Scintillation based gamma-ray detectors are widely used in medical imaging, high-energy physics, astronomy and national security. Scintillation gamma-ray detectors are field-tested, relatively inexpensive, and have good detection efficiency. Semi-conductor detectors are gaining popularity because of their superior capability to resolve gamma-ray energies. However, they are relatively hard to manufacture and therefore, at this time, not available in as large formats and much more expensive than scintillation gamma-ray detectors. Scintillation gamma-ray detectors consist of: a scintillator, a material that emits optical (scintillation) photons when it interacts with ionization radiation, and an optical detector that detects the emitted scintillation photons and converts them into an electrical signal. Compared to semiconductor gamma-ray detectors, scintillation gamma-ray detectors have relatively poor capability to resolve gamma-ray energies. This is in large part attributed to the "statistical limit" on the number of scintillation photons. The origin of this statistical limit is the assumption that scintillation photons are either Poisson distributed or super-Poisson distributed. This statistical limit is often defined by the Fano factor. The Fano factor of an integer-valued random process is defined as the ratio of its variance to its mean. Therefore, a Poisson process has a Fano factor of one. The classical theory of light limits the Fano factor of the number of photons to a value greater than or equal to one (Poisson case). However, the quantum theory of light allows for Fano factors to be less than one. We used two methods to look at the correlations between two detectors looking at same scintillation pulse to estimate the Fano factor of the scintillation photons. The relationship between the Fano factor and the correlation between the integral of the two signals detected was analytically derived, and the Fano factor was estimated using the measurements for SrI₂:Eu, YAP:Ce and CsI:Na. We also found an empirical relationship between the Fano factor and the covariance as a function of time between two detectors looking at the same scintillation pulse. This empirical model was used to estimate the Fano factor of LaBr₃:Ce and YAP:Ce using the experimentally measured timing-covariance. The estimates of the Fano factor from the time-covariance results were consistent with the estimates of the correlation between the integral signals. We found scintillation light from some scintillators to be sub-Poisson. For the same mean number of total scintillation photons, sub-Poisson light has lower noise. We then conducted a simulation study to investigate whether this low-noise sub-Poisson light can be used to improve spatial resolution. We calculated the Cramér-Rao bound for different detector geometries, position of interactions and Fano factors. The Cramér-Rao calculations were verified by generating simulated data and estimating the variance of the maximum likelihood estimator. We found that the Fano factor has no impact on the spatial resolution in gamma-ray imaging systems.

abstract: Nuclear proliferation concerns have resulted in a desire for radiation detectors with superior energy resolution. In this dissertation a Monte Carlo code is developed for calculating energy resolution in gamma-ray detector materials. The effects of basic material properties such as the bandgap and plasmon resonance energy are studied using a model for inelastic electron scattering based on electron energy-loss spectra. From a simplified "toy model" for a generic material, energy resolution is found to oscillate as the plasmon resonance energy is increased, and energy resolution can also depend on the valence band width. By incorporating the model developed here as an extension of the radiation transport code Penelope, photon processes are also included. The enhanced version of Penelope is used to calculate the Fano factor and average electron-hole pair energy in semiconductors silicon, gallium arsenide, zinc telluride, and scintillators cerium fluoride and lutetium oxyorthosilicate (LSO). If the effects of the valence band density-of-states and phonon scattering are removed, the calculated energy-resolution for these materials is fairly close to that for a toy model with a uniform electron energy-loss probability density function. This implies that the details of the electron cascade may in some cases have only a marginal effect on energy resolution. / Dissertation/Thesis / Ph.D. Physics 2011

Previous studies have shown that it is possible for juvenile songbirds to learn songs through listening to prerecorded songs played back to them. What is not known however, is how this will differ from normal learning, both on neural level as well as on the bird as whole. In this project we have taken data from playback experiments and attempted to measure the differences in neuron spiking activity across two different contexts. Firstly, when the bird is only listening to playback recordings and secondly when the bird is listening to playback recordings on the same day as listening to a live tutor. We analysed the spiking activity with several different methods in order to establish a distinction between these contexts that could be seen across birds and across trials. The methods include analysing joint spiking events as binary spike trains, the Fano factor across trials as well as the variability of the spike rate. Our hypothesis was that the birds would learn more effectively on days when exposed to a live tutor, therefore, the playback days would show much higher and much more varied spiking data. From our results we found many cases when this hypothesis is true. However, it does not hold true for each of the birds, as some are offered similar results in either context. Therefore we believe that further study would be required to get conclusive results. Although, our results tend to favour the tutoring days it is only suggestive that this shows evidence of better learning. / Tidigare studier har visat att det är möjligt för unga sångfåglar att lära sig sånger genom att lyssna på förinspelade läten som spelas upp för dem. Vad som dock inte är känt är hur detta sätt kommer att skilja sig, jämfört med normalt lärande, både på neural nivå och på fågeln som helhet. I detta projekt har vi tagit data från ett uppspelningsexperiment och försökt mäta skillnaderna neuronspikande aktiviteter i två fall. I det första fallet lyssnar fågeln bara på inspelad fågelsång och i det andra fallet lyssnar fågeln på inspelad fågelsång samma dag som den lyssnar på en vuxen fågel som mentor. Vi analyserade spikningsaktiviteten med flera olika metoder för att finna en skillnad mellan dessa fall, som kan ses både mellan fåglar och mellan ollika försök. Metoderna inkluderar analys av gemensamma spikinghändelser som binära spiktåg, Fanofaktorn över försöken samt variationen i spikhastigheten. Vår hypotes var att fåglarna skulle lära sig mer effektivt på dagar när de utsattes för en vuxen fågel som mentor, därför skulle uppspelningsdagarna visa mycket högre och mycket mer varierad spikdata. Från våra resultat fann vi att i många fall där hypotesen är sann. Men den stämmer inte för alla fåglarna eftersom några fåglar hade liknande resultat för båda fallen. Därför tror vi att ytterligare studier krävs för att få tydliga resultat. Dock så tenderar våra resultat att gynna mentordagarna, även om det bara antyder att detta visar på bättre lärande.

No description available.

Cette thèse est consacrée à l'étude expérimentale du bruit quantique électronique d'un système mésoscopique. Dans une première partie, nous nous sommes intéressés au bruit de partition d'un conducteur unidimensionnel balistique : un contact ponctuel quantique (QPC). Nous avons montré que, lorsque l'un des contacts du QPC est modulé par une onde radio-fréquence, il apparaît un bruit de partition en l'absence de courant moyen à travers le conducteur. Nous avons ainsi validé la théorie de la diffusion appliquée au bruit photo-assisté, d'une part en mesurant le facteur de Fano en l'absence de tension appliquée au QPC, et d'autre part en mesurant le bruit en présence d'une tension continue et d'une irradiation micro-onde. Dans une seconde partie, nous avons testé le système de mesure d'une nouvelle expérience qui, à terme, permettra de mesurer le bruit à haute fréquence d'un conducteur mésoscopique, ainsi que la statistique des photons qu'il émet dans le circuit de mesure. Le test a consisté à réaliser des expériences de type Hanbury-Brown et Twiss (interférométrie d'intensité) avec deux types de sources de photons micro-ondes. D'abord, nous avons utilisé une source thermique incohérente (résistance macroscopique de 50 Ohms) qui présente une statistique super-poissonnienne : les fluctuations de puissance sont proportionnelles au carré de la puissance moyenne émise par la source. Puis nous avons mis en évidence la statistique poissonnienne d'une source classique monochromatique, et nous avons montré que le facteur de Fano géant mesuré est parfaitement expliqué par le bruit des chaînes d'amplification.