Scintillation (physics)

Scintillation is an example of luminescence, whereby light of a characteristic spectrum is emitted following the absorption of radiation. The scintillation process can be summarized in three main stages: conversion, transport and energy transfer to the luminescence center, and luminescence. The emitted radiation is usually less energetic than the absorbed radiation, hence scintillation is generally a down-conversion process. == Conversion processes ==

The first stage of scintillation, conversion, is the process where the energy from the incident radiation is absorbed by the scintillator and highly energetic electrons and holes are created in the material. The energy absorption mechanism by the scintillator depends on the type and energy of radiation involved. For highly energetic photons such as X-rays (0.1 keV E_{\gamma} E_{\gamma} > 100 keV), three types of interactions are responsible for the energy conversion process in scintillation: photoelectric absorption, Compton scattering, and pair production, which only occurs when E_{\gamma} > 1022 keV, i.e. the photon has enough energy to create an electron-positron pair. These processes have different attenuation coefficients, which depend mainly on the energy of the incident radiation, the average atomic number of the material and the density of the material. Generally the absorption of high energy radiation is described by: :I= I_0\cdot e^{-\mu d} where I_0 is the intensity of the incident radiation, d is the thickness of the material, and \mu is the linear attenuation coefficient, which is the sum of the attenuation coefficients of the various contributions: :\mu = \mu_{pe} + \mu_{cs} + \mu_{pp} + \mu_{oc} At lower X-ray energies (E_{\gamma} \lesssim 60 keV), the most dominant process is the photoelectric effect, where the photons are fully absorbed by bound electrons in the material, usually core electrons in the K- or L-shell of the atom, and then ejected, leading to the ionization of the host atom. The linear attenuation coefficient contribution for the photoelectric effect is given by: :\mu_{pe} \propto {\rho Z^n \over E_{\gamma}^{3.5}} where \rho is the density of the scintillator, Z is the average atomic number, n is a constant that varies between 3 and 4, and E_{\gamma} is the energy of the photon. At low X-ray energies, scintillator materials with atoms with high atomic numbers and densities are favored for more efficient absorption of the incident radiation. At higher energies (E_{\gamma} \gtrsim 60 keV) Compton scattering, the inelastic scattering of photons by bound electrons, often also leading to ionization of the host atom, becomes the more dominant conversion process. The linear attenuation coefficient contribution for Compton scattering is given by: which is much faster than the average decay time in photoluminescence. == Charge transport of excited carriers ==

The second stage of scintillation is the charge transport of thermalized electrons and holes towards luminescence centers and the energy transfer to the atoms involved in the luminescence process. In this stage, the large number of electrons and holes that have been generated during the conversion process, migrate inside the material. This is probably one of the most critical phases of scintillation, since it is generally in this stage where most loss of efficiency occur due to effects such as trapping or non-radiative recombination. These are mainly caused by the presence of defects in the scintillator crystal, such as impurities, ionic vacancies, and grain boundaries. The charge transport can also become a bottleneck for the timing of the scintillation process. The charge transport phase is also one of the least understood parts of scintillation and depends strongly on the type material involved and its intrinsic charge conduction properties. ==Luminescence==

Once the electrons and holes reach the luminescence centers, the third and final stage of scintillation occurs: luminescence. In this stage the electrons and holes are captured potential paths by the luminescent center, and then the electrons and hole recombine radiatively. The exact details of the luminescence phase also depend on the type of material used for scintillation. Inorganic crystals For photons such as gamma rays, thallium activated NaI crystals (NaI(Tl)) are often used. For a faster response (but only 5% of the output) CsF crystals can be used. Organic scintillators In organic molecules scintillation is a product of π-orbitals. Organic materials form molecular crystals where the molecules are loosely bound by Van der Waals forces. The ground state of 12C is 1s2 2s2 2p2. In valence bond theory, when carbon forms compounds, one of the 2s electrons is excited into the 2p state resulting in a configuration of 1s2 2s1 2p3. To describe the different valencies of carbon, the four valence electron orbitals, one 2s and three 2p, are considered to be mixed or hybridized in several alternative configurations. For example, in a tetrahedral configuration the s and p3 orbitals combine to produce four hybrid orbitals. In another configuration, known as trigonal configuration, one of the p-orbitals (say pz) remains unchanged and three hybrid orbitals are produced by mixing the s, px and py orbitals. The orbitals that are symmetrical about the bonding axes and plane of the molecule (sp2) are known as σ-electrons and the bonds are called σ-bonds. The pz orbital is called a π-orbital. A π-bond occurs when two π-orbitals interact. This occurs when their nodal planes are coplanar. In certain organic molecules π-orbitals interact to produce a common nodal plane. These form delocalized π-electrons that can be excited by radiation. The de-excitation of the delocalized π-electrons results in luminescence. The excited states of π-electron systems can be explained by the perimeter free-electron model (Platt 1949). This model is used for describing polycyclic hydrocarbons consisting of condensed systems of benzenoid rings in which no C atom belongs to more than two rings and every C atom is on the periphery. The ring can be approximated as a circle with circumference l. The wave-function of the electron orbital must satisfy the condition of a plane rotator: :\psi(x)=\psi(x+l) \, The corresponding solutions to the Schrödinger wave equation are: :\begin{align} \psi_0 &= \left( \frac{1}{l} \right)^{\frac{1}{2}} \\ \psi_{q1} &= \left( \frac{2}{l} \right)^{\frac{1}{2}} \cos{\left( \frac{2\pi\ qx}{l} \right)} \\ \psi_{q2} &= \left( \frac{2}{l} \right)^{\frac{1}{2}} \sin{\left( \frac{2\pi\ qx}{l} \right)} \\ E_q &= \frac{q^2\hbar^2}{2m_0l^2} \end{align} where q is the orbital ring quantum number; the number of nodes of the wave-function. Since the electron can have spin up and spin down and can rotate about the circle in both directions all of the energy levels except the lowest are doubly degenerate. The above shows the π-electronic energy levels of an organic molecule. The process of absorption of radiation followed by molecular vibration to the excited singlet state S1 and subsequent de-excitation to the ground state S0 (an "allowed" transition resulting in photon emission) is called the "fast component" or fluorescence. Triplet states decay with a much longer decay time than singlet states; this "slow component" can arise from either delayed fluorescence (e.g., thermally activated delayed fluorescence, triplet-triplet annihilation) or phosphorescence (if the decay from triplet state to ground state involves a "forbidden" transition with a change in spin multiplicity). Depending on the particular energy loss of a certain particle (dE/dx), the "fast" and "slow" components are occupied in different proportions. The relative intensities in the light output of these components thus differs for different dE/dx. This property of scintillators allows for pulse shape discrimination: it is possible to identify which particle was detected by looking at the pulse shape. Of course, the difference in shape is visible in the trailing side of the pulse, since it is due to the decay of the excited states. ==See also==