LEXS

Low Energy X-ray (WDS) Spectrometer

Choosing a WDS



Parallax's new Low Energy X-ray Spectrometer is the first x-ray spectrometer specifically designed for low energy x-ray analysis to provide very high count rates, Peak-to-Background ratios and better than 18 eV energy resolution for x-ray energies below 2.5 KeV (<5eV at Si) -- the region where most spectrometer systems have problems.  LEXS uses proprietary x-ray collimator optics in a patented configuration to produce detection sensitivity for low energies better than any other commercially available system.  LEXS is intended to be used with electron microscope systems with low beam currents and low acceleration voltages while still achieving very good detection sensitivity for problem elements.  Use of low accelerating voltage limits analysis to depths less than .5 micron to avoid confusion with deeper layers.  Because of its unusual optical configuration, LEXS can be placed on most electron microscopes including TEM, FESEM, and ESEM systems with port diameters larger than 30mm.  There is no prescribed source to optic distance and no preferred orientation allowing it to be placed on almost any EM system.  LEXS is sufficiently small and of low weight that it can be placed in a crowded environment.  Since it requires no detector cooling, there is no liquid nitrogen filling.  LEXS can also be configured for small spot XRF systems.  Because LEXS runs under Windows™, graphical output can be easily incorporated into spreadsheets and documents.


Fig. 1. LEXS mounted on a JEOL 840 showing two positions of
pentagonal diffractor turret and two positions of moving proportional
counter.  X-ray collimator is located close to the sample.


LEXS Scanning Modes

LEXS has several scanning modes which are unlike any other WDS spectrometer but it can also scan like a conventional WDS.  A user can specify an energy range and LEXS will do a user specified resolution scan over that range.  A user can select an element(s) and LEXS will scan over the energy range corresponding to the selection(s).  Dwell time at each energy is selected by the user allowing either fast scans or slower scans.

LEXS can do a scan over the entire energy range from 100-2600 eV at user selected resolution or it can do a scan over that range looking only at energies corresponding to known spectral peaks for a faster scan.  Dwell time at each point is user selectable.

LEXS can do a Peak and Background scan for a selection of elements.  In this fast mode, it looks at a background position for each element, at a position on either side of the spectral peak and at the peak position.  This mode allows very fast analysis of elements when the constituency is known or suspected.

LEXS can do repeated measurements at the peaks of selected elements.  This mode is useful when the user wants fast comparisons of many samples to a standard.

Because LEXS can randomly access any point in the spectrum from 100-2600 eV, it can do fast "intelligent" scans to quickly characterize samples based on the users prior knowledge of sample composition.  This feature will be particularly useful for semiconductor defect characterization where the user knows the probability of various defect types and simply wants to identify the defects.


Choice of Diffractors

Most users would probably prefer to never have to deal with choosing diffractors so the LEXS spectrometer operates in an Energy mode never mentioning wavelength unless the user desires it.  However, a proper choice of diffractors selected for the users needs can be very helpful.  The normal selection of diffractors is as follows:
 

Mo/B4C 2d = 200 For very low energy lines such as Be and B
Cr/Sc 2d = 80 For C and N
W/Si 2d = 60 For energies between 500 and 1000 eV
TAP 2d = 30 For energies between 500 and 2000 eV
PET 2d = 8.79 For energies between 1700 and 2400 eV
Alternate choices:
2d = 120 Specifically for C. This diffractor has limited use other than C but gives
the 5750 cps/na that we quote.  Unless you really want C sensitivity, we do not
recommend it because you will have to give up sensitivity to other elements and
the standard diffractor (2d = 80) works reasonably well for C.
2d = 160 A new diffractor from Osmic specifically for B that gives
about 50% higher counts for B and also works well for Be.
Cr/Ti 2d=80 Specifically for the Ti (L a) line and it suppresses the N line.


Using LEXS for Energy above 2200eV

LEXS was specifically designed for low energy x-rays where Energy Dispersive Spectrometers have their biggest problems so we did not worry about performance above 2 KeV at the time.  However, several users have asked if it could be easily modified to cover the Lead-Molybdenum-Sulfur overlap region (about 2300 eV) and slightly higher with less background.  Keeping the entire system optimized for lower energy is more important than achieving higher count rates for this 2300-3300 eV region but getting the background low enough would greatly extend the utility of the system.  So, we looked for easy ways to get rid of background at these energies resulting in the improved LEXS.  The improved LEXS has the same diffractors to keep optimum performance below 2 KeV but we have managed to greatly reduce background above 1500 eV using an anti-scattering filter so that the high energy PET diffractor can be used over more of its range.

Fig. 1a. shows the Mo (L) lines without the background reducing filter (old LEXS) and Fig. 1b. shows them with the background reducing filter (new LEXS).  The peak count rates are hardly changed but the background is greatly reduced.  LEXS becomes useful for the region between 2200 eV and 2600 eV covering several well known overlaps and it becomes possible to use higher energy lines, such as the U (M) lines for alignment.

Without the anti-scatter filter, the P/B for the Si (K) line is about 200.  The anti-scatter filter increases the P/B to over 600 greatly improving the sensitivity for this spectral region.


    Fig. 1a. Molybedenum (L) lines without Antiscatter filter.



Fig. 1b. Molybedenum (L) lines WITH Anti-scatter filter.
Note that the Mo (L1, and Ln) lines are readily visible.



Fig. 2a. PbS spectrum from improved LEXS. Peaks left
to right are: S(Kα), Pb(Mα) and Pb(Mβ). The
S(Kβ) is just to the right of the Pb(Mβ) but is not resolved.



Fig. 2b. PbS spectrum with optional Ge diffractor.


In this spectral region, there are about 8 peak overlaps that could not be resolved with the old LEXS and EDS but with this improvement, all of these can be resolved.  Above 2600 eV, there are no significant overlaps that cannot be resolved with LEXS and EDS.

Some Applications:

Metallurgy
Be in Beryllium Copper
Identification of alloys
Diffusion of O2 into metals
Carbon content of steel
Quality control of alloy content
Identification of contaminants
Cr monolayers on electroform mandrels         
Detecting surface oxidation on metals
Semiconductor
Wafer Dopant Analysis
Thin Film Analysis
Strontium Titanate on Silicon
Boron in BPSG glass
WSi Stoichiometry
Oxide layer Stoichiometry
TiN, TaN Stoichiometry
Detection of surface oxidation
TaSi2
Coatings
QC of tool coatings (TiN, TiAlN, etc)
QC of optical coatings (TiO2) SiO, SiO2)
Phosphorus content of electroless Ni
Oxidation of coatings
Other
Dopants in Sol-Gel Optics
MgF
Analysis of Stardust
Comet Dust


  Sample spectrum from a TiN coated tool insert
  showing good separation of the Ti and N peaks
  and an unexpected O line from Oxygen in the
  coating
        LEXS minimum detectable limits for various
        elements in %wt

Spectrum of GaAs sample showing the Ga and
As alpha and beta peaks.

Manganese Fluoride (not Magnesium Fluoride)
showing an O line Mn (L1), Mn (La), and F lines.
       TaSi2 showing peaks only 30 eV apart.



Physical and Performance Characteristics of LEXS

Size 25 cm. X 25 cm. X 10 cm.  The motor drive projects 5 cm. beyond the 10 cm. on part of one side.

Detector Gas flow proportional counter using P10 gas (90% argon and 10% methane).  No detector cooling is needed. 0-3000 V power supply.

Software Runs on a PC under Windows™. (Trademark of Microsoft)

Measured LEXS Performance
Element Energy(eV) Counts/sec/na P/B Resolution (eV) Sensitivity(ppm)
Be 10KV 108 400 40 8 100
B 10KV 183 6000 100 18 <20
C 10KV 277 5750 >100 18.6 14
N(BN) 10KV 392 416 40 16 130
O(SiO2) 525 375 80 17 60
Mg 10KV 1254 600 400 14 18
Al 10KV 1487 500 300 19 25
Si 25KV 1740 550 500 5 15



Questions and answers about LEXS.

Q. I have a light element capable EDS system, Why would I need LEXS?

A. There are two answers: resolution and sensitivity. If you want to analyze very thin films or achieve good analytical resolution, you should be using low accelerating voltages (5 KV or less) to avoid exciting the substrate or lower layers. This means you will be using low energy K, L and M lines. There are so many peak overlaps using these lines that EDS is nearly useless while LEXS will easily resolve most of the necessary peaks allowing you to see spectra of films such as TiN, Strontium Titanate on Si, TaSi, and WSi, etc.

For all K lines for Z<15, LEXS is much more sensitive than conventional EDS. Using L, and M lines, LEXS is usually more sensitive than conventional EDS would be using all K lines. When conventional EDS is forced to use L lines, LEXS is almost always more sensitive.

Q. What is the operational energy range of LEXS?

A. Qualitatively:

100 eV to 2600 eV and in some cases 3300 eV.

Q. How does LEXS differ from other high resolution x-ray spectrometers?

A. There are several Wavelength Dispersive Spectrometers (WDS) available, but LEXS is fundamentally different both in the way it collects x-rays and in its response to low energy x-rays. Conventional WDS uses curved crystals to disperse and focus the x-rays onto a detector. LEXS collects a large solid angle of x-rays diverging from the sample and re-directs them into a parallel beam incident on various flat dispersing elements and then into a detector. Some WDS systems are optimized for only one or two elements for each diffractor while LEXS is optimized over its entire range of operation. LEXS produces far greater count rates for low energy x-rays than any conventional WDS. Conventional WDS systems emphasize the use of high accelerating voltages for higher Z elements which is useless for thin films while LEXS is designed for low accelerating voltages. There has been considerable discussion of high resolution micro-calorimeters for x-ray spectroscopy but due to the requirement of using liquid helium and very small solid acceptance angles, we consider micro-calorimeters to be laboratory curiosities while LEXS is very practical.

Q. What options are available?

A. Any orientation of the spectrometer, right or left handed versions, gate valve between spectrometer and SEM and specialized software for your types of samples.

Q. What about leakage of the argon from the flow proportional counter, especially in FESEM systems.

A. We have recently obtained new proportional counter windows with very low leakage rate. We have also replaced the old polypropylene tubing and hose barbs with rigid steel tubing, PEEK tubing and Swage-Lok connectors to nearly eliminate this problem. However, LEXS is available with an optional stand alone pumping system that is used on a system with a gate valve.

Q. If the window fails or there is other vacuum failure in the LEXS, does it shut down the SEM?

A. With the existing optional gate valve, one would simply withdraw the collimator all the way into the LEXS and close the gate valve to isolate the LEXS from the SEM and continue running the SEM while the LEXS is repaired.

Q. What is the best obtainable resolution with LEXS?

A. We have obtained a resolution of <4 eV at the Si (K) line using a PET diffractor. We routinely obtain 5 eV at this energy. By using second order lines, the resolution can be approximately halved at the expense of reducing the peak intensities by 10X.



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