Titles: SCNT: Scintillator and wavelength shifter (WLS) additive optical data ============================================================================== Contact: N. Tagg, Oxford Titles Files ------------ scintillator.dat Verification ------------ SCNT ------ Description ----------- The SCNT banks contain data describing the properties of scintillator, wavelength-shifter, or simply an absorber. These are called 'additives', and can be added to the materials in the MEDA bank. The bank number is used as the ID number of a given medium. Data Words - SCNT ------------------- Fixed length Database Header. See titles_dbhdr.html Data types: B(bit), I, F, D(double), H(hollerith 4 char) 1 H NAME The name of the additive. 6 F QE The quantum efficiency of the scintillator, in units of photons/MeV. This is used in computing the photon yield for an ionizing particle. See note 1. 7 F BIRKS The Birk's constant of the scintillator, in Mev/cm 8 I NUM_TIME_COMPONENTS The number of components in the emission time spectrum 9 F TIME_COMPONENTS Array with decay time data, KSCNT_NUM_TIME_COMPONENTS words. See note 2. 19 I EMM_MODE Mode flag for how to interpret emission spectrum data. See note 3. 20 I EMM_N Number of components in the emission profile data. See note 3. 21 F EMM_DATA Array of emission spectrum data. See note 3. Synonyms: EMM_WAVELENGTHS = EMM_DATA EMM_SPECTRUM = EMM_DATA + 20 61 I ABS_N Number of points in absorption spectrum. See note 4. 62 F ABS_WAVELENGTHS Array of KSCNT_ABS_N wavelengths in the absorption spectrum. In nanometers 82 F ABS_SPECTRUM Array of KSCNT_ABS_N absorption lengths, in cm. 92 I WLSQE_N Number of words in WLS quantum efficiency spectrum 93 F WLSQE_WAVELENGTHS Array of KSCNT_WLSQE_N wavelengths. In nanometers 113 F WLSQE_SPECTRUM Array of KSCNT_WLSQE_N quantum efficiencies. See note 5 Notes ----- 1) Scintillation light. If KSCNT_QE is non-zero, the additive will be treated like scintillator. Ionizing particles will generate scintillation photons in the associated medium. The number of photons created by a track of energy deposition dE and track length dX is: NPHOT = concentration * KSCNT_QE * dE / (1 + KSCNT_BIRKS * dE/dX) where the concentration is taken from the associated MEDA bank. 2) Decay time. The scintillator or wavelength shifter is assumed to emit light over time with an probability described as the sum of several exponentials. Example: a fluor with two decay components, described by: I(t)t = 0.3 exp(-t/10ns) + 0.7 exp(-t/20ns) is represented as: KSCNT_NUM_TIME_COMPONENTS = 2 KSCNT_TIME_COMPONENTS: 0.3 10.0 0.7 20.0 3) Emission spectrum. The emission spectrum of the additive can be described in one of two ways: EMM_MODE = 0 The emission is chosen from a user-defined spectrum. There are KSCNT_EMM_N wavelengths at position KSCNT_EMM_WAVELENGTHS and KSCNT_EMM_N intensities at position KSCNT_EMM_SPECTRUM. EMM_MODE = 1 The emission spectrum is represented by a sum of Gaussian peaks. There are KSCNT_EMM_N such peaks. Each peak is represented by three values: Fractional intensity, mean wavelength, and width. E.g. 1 1.0 450. 10. would represent a single line source centered at 450 nm with an RMS width of 10 nm. In both cases, the spectrum is normalized at run-time. 4) Absorption spectrum. This should be filled for both scintillator and WLS. KSCNT_ABS_N points of absorption length can be given, just like for the MEDA banks. Absorption for the medium is treated as an admixture with the basic medium. If the concentration of additive is zero, the absorption is just like that described in the medium. If the concentration is set to 1, the absorption is set to that of the additive. If in between, the absorption is a linear admixture of the two. 5) WLS QE. If the medium acts as a wavelength shifter (i.e. it has a chance of re-emitting a photon after absorbing it) the WLSQE should be set to non-zero. The WLSQE is set as a function of the incident photon wavelength. The SPECTRUM words should vary from 0 to 1, where 1 represents a perfect wavelength shifter (all photons are re-emitted).