58 research outputs found

    Design and modelling of ring resonators used as optical filters for communications applications

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    This project is a theoretical study of multiple coupled ring resonators, which offer potential applications as demultiplexing filters in DWDM optical transmission systems. The rings can be fabricated as integrated optical structures or they can be formed using micro- or nano-optical fibres. Our approach is analytical, which provides detailed predictions with minimal computer resources. The ideal filter spectral profile for most applications is as close as possible to a rectangle (known as “box-like”) and in order to achieve this we design and model multiple ring resonators. We formulate the compound ring resonator theory with complex field equations to account for phase and amplitude. Then we calculate the transfer functions. We do it in two ways: one way is using linear equations and the other is by matrix theory. We apply both methodologies to one-, two- and three-ring resonators and we show how the matrix formalism can be extended to model arrays of N identical rings. By using the transfer functions we provide detailed physical interpretations of the spectra which are required to design good filter characteristics. We show that rings of equal circumferences provide the best profiles and we derive simple analytical formulas, called “degeneracy condition”, to predict the required coupler ratios for two- and three-ring resonators. It is thus possible to provide a transfer function with single peaks of equal and unity magnitude and a depth of modulation that we choose. Provided that the couplers within the rings conform to the degeneracy condition, we can predict the finesse of a double-ring transfer function. We further extend the ring resonator matrix theory to N identical rings by using a method called “diagonal decomposition”. The amplitude transfer function for N rings can thus be derived with this more advanced mathematical technique. The result that we obtain is in a format that can be extended in future more extended studies. Throughout this project our aim is to provide tangible design guidelines for compound ring resonators, with their potential application to telecommunications networks in mind

    Event-by-event reconstruction of the shower maximum XmaxX_{\mathrm{max}} with the Surface Detector of the Pierre Auger Observatory using deep learning

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    Reconstruction of Events Recorded with the Water-Cherenkov and Scintillator Surface Detectors of the Pierre Auger Observatory

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    Status and performance of the underground muon detector of the Pierre Auger Observatory

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    The XY Scanner - A Versatile Method of the Absolute End-to-End Calibration of Fluorescence Detectors

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    First results from the AugerPrime Radio Detector

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    Update of the Offline Framework for AugerPrime

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    Outreach activities at the Pierre Auger Observatory

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    The ultra-high-energy cosmic-ray sky above 32 EeV viewed from the Pierre Auger Observatory

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    A search for ultra-high-energy photons at the Pierre Auger Observatory exploiting air-shower universality

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    The Pierre Auger Observatory is the most sensitive detector to primary photons with energies above ∼0.2 EeV. It measures extensive air showers using a hybrid technique that combines a fluorescence detector (FD) with a ground array of particle detectors (SD). The signatures of a photon-induced air shower are a larger atmospheric depth at the shower maximum (Xmax_{max}) and a steeper lateral distribution function, along with a lower number of muons with respect to the bulk of hadron-induced background. Using observables measured by the FD and SD, three photon searches in different energy bands are performed. In particular, between threshold energies of 1-10 EeV, a new analysis technique has been developed by combining the FD-based measurement of Xmax_{max} with the SD signal through a parameter related to its muon content, derived from the universality of the air showers. This technique has led to a better photon/hadron separation and, consequently, to a higher search sensitivity, resulting in a tighter upper limit than before. The outcome of this new analysis is presented here, along with previous results in the energy ranges below 1 EeV and above 10 EeV. From the data collected by the Pierre Auger Observatory in about 15 years of operation, the most stringent constraints on the fraction of photons in the cosmic flux are set over almost three decades in energy
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