Vary initials in XPS smoothly

Aug 6th, 2022
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How to Vary initials in XPS

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hello friends welcome to the second part of the complete series on photoemission spectroscopy in the previous video we have seen the basic principles and instrumentation of xps if you have missed that video you can find the link for the first video in description box now lets talk about the spectra obtained from the xps instrument we have seen that the instrument gives a plot of kinetic energy versus the number of electrons counted so number of electrons counted is plotted in y-axis and kinetic energy is plotted in x-axis so now you can see that it starts from the lower kinetic energy in the left and goes to higher kinetic energy in right as normally a graph is plotted but in most of the modern instruments kinetic energy is converted to binding energy with the formula h nu is equals to binding energy plus kinetic energy plus phi therefore the lower kinetic energy becomes higher binding energy and higher kinetic energy becomes lower binding energy this means now x-axis starts from high

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In most cases, XPS analysis samples many particles or many grains in a polycrystalline material, while EDX analysis may sample only one particle or one grain. EDX analysis may require many more sets of data to achieve an accurate average simply due to local sample inhomogeneity.
In XPS, the occupation of the 4d orbital of Pd controls the initial state shift offering information about the hybridization of the cluster, while the size and the charging of the cluster controls the final state shift.
The perturbation is called shake-up if they refer to an excitation in the final system, or shake-off if the result is the loss of one or more outer shell electrons from the ion.
Hence, the XPS spectrum maps the final states, i.e., energy differences between the ground state of the sample and the numerous final (or ionized) states.
Initial state effects describe any effect that results from the electronic structure of an atom/ion undergoing photoelectron emission that was present prior to the photoelectron emission process. These effects are split into two subgroups: Spin-induced interactions present within the photoelectron emitting atom/ion.
Ultraviolet Photoelectron Spectroscopy (UPS) operates on the same principle as XPS, but ultraviolet (UV) radiation is used to induce the photoelectric effect. UV photons are produced using a gas discharge lamp, typically filled with helium and have energies of 21.2eV (He I) and 40.8eV (He II).
The greater the binding energy, the greater the attraction of that electron to the nucleus. i.e. peaks from electrons in 1s will have a greater energy than peaks representing electrons from 2s. Electrons in 2s will have greater energy than those in 2p.
X-ray photoelectron spectroscopy (XPS) is a surface analytical technique, which is based upon the photoelectric effect. Each atom in the surface has core electron with the characteristic binding energy that is conceptually, not strictly, equal to the ionization energy of that electron.
The shifts in the XPS peak is related to its oxidation state and higher shift in binding energy corresponds to higher oxidation state. Some times more shift with noise peak is related to the satellite peak or shake up and it is a case for only some metal or its oxide for example Ni or NiO.
X-ray Photoelectron Spectroscopy (XPS) uses soft x-rays (with a photon energy of 200-2000 eV) to examine electrons in core-levels. Ultraviolet Photoelectron Spectroscopy (UPS) using vacuum UV radiation (with a photon energy of 10-45 eV) to examine electrons in valence levels.

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