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Photoabsorption

Excitation and ionization energies derived from photoabsorption (PA) or dipole (e,e) spectroscopy (simulating PA) and also from multiphoton ionization (MPI) work (which is not accounted for in the following) are reported in the chapters on electronically excited states (p. 144) and on ionization potentials (p. 149). The absolute photoabsorption oscillator strength df/dE and cross section a, related via a(in Mb)=109.75 df/dE(in eV ), were obtained from gas-phase dipole (e,e) spectroscopy [1, 2] and are shown for a large range of photon energies. [Pg.193]

Relative photoion yields of PHJ, PHJ, and PH+ from PH3 were measured between 130 and 55 nm [18]. [Pg.195]


The temi action spectroscopy refers to those teclmiques that do not directly measure die absorption, but rather the consequence of photoabsorption. That is, there is some measurable change associated with the absorption process. There are several well known examples, such as photoionization spectroscopy [47], multi-photon ionization spectroscopy [48], photoacoustic spectroscopy [49], photoelectron spectroscopy [, 51], vibrational predissociation spectroscopy [ ] and optothemial spectroscopy [53, M]. These teclmiques have all been applied to vibrational spectroscopy, but only the last one will be discussed here. [Pg.1173]

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.
Figure B3.4.7. Schematic example of potential energy curves for photo-absorption for a ID problem (i.e. for diatomics). On the lower surface the nuclear wavepacket is in the ground state. Once this wavepacket has been excited to the upper surface, which has a different shape, it will propagate. The photoabsorption cross section is obtained by the Fourier transfonn of the correlation function of the initial wavefimction on tlie excited surface with the propagated wavepacket. Figure B3.4.7. Schematic example of potential energy curves for photo-absorption for a ID problem (i.e. for diatomics). On the lower surface the nuclear wavepacket is in the ground state. Once this wavepacket has been excited to the upper surface, which has a different shape, it will propagate. The photoabsorption cross section is obtained by the Fourier transfonn of the correlation function of the initial wavefimction on tlie excited surface with the propagated wavepacket.
Before progressing, it is useful to review the dynamics of typical molecular systems. We consider three types scattering (chemical reaction), photodissociation, and bound-state photoabsorption (no reaction). [Pg.260]

Recently, Navarro et al. [286] prompted the combination of ZnO and CdO with CdS to improve its photoabsorption ability CdO exhibits a band gap in the interval 2.2-2.4 eV with high transmittance and very low resistance, while ZnO has... [Pg.277]

After the electrolysis for 5 h at —0.15 V with the bubbling of O2 into W, the amount of CO2 produced was found to be 1.6 x 10 moles. A photoabsorption spectrum of the NB after electrolysis gave a peak at 780 nm. The peak was identical with that of the one electron oxidation product of DMFC, DMFC, which had been prepared coulometrically by using a column electrode with glassy carbon fiber working electrode [40]. This fact indicates that the electrolysis product was DMFC. The DMFC produced by the electrolysis was estimated to be 3.08 x 10 moles. [Pg.498]

The adiabatic ionization potential (1A) of a molecule, as shown in Figure 4.1, equals the energy difference between the lowest vibrational level of the ground electronic state of the positive ion and that of the molecule. In practice, few cases would correspond to adiabatic ionization except those determined spectroscopically or obtained in a threshold process. Near threshold, there is a real difference between the photoabsorption and photoionization cross sections, meaning that much of the photoabsorption does not lead to ionization, but instead results in dissociation into neutral fragments. [Pg.72]

The distinction between photoabsorption and photoionization is important, particularly near threshold, where the probability that ionization will not occur upon photoabsorption is significant. Thus, the ionization efficiency is defined by TJ. = a. /photoionization cross section and photoabsorption cross section, is related to the absorption coefficient a by a = n(7, n being the absorber density. [Pg.77]

In Eq. (4.9), V is the frequency of radiation and a>. and (Ox are the statistical weights of the initial and final states. It should be remembered that Eq. (4.9) refers to the photoionization cross section, not the total photoabsorption cross section (see Sect. 4.2). [Pg.94]

The dipole oscillator strength is the dominant factor in dipole-allowed transitions, as in photoabsorption. Bethe (1930) showed that for charged-particle impact, the transition probability is proportional to the matrix elements of the operator exp(ik r), where ftk is the momentum transfer. Thus, in collision with fast charged particles where k r is small, the process is again controlled by dipole oscillator strength (see Sects. 2.3.4 and 4.5). [Pg.102]

The quantity L(0) = In I, where I is the mean excitation potential introduced by Bethe, which controls the stopping of fast particles (see Sect. 2.3.4) L(2) = In K, where K is the average excitation energy, which also enters into the expression for Lamb shift (Bethe, 1947). Various oscillator sum rules have been verified for He and other rare gases to a high degree of accuracy. Their validity is now believed to such an extent that doubtful measurements of photoabsorption and electron-impact cross sections are sometimes altered or corrected so as to satisfy these. [Pg.103]

Bound-state photoabsorption, direct molecular dynamics, nuclear motion Schrodinger equation, 365-373... [Pg.70]

Extensive discussion on the ionization potentials of 1,2,5-thiadiazole and its derivatives can be found in CHEC(1984) and CHEC-II(1996) <1984CHEC(6)513, 1996CHEC-II(4)355>. Hel photoelectron spectroscopy, inner-shell electron energy loss spectroscopy involving the S2p, S2s, Cls and Nls edges, and Sis synchrotron radiation photoabsorption spectroscopy were used to probe the occupied and unoccupied valence levels of benzothiadiazole 2 <1991MI165>. [Pg.523]

J. Berkowitz, Photoabsorption, Photoionization, and Photoelectron Spectroscopy, Academic Press, New York, 1979. [Pg.333]

Rhodopsin is a transmembrane protein linked to 1 l as-retinal, which, on photoabsorption, decomposes to opsin and all-trans-retinal 809... [Pg.807]

Rhodopsin is a transmembrane protein linked to 11-c/s-retinal, which, on photoabsorption, decomposes to opsin and all-f/a/75-retinal. Rhodopsin has a molecular weight of about 40,000. Its C-terminus is exposed on the cytoplasmic surface of the disk, and its sugar-containing... [Pg.809]

The propagation effects of harmonics, which are due to the two processes of the photoabsorption by each gas and the phase (mis-)matching between the harmonics and the fundamental pulse, can be determined by observing harmonic intensities as functions of the gas pressure [11]. Figure 4.7 shows the... [Pg.73]


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Photoabsorption and photoionization

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Photoabsorption measurements

Photoabsorption molecular

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Photoabsorption, cross section

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X-ray photoabsorption

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