A Course in Luminescence Measurements and Analyses for Radiation Dosimetry. Stephen W. S. McKeever
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СКАЧАТЬ where the density of allowed states of a crystalline material (Figure 2.5a) is compared with that of an amorphous material (Figure 2.5b). As with crystalline materials, allowed energy zones do exist, but with non-crystalline materials the density of states Z(E) partially extends into the gap, creating so-called band-tail states. Defect state energies are distributed rather than discrete and can extend above or below the Fermi Level, EF, such that Z(EF) ≠ 0. Localized energy levels (shaded in Figure 2.5b) require absorption of external energy (thermal or optical) to ionize the defects, i.e. to excite the charge carriers (electrons or holes) into the delocalized bands (conduction and valence bands). Thus, a non-crystalline solid can be treated in much the same way as a crystalline solid in the sense that the delocalized bands are separated by an energy gap (more correctly termed a “mobility gap” since Z(E) tail states extend into the gap) with localized states due to defects existing within the gap but with distributions of energy (band-tail states).

      Figure 2.5 Density of states functions Z(E) for (a) a crystalline solid, and (b) an amorphous (non-crystalline) solid. For non-crystalline materials the density of states extends into the band gap (band-tail states) and localized states (shaded) are distributed in energy.

      It should also be mentioned that even crystalline materials can exhibit band-tail states extending into the gap if they exhibit sufficient lattice disorder due to variations in bond lengths, bond angles, local density fluctuations, and/or contain high concentrations of impurities or other extrinsic defects. If the disorder is sufficiently high, it can give rise to a density of states Z(E) that extends into the band gap. Such materials may include, for example, natural minerals, such as the feldspar family or the various polymorphs of silicon dioxide.

      2.2 Trapping, Detrapping, and Recombination Processes

      2.2.1 Excitation Probabilities

      2.2.1.1 Thermal Excitation

      Consider an electron localized at a lattice defect, at energy Et below the conduction band and probability p that the electron will absorb external energy and be excited from the trap into the conduction band. If the temperature of the system is T, the probability per second p that the electron will be thermally excited into the conduction band is given by:

      where v is the lattice phonon vibration frequency, K is the transition probability constant, k is Boltzmann’s constant, F is the Helmholtz free energy = Et−ΔST, and ΔS is the entropy change associated with the transition. Thus:

      p equals nu upper K exp left-brace StartFraction upper Delta upper S Over k EndFraction right-brace exp left-brace minus StartFraction upper E Subscript t Baseline Over k upper T EndFraction right-brace equals s exp left-brace minus StartFraction upper E Subscript t Baseline Over k upper T EndFraction right-brace period (2.2)

      Here, s is known as the “attempt-to-escape” frequency (also known as the “frequency factor,” or the “pre-exponential factor”), with units of s–1. It is the number of times per second that energy is absorbed from phonons in the lattice, and the term exp{−EtkT} is the probability that the energy absorbed is enough to cause a transition from the localized state to the conduction band. Typically, one can expect s ~ 1012–1014 s–1; that is, of the order of the lattice vibration frequency, v, but differing from it by the factor Kexp{ΔSk}.

      By applying equilibrium statistics, it is possible to show that:

      where, Nc is the concentration of available states in the conduction band (units, m–3), ve is the thermal velocity of free electrons (m.s–1) and σ is the capture cross-section for the trap (m2).

      The concentration of free electrons, nc at any given temperature may be written:

      n Subscript c Baseline equals integral Subscript upper E Subscript c Baseline Superscript infinity Baseline upper Z left-parenthesis upper E right-parenthesis f left-parenthesis upper E right-parenthesis d upper E almost-equals upper N Subscript c Baseline exp left-brace minus StartFraction upper E Subscript c Baseline minus upper E Subscript upper F Baseline Over k upper T EndFraction right-brace period (2.4)

      Since the occupancy of the conduction band is essentially zero at the top of the conduction band, the integral can be taken to infinity. It is also assumed that Ec – EF >> kT, which is a good approximation in insulators, even for T = 1000s K. Nc can, therefore, be considered to be the effective density of states of a fictional level lying at the conduction band edge and is defined by:

      Similarly, the number of free holes in the valence band is given by:

      m Subscript v Baseline almost-equals upper M Subscript v Baseline exp left-brace minus StartFraction upper E Subscript upper F Baseline minus upper E Subscript v Baseline Over k upper T EndFraction right-brace (2.6)

      and

      is the density of available states in the valence band. In Equations 2.5 and 2.7, me* and mh* are the effective masses of the free electrons and free holes in the conduction and valence bands, respectively, and h is Planck’s constant.

      Figure 2.6 Potential ϕ as a function of distance r in the СКАЧАТЬ