the distance over which the x-ray beam is absorbed. By convention, the absorption length ϵ is defined as the distance into a material where the beam flux has dropped to 1/e of its incident flux.
Contents
Absorption
The absorption follows a simple Beer-Lambert law:
The attenuation coefficient (or absorption coefficient) is simply the inverse of the absorption length;
Calculating
The absorption length arises from the imaginary part of the atomic scattering factor, f2. It is closely related to the absorption cross-section, and the mass absorption coefficient. Specifically, the atomic photoabsorption cross-section can be computed via:
Where λ is the x-ray wavelength, and re is the classical electron radius. The attenuation coefficient is given by:
where ρ is density, Na is the Avogadro constant, and ma is the atomic molar mass. Note that the mass attenuation coefficient is simply .
Elemental dependence
Energy dependence
Notice that the absorption undergoes sharp increases when passing through an absorption edge.
Examples
silicon
gold
Elemental/Energy dependence
Related forms
As can be seen, there are many related quantities which express the material's absorption:
- Absorption length , the distance over which the intensity falls to 1/e.
 - Attenuation coefficient , the characteristic inverse-distance for attenuation.
 - Mass attenuation coefficient , the density-scaled attenuation.
 - Absorptive atomic scattering factor , the intrinsic dissipative interaction of the material.
 - Atomic photoabsorption cross-section , the cross-section ('effective size') of the atom's x-ray absorption (capture) efficiency.
 - Imaginary refractive index , the resonant component of the refractive index.
 - Imaginary Scattering Length Density , the absorptive component of the scattering contrast.
 
See also scattering factors for a comparison of the quantities related to f1.