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Ionization energy loss

Used effects Phonon excitation (20 meV-1 eV) Plasmon and interband excitations (1-50 eV) Inner-shell ionization (A = ionization energy loss) Emission of x-ray (continuous/characteristic, analytical EM)... [Pg.1626]

Fig. 5 illustrates the relative dependence of the fluorescence yield of the 337 nm line on different electron energies at a pressure of 400 hPa. The drawn curve corresponds to the Bethe-Bloch function [6] for ionization energy loss which was fitted to the data by a constant factor. The statistics in this plot is still very limited but the number of emitted fluorescence photons indeed seems to be proportional to the energy loss as it is suggested by Eq. (2). [Pg.407]

Equation 4.7, relating radiation to ionization energy loss, is a function of the kinetic energy of the particle. As the particle slows down, T decreases and (d /dr)rad also decreases. The total energy radiated as bremsstrahlung is approximately equal in MeV to ... [Pg.130]

The ionization energy loss of non-relativistic electrons can be approximated (Vertes and Kiss 1987) as... [Pg.377]

Figure 8.7 presents ionization energy loss curves for electrons in some common materials. [Pg.377]

Critical energy, in general, is defined as the particle energy at which the ionization energy loss equals the radiation one. As the radiation losses depend very sensitively on the absorber... [Pg.378]

Electron-impact energy-loss spectroscopy (EELS) differs from other electron spectroscopies in that it is possible to observe transitions to states below the first ionization edge electronic transitions to excited states of the neutral, vibrational and even rotational transitions can be observed. This is a consequence of the detected electrons not originating in the sample. Conversely, there is a problem when electron impact induces an ionizing transition. For each such event there are two outgoing electrons. To precisely account for the energy deposited in the target, the two electrons must be measured in coincidence. [Pg.1307]

The infonnation from energy-loss measurements of transitions mto the contimiiim, that is, ionizing excitations, is significantly diminished because the energy of the ionized electron is not known. The problem can be overcome by... [Pg.1326]

Figure Bl.6.12 Ionization-energy spectrum of carbonyl sulphide obtained by dipole (e, 2e) spectroscopy [18], The incident-electron energy was 3.5 keV, the scattered incident electron was detected in the forward direction and the ejected (ionized) electron detected in coincidence at 54.7° (angular anisotropies cancel at this magic angle ). The energy of the two outgoing electrons was scaimed keeping the net energy loss fixed at 40 eV so that the spectrum is essentially identical to the 40 eV photoabsorption spectrum. Peaks are identified with ionization of valence electrons from the indicated molecular orbitals. Figure Bl.6.12 Ionization-energy spectrum of carbonyl sulphide obtained by dipole (e, 2e) spectroscopy [18], The incident-electron energy was 3.5 keV, the scattered incident electron was detected in the forward direction and the ejected (ionized) electron detected in coincidence at 54.7° (angular anisotropies cancel at this magic angle ). The energy of the two outgoing electrons was scaimed keeping the net energy loss fixed at 40 eV so that the spectrum is essentially identical to the 40 eV photoabsorption spectrum. Peaks are identified with ionization of valence electrons from the indicated molecular orbitals.
The occurrence of fine structures has already been noted in the sections on spectral information and ionization losses (Sects. 2.5.3 and 2.5.3.2). In the following text some principal considerations are made about the physical background and possible applications of both types of feature, i. e. near-edge and extended energy-loss fine structures (ELNES/EXELFS). A wealth of more detailed information on their usage is available, especially in textbooks [2.171, 2.173] and monographs [2.210-2.212]. [Pg.62]

The total energy, E, is obtained from the total charge accumulated in both sections of the anode. The second part of the ionization chamber, which measures the energy E - AE, can be replaced by an SBD [3.167], and the first part, which measures the energy loss AE, by a transmission SBD [3.168, 3.169]. When SBDs are used to measure heavy ions, radiation damage of the detector by the ions must be taken into account. [Pg.165]

A strongly negative standard potential indicates a tendency to undergo oxidation, which involves loss of electrons. Elements at the left of the d block have lower ionization energies than those at the right. [Pg.1015]

Experiments and calculations both indicate that electron transfer from potassium to water is spontaneous and rapid, whereas electron transfer from silver to water does not occur. In redox terms, potassium oxidizes easily, but silver resists oxidation. Because oxidation involves the loss of electrons, these differences in reactivity of silver and potassium can be traced to how easily each metal loses electrons to become an aqueous cation. One obvious factor is their first ionization energies, which show that it takes much more energy to remove an electron from silver than from potassium 731 kJ/mol for Ag and 419 kJ/mol for K. The other alkali metals with low first ionization energies, Na, Rb, Cs, and Fr, all react violently with water. [Pg.1369]


See other pages where Ionization energy loss is mentioned: [Pg.166]    [Pg.42]    [Pg.303]    [Pg.130]    [Pg.341]    [Pg.50]    [Pg.166]    [Pg.42]    [Pg.303]    [Pg.130]    [Pg.341]    [Pg.50]    [Pg.1124]    [Pg.1306]    [Pg.1317]    [Pg.1320]    [Pg.1322]    [Pg.1323]    [Pg.1323]    [Pg.1324]    [Pg.1324]    [Pg.1625]    [Pg.481]    [Pg.103]    [Pg.145]    [Pg.151]    [Pg.176]    [Pg.359]    [Pg.361]    [Pg.493]    [Pg.40]    [Pg.52]    [Pg.56]    [Pg.59]    [Pg.59]    [Pg.65]    [Pg.67]    [Pg.142]    [Pg.81]    [Pg.433]    [Pg.11]   
See also in sourсe #XX -- [ Pg.377 , Pg.378 ]




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