Auger Electron Spectroscopy. Outline 1.Introduction 2.Principle of AES 3.Instrumentation 3.1 UHV environment 3.2 Electron gun 3.3 Electron energy analyzer.

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Auger Electron Spectroscopy
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Presentation transcript:

Auger Electron Spectroscopy

Outline 1.Introduction 2.Principle of AES 3.Instrumentation 3.1 UHV environment 3.2 Electron gun 3.3 Electron energy analyzer 3.4 Electron detector 3.5 Data recording, processing, and output system 4. Advantages 5. Disadvantages / Limitations

1-Introduction Auger Electron Spectroscopy (AES), is a widely used technique to investigate the composition of surfaces of solids. First discovered in 1923 by Lise Meitner and later independently discovered once again in 1925 by Pierre Auger. It can also be used for the study of oxidation catalysis, chemistry of fractured interfaces and grain boundries.

2-Principle of AES A fine focused electron beam bombards the sample and ejects an electron of the inner shell of the atom. This vacancy must be refilled by an electron from a higher energy level. When the higher energy electron fills the hole, the release of energy is transferred to an electron in an outer orbit electron. That electron has sufficient energy to overcome the binding energy and the work function to be ejected with a characteristic kinetic energy.

The ejected electron is referred to as an Auger electron after Pierre Auger. The Auger process require three electrons, thus we can not detect H and He but can detect all other elements from Li on up.

3-Instrumentation The essential components of an AES spectrometer are UHV environment Electron gun Electron energy analyzer Electron detector Data recording, processing, and output system

The sample is irradiated with electrons from an electron gun. The emitted secondary electrons are analyzed for energy by an electron spectrometer. The experiment is carried out in a UHV environment because the AES technique is surface sensitive due to the limited mean free path of electrons in the kinetic energy range of 20 to 2500 eV.

3.1-UHV Environment UHV is the abbreviation of ultra high vacuum. UHV is required for the surface analysis for the following reasons. – To remove absorbed gases from the sample. – To eliminate absorption of contaminants on the sample. – To prevent arcing and high voltage breakdown. – To increase the mean free path for electrons, ions and photons.

3.2-Electron Gun The nature of the electron gun used for AES analysis mainly depends upon three factors: --The speed of analysis (requires a high beam current). --The desired spatial resolution. --Beam-induced which changes to the sample surface. The range of beam currents normally used in AES is between 10 –9 and 5.10 –6 A. The lower current gives high spatial resolution whereas the higher current may be used to give speed and high sensitivity where spatial resolution is of little concern.

In certain samples the high current used may induce surface damage to the specimen and should be avoided. The electron gun optical system has two critical components. i- The electron source In most cases the electron source is thermionic but for the highest spatial resolution the brighter field emission source may be used.

The field emission sources have problems of cost and stability and are therefore limited in their use. ii- The focus forming lens The electron lenses used to focus the beam may be either magnetic or electrostatic. The magnetic lenses have low aberrations and therefore give the best performance. However, these lenses are complicated and expensive. The electrostatic lenses are easier to fit in a UHV system.

3.3-Electron Energy Analyzer The function of an electron energy analyzer is to disperse the secondary emitted electrons from the sample according to their energies. An analyzer may be either magnetic or electrostatic. Because electrons are influenced by stray magnetic fields (including the earth’s magnetic field). It is essential to cancel these fields within the enclosed volume of the analyze. The stray magnetic field cancellation is accomplished by using Mu metal shielding.

Mu-metal is a range of nickel-iron alloys that are composed of approximately 77% nickel, 16% iron, 5% copper and 2%chromium or molybdenum. The high permeability makes mu-metal useful for shielding against static or low-frequency magnetic fields. Electrostatic analyzers are used in all commercial spectrometers today because of the relative ease of stray magnetic field cancellation.

Electron energy analyzer Five-layer mu-metal box. Each layer is about 5 mm thick. It reduces the Earth's magnetic field inside by about 1500 times.

3.4-Electron Detector Having passed through the analyzer, the secondary electrons of a particular energy are spatially separated from electrons of different energies. Various detectors are used to detect these electrons. i- Single-Channel Detector (SCD) The detector used in conventional instrumentation is a channel electron multiplier. It is an electrostatic device that uses a continuous dynode surface which is a thin-film conductive layer on the inside of a tubular channel.

It requires only two electrical connections to establish the conditions for electron multiplication. The output of this detector consists of a series of pulses that are fed into a pulse amplifier/ discriminator and then into a computer. The advantage of such a detector is that it can be exposed to air for a long time without damage. It counts electrons with a high efficiency. The only drawback is that a high count rate causes a saturation effect.

ii- Multi-Channel Detector (MCD) A multiple detection system can be added at the output of the analyzer. The system may be in the form of a few multiple, parallel, equivalent detector chains or position- sensitive detectors spread across the whole of the analyzer output slit plane.

3.5-Data Recording, Processing, and Output System The Auger electrons appear as peaks on a smooth background of secondary electrons. The background is usually sloping therefore, the Auger spectra are usually recorded in a differential form. In the differential mode it is easy to increase the system gain to reveal detailed structure not directly visible in the undifferentiated spectrum. At present, the data in commercial instruments are acquired digitally and can be presented in either analog or digital mode.

A conventional Auger electron spectrometer uses a lock-in amplifier. The oscillator in this amplifier superimposes a sinusoidal modulation on the potential applied to the outer cylinder of the analyzer. The AC component of the signal is decoupled from the multiplier high voltage and detected in the lock- in amplifier. The output is then fed to an x–y recorder.

The amplitude of the modulation is chosen to yield a compromise between sensitivity and resolution. A typical modern Auger electron spectrometer collects the data in the N(E) versus E integral mode. The data are then mathematically differentiated using computer software to yield dN(E)/dE versus E Auger spectra.

4-Advantages Surface sensitive. Elemental and chemical composition analysis by comparison with standard samples of known composition. Detection of elements heavier than Li. Very good sensitivity for light elements. Depth profiling analysis: quantitative compositional information as a function of depth below the surface. Spatial distribution of the elements (SAM): Elemental or even chemical Auger maps analysis in lines, points and areas.

5-Disadvantages / Limitations Analyzes conducting and semiconducting samples. Special procedures are required for non-conducting samples. Only solid specimens can be analyzed. Samples that decompose under electron beam irradiation cannot be studied. Quantification is not easy. Hydrogen and helium are not detectable as they have electrons less than three.

The Auger spatial resolution common to most commercial instruments is of the order of 0.2 μm. or less and is a function of analysis time. The sampling depth is about three mono-layers.