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Time constants radiative

Following a b-pulsc excitation, a fraction of excited molecules can reach the triplet state, from which they return to the ground state either radiatively or non-radiatively. The concentration of molecules in the triplet state decays exponentially with a time constant tt representing the lifetime of the triplet state... [Pg.44]

This process is unfavorable because it involves a change in spin, a change in A of two, and a g —> g transition. Thus its probability is relatively low, which is reflected in a time constant for radiative decay of almost an hour. Similarly, the cross section for production of 02 (1 Ag) by photon absorption from the ground state... [Pg.20]

For a lumped detector active junction (bismuth and tellurium layers of thickness 5-1 and 82, respectively, and surface area. 4), neglecting the conductive loss to the Mylar as well as the convective and radiative losses to the ambient, determine (a) the steady temperature, (b) the unsteady temperature, and (c) the time constant of the thermopile. [Pg.183]

The dynamics of the photochemical process involving the ZnTPPS-ZnTMPyP ion pair has been recently investigated by pump-probe transient absorption. The transient absorption responses shown in Figure 11.10 were obtained by pumping the porphyrins at 560 nm and probing at 510 nm. It should be indicated that the depopulation of the Si state for ZnTPPS and ZnTMPyP in their monomeric form exhibits time constants of 1.6 and 0.6 ns, respectively. As mentioned before, this relaxation mainly contains contribution from radiative... [Pg.528]

D-A where Eu is in the excited state, and A is the D-A pair where RET has occurred and the acceptor is in the excited state. The donor emission at 615 nm corresponds to model I. We should observe rally a single lifetime, the inverse of the sum of rate coefficients, l/(A io + itia). In fact, we observe three time constants. The presence of the first of them, 0.983 ms, corresponds to the donor alone without any RET and is expected due to incomplete labeling. Obviously 13 = 0.148 ms corresponds to the radiative Dq —> F2 transition. This is within the error margins, the same as the first lifetime of the acceptor, 0.145 ms. According to (32) and (34), the... [Pg.303]

Figure 7.10 LIF lifetime measurements, following an excitation laser pulse of duration At = 4.5 ns FWHM. If the lifetime of the excited levelis longerthan the excitation pulse, then the lifetime can be extracted from theslopeof the semi-logarithmic plot (trace a) if the radiative lifetime signal is detected with electronics of similar time constants, then / C-response deconvolution needs to be applied (trace b) and if the lifetime is of similar length or slightly shorter than the laser pulse, full line shape function deconvolution procedures are required (trace c). Data shown in trace (b) are adapted from Verdasco et al Laser Chem., 1990, 10 239, with permission of Taylor Francis Group... Figure 7.10 LIF lifetime measurements, following an excitation laser pulse of duration At = 4.5 ns FWHM. If the lifetime of the excited levelis longerthan the excitation pulse, then the lifetime can be extracted from theslopeof the semi-logarithmic plot (trace a) if the radiative lifetime signal is detected with electronics of similar time constants, then / C-response deconvolution needs to be applied (trace b) and if the lifetime is of similar length or slightly shorter than the laser pulse, full line shape function deconvolution procedures are required (trace c). Data shown in trace (b) are adapted from Verdasco et al Laser Chem., 1990, 10 239, with permission of Taylor Francis Group...
The fact that saturation is often not observed must mean that there are non-radiative processes by which p nuclear spins can become a spins again and hence help to maintain the population difference between the two sites. The nonradi-ative return to an equilibrium distribution of populations in a system (eqn 13.9) is an aspect of the process called relaxation. If we were to imagine forming a system of spins in which all the nuclei were in their p state, then the system returns exponentially to the equilibrium distribution (a small excess of a spins over p spins) with a time constant called the spin-lattice relaxation time, T, (Fig. 13.25). [Pg.530]

The spherical shock wave produces nitric oxide by heating air to temperatures above 2200 K. This air is subsequently cooled by rapid expansion and radiative emission, while the shock front moves out to heat more air. At a particular temperature the cooling rate becomes faster than the characteristic time constant for maintaining equilibrium between NO and air. For cooling times of seconds to milliseconds the NO concentration freezes at temperatures between 1700 and 2500 K, corresponding to NO concentrations of 0.3-2 %. Gilmore [72] estimates a yield of 0.8 x 10 NO molecules per Mt for this mechanism. [Pg.146]


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See also in sourсe #XX -- [ Pg.215 ]




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Radiative constant

Time constant

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