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NIST Standard Reference Database 100

NIST Database for the Simulation of Electron Spectra for Surface Analysis (SESSA): Version 2.1.1

 

Version 2.1.1 of SESSA can be used to simulate AES and XPS spectra of nanostructures such as islands, lines, spheres, and layered spheres on surfaces. As for earlier versions, such simulations can be performed for multilayer films. Users can specify the compositions and dimensions of each material in the sample structure as well as the measurement configuration, and the simulated spectra can be compared with measured spectra. Compositions and dimensions can then be adjusted to find maximum consistency between simulated and measured spectra.

This database has been designed to facilitate quantitative interpretation of AES and XPS spectra and to improve the accuracy of quantitation in routine analysis [1-3]. SESSA contains physical data needed to perform quantitative interpretation of an AES or XPS spectrum for a specimen of given composition and morphology (differential inverse inelastic mean free paths, total inelastic mean free paths, differential elastic-scattering cross sections, total elastic-scattering cross sections, transport cross sections, photoionization cross sections, photoionization asymmetry parameters, electron-impact ionization cross sections, photoelectron lineshapes, Auger-electron lineshapes, fluorescence yields, and Auger-electron backscattering factors). Retrieval of relevant data is performed by a small expert system that queries the comprehensive databases. A simulation module provides an estimate of peak intensities as well as the peak spectra.

The design of the software allows the user to enter the required information in a reasonably simple way. The modular structure of the user interface closely matches that of the usual control units on a real instrument. Any user who is familiar with a typical AES or XPS spectrometer can perform a retrieval/simulation operation with the SESSA software in a few minutes for a specimen with a given composition and morphology. A command line interface can also control the software; this feature allows users to load sequences of commands that facilitate simulations for similar conditions.

Version 1.0 of this database was released in December, 2005. Version 1.1 was released in December, 2006 with an enhancement to the Model Calculation screen that permits the user to display and save the zero-order partial intensities. Previously, a user had to go to another screen to perform these operations. Version 1.2 was released in March, 2010 with the following enhancements: an additional and more intuitive format for specifying the composition of a material; a new capability to perform simulations with polarized photons; the ability to save plots in additional file formats; the addition of a chemical-shift database for selected peaks; improvements in the peak-management software; and incorporation of a faster random number generator. In addition, an internet SESSA forum has been established for user questions and a new SESSA bug-tracking web page has been established. Version 1.3 was released in May, 2011 with a new database of non-dipole photoionization cross sections that are necessary in simulations of X-ray photoelectron intensities with X-ray energies higher than a few keV. In addition, a description is given of how SESSA can be called and controlled from an external application. Version 2.0 was released in October, 2014 with additional capabilities for specifying specimen nanomorphologies (such as islands, lines, spheres, and layered spheres on surfaces) and with updated data for electron inelastic mean free paths. Version 2.1 was released in December, 2017 with corrections of two software bugs in SESSA 2.0 that affected simulations with the islands morphology and simulations with the spheres morphology if one or more additional layers had been added to the substrate. This version allows users to create new sample morphologies with the PENGEOM geometry package [4] and has two new databases, one for the inelastic mean free path and another for the electron-impact ionization cross section. Version 2.1.1 was released in August, 2018 to correct a software bug that affected calculations of photoelectron intensities involving non-dipole terms in the photoionization cross section. This bug could have significant effects only for X-ray energies in excess of 2 keV.
 

A fully functional demonstration version of SESSA can be downloaded by clicking here. This trial version can be used for a 15-day trial period without charge. The sessa.exe file is encrypted and it is possible that a virus scan with some antivirus software might prevent execution of this file. Installation on a computer with different antivirus software would likely overcome this problem.
 

Please click to view the PDF version of the Users' Guide .

Systems Requirements:
SESSA runs on personal computers using the Windows operating system including Windows 7 32-bit and 64-bit systems. The databases and software require a hard disc space of approximately180 MB. The minimum amount of RAM needed to run SESSA is about 15 MB, but 30 MB or more is needed for simulations. SESSA is also available for MacIntosh OS X and Linux operating systems, but these versions have not been as extensively tested as the Windows version, and are not supported.
 

For more information please contact:
Standard Reference Data Program
National Institute of Standards and Technology
100 Bureau Dr., Stop 6410
Gaithersburg, MD 20899-6410
(844) 374-0183 (Toll Free)  
data [at] nist.gov () (E-MAIL)

 

The scientific contact for the database is:
Cedric Powell
National Institute of Standard and Technology
Materials Measurement Science Division (643)
phone: (301) 975-2534
email: 
cedric.powell [at] nist.gov

1. W. Smekal, W. S. M. Werner, and C. J. Powell, Surf. Interface Anal. 37, 1059 (2005).
2. W. S. M. Werner, Surf. Interface Anal. 31, 141 (2001).
3. W. S. M. Werner, in Surface Analysis by Auger and X-ray Photoelectron Spectroscopy, D. Briggs and J. T. Grant, eds. (IMPublications, Chichester, 2003), p. 235.
4. J. Almansa, F. Salvat-Pujol, G. Diaz-Londono, A. Carnicer, A. M. Lallena, and F. Salvat, Comput. Phys. Comm. 199, 102 (2016).

 

Keywords: Auger-electron backscattering factors, Auger-electron lineshapes, Auger electron spectroscopy, cross sections, elastic scattering, electron-impact ionization cross section, electron scattering, electron transport, fluorescence yields, inelastic mean free paths, inelastic scattering, photoelectron lineshapes, photoionization asymmetry parameters, photoionization cross sections, surface analysis, transport cross sections, x-ray photoelectron spectroscopy.

 

 

Customer Support

Contact

Standard Reference Data, NIST:
100 Bureau Drive, Stop 6410
Gaithersburg, MD 20899-6410
Tel: 844-374-0183 (Toll Free)

If you have any questions regarding this website, or notice any problems or inaccurate information, please contact the webmaster by sending e-mail to: data [at] nist.gov

Created August 26, 2010, Updated May 9, 2019