The use of organic scintillators is an established method for the measurement of neutron spectra above several hundred keV. Fast neutrons are detected largely by proton recoils in the scintillator resulting from neutron elastic scattering with hydrogen. This leads to a smeared rectangular pulse-height distribution for monoenergetic neutrons. The recoil proton distribution ranges in energy from zero to the incident neutron energy. In addition, the pulse-height distribution is further complicated by structure due to energy deposition from alpha particle recoils from interactions with carbon as well as carbon recoils themselves. In order to reconstruct the incident neutron spectrum, the pulse-height spectrum has to be deconvoluted (unfolded) using the computed or measured response of the scintillator to monoenergetic neutrons. In addition gamma rays, which are always present when neutrons are present, lead to Compton electron recoils in the scintillator. Fortunately, for certain organic scintillators, the electron recoil events can be separated from the heavier particle recoil events in turn to distinguish gamma-ray induced events from neutron-induced events. This is accomplished by using the risetime of the pulse from the organic scintillator seen in the photomultiplier tube as a decay of light. In this work, an organic scintillator detection system was assembled which includes neutron-gamma separation capabilities to store the neutron-induced and gamma-induced recoil spectra separately. An unfolding code was implemented to deconvolute the spectra into neutron and gamma energy spectra. In order to verify the performance of the system, a measurement of two reference neutron fields will be performed with the system, unmoderated Cf-252 and heavy-water moderated Cf-252. After the detection system has been verified, measurements will be made with an AmBe neutron source.

Particle physics experiments with low event rates highly depend on background suppression methods. Neutron component of the ambient background radiation is especially problematic since neutrons are difficult to shield directly. TEXONO collaboration has employed a hybrid neutron detector composed of two different scintillating materials to measure the neutron background directly in the Kuo-Sheng Neutrino Laboratory. Detector is operated after calibration and optimization studies and from collected data, neutron flux is obtained using computational methods.

SNO+, the successor of the Sudbury Neutrino Observatory, is an upcoming low energy neutrino experiment, located in the 2 km deep laboratory SNOLAB, Canada. The spheric acrylic vessel in the detector center will contain 780 t of LAB. The main goal of SNO+ is the search for the neutrinoless double beta decay of 130Te, using a novel scintillator in which natural Te is bound with an initial loading of 0.3% via water and a surfactant. Within this thesis, the first measurement of the Alpha-particle and proton quenching parameters of loaded and unloaded LAB is described. These parameters are crucial for an efficient background suppression, necessary to reach a sensitivity above the current limit in 76Ge of T1/2(0v) > 2.1 x 10^(25) y (90% C.L.). For 0.3% Te-loading, the quenching parameter obtained is kB = (0.0070 +/- 0.0004) cm/MeV for Alpha-particles and kB = (0.0090 +/- 0.0003) cm/MeV for protons. Additionally, the spectral sensitivity of SNO+ to supernova electron anti-neutrinos and muon and tau (anti-)neutrinos is determined for the first time, using inverse beta decay and v-p elastic scattering with the measured quenching parameters. The obtained sensitivity to the mean energy of electron anti-neutrinos is E = 15.47^(+1.54)_(-2.43) MeV and of muon and tau (anti-)neutrinos is E = 17.81^(+3.49)_(-3.09) MeV. / SNO+, der Nachfolger des Sudbury Neutrino Observatorys, ist ein bevorstehendes Niederenergie-Neutrino-Experiment im 2 km tiefen Untergrundlabor SNOLAB in Kanada. Die Acryl-Kugel im Zentrum des Detektors wird mit 780 t LAB gefüllt werden. Das Hauptziel von SNO+ ist die Suche nach dem neutrinolosen Doppelbetazerfall von 130Te mit einem neuartigen Szintillator, in dem natürliches Te mit einer Anfangskonzentration von 0.3% über Wasser und ein Tensid gebunden wird. In dieser Arbeit wird erstmals die Messung der Alpha-Teilchen und Proton Quenching Parameter in diesem und in normalem LAB beschrieben. Die Parameter sind unverzichtbar für eine effiziente Untergrund Unterdrückung, die notwendig ist um auf das bestehende Limit in 76Ge von T1/2(0v) > 2.1 x 10^(25) y (90% C.L.) sensitiv zu sein. Der ermittelte Quenching Parameter bei 0.3% Te beträgt kB = (0.0070 +/- 0.0004) cm/MeV für Alpha-Teilchen und kB = (0.0090 +/- 0.0003) cm/MeV für Protonen. Zusätzlich wird erstmals die spektrale Sensitivität von SNO+ auf Supernova Elektron Anti-Neutrinos und Muon and Tau (Anti-)Neutrinos bestimmt über den inversen Betazerfall und die elastische v-p Streuung zusammen mit den gemessenen Quenching Parametern. Die ermittelte Sensitivität auf die mittlere Energie der Elektron Anti-Neutrinos ist E = 15.47^(+1.54)_(-2.43) MeV und der Muon und Tau (Anti-)Neutrinos ist E = 17.81^(+3.49)_(-3.09) MeV.

This report describes investigations of the NE213-detector and the possibility to utilize pulse shape analysis to separate neutrons and gammas in a mixed emission field. Neutron fluxes are often contaminated with gammas, to which the detectors are sensitive. Sorting out the unwanted gamma pulses from the interesting neutrons is therefore crucial in many situations, for instance in fusion reactor diagnostics, such as for neutron cameras. This can be done based on pulse shapes, which differ for gammas and neutrons interacting in the NE213-detector. By analyzing the pulse shapes from a digital transient recorder, neutrons can be distinguished from gammas. An experiment with a Cf-252 neutron source was set up and provided data. The separation algorithm was based on charge comparison and gave good results. Furthermore the results of the pulse shape analysis were verified by TOF-measurements. The lowest permissible energy for a reasonable separation was found to be around 0.5 MeV. Some conclusions on the limitations of the equipment were also made.

This thesis presents the design qualification and construction of the Beam Scintillator Counter (BSC) for the CMS Collaboration at CERN in 2007 - 2008. The BSC detector is designed to aid in the commissioning of the Compact Muon Solenoid (CMS) during the first 2 years of operation and provide technical triggering for beam halo and minimum-bias events. Using plastic scintillator tiles mounted at both ends of CMS, it will detect minimum ionizing particles through the low-to-mid luminosity phases of the Large Hadron Collider (LHC) commissioning. During these early phases, the BSC will provide probably the most interesting and widely used data of any of the CMS sub-detectors and will be employed in the track based alignment procedure of the central tracker and commissioning of the Forward Hadron Calorimeter.

Submitted by EDER QUEIROZ BARBOSA (ederqb_eaunesp@hotmail.com) on 2017-08-25T17:41:03Z No. of bitstreams: 1 DISSERTACAO MESTRADO BARBOSA, E. Q. FINAL CORRIGIDA.pdf: 9658662 bytes, checksum: 8ed25992d35956a209ef71c55c30f430 (MD5) / Approved for entry into archive by Monique Sasaki (sayumi_sasaki@hotmail.com) on 2017-08-25T17:57:43Z (GMT) No. of bitstreams: 1 barbosa_eq_me_rcla.pdf: 9658662 bytes, checksum: 8ed25992d35956a209ef71c55c30f430 (MD5) / Made available in DSpace on 2017-08-25T17:57:43Z (GMT). No. of bitstreams: 1 barbosa_eq_me_rcla.pdf: 9658662 bytes, checksum: 8ed25992d35956a209ef71c55c30f430 (MD5) Previous issue date: 2016-10-03 / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES) / O presente trabalho descreve etapas realizadas para a viabilização de novas metodologias de calibração de sistemas radiométricos portáteis utilizados no LABIDRO (Laboratório de Isótopos e Hidroquímica) do DPM (Departamento de Petrologia e Metalogenia) do IGCE (Instituto de Geociências e Ciências Exatas) da UNESP, Campus de Rio Claro. Dentre os tópicos abordados estão a determinação de tempos de detecção de maior precisão, curvas de calibração dosimétrica e a aquisição de dados de dosimetria no ar, para ambientes indoor e outdoor, por intermédio de gamaespectrômetros portáteis. Os modelos geoestatísticos gerados a partir da conversão de dados em dose efetiva para os locais analisados nos departamentos do Curso de Geologia da UNESP de Rio Claro (SP), demonstraram que apesar de existirem alguns valores situados acima daqueles recomendados pela ICRP e norma CNEN-NN-3.01 de 1 mSv.ano-1, não há a necessidade de intervenção nos locais onde ocorreram (Museu Heinz Ebert; Litoteca do DPM) pois, não são de uso frequente e, além disso, situam-se abaixo do limite recomendado de 20 mSv.ano-1 para indivíduos ocupacionalmente expostos. / The present work describes steps undertaken for the viability of new radiometric methodologies of the portable systems calibration used in the LABIDRO (Isotopes and Hydrochemistry Laboratory) of DPM (Petrology and Metalogeny Department) of IGCE (Geoscience and Exact Sciences Institute) at UNESP, Rio Claro Campus. Among the topics covered are the determination of detection times with greater accuracy, dosimetric calibration curves and dosimetry data acquisition in the air, for indoor and outdoor environments, through gamma spectrometer detectors. Geostatistical models generated from the conversion of data, to the sites analyzed in the departments of Geology Course at UNESP, in effective dose, have shown that although there are some values set above those recommended by ICRP and by legal norm CNEN-NN-3.01 of 1 mSv.year-1, there is no need to intervene in places where it occurred (Heinz Ebert Museum; Deposit of rocks and minerals - DPM), Since these sites are of short period of visit time and, in addition, are below the recommended limit of 20 mSv.year-1 for occupationally exposed individuals. / CAPES: 00.889.834/0001-08

O conhecimento preciso do espectro energético de fótons é de extrema importância na radioterapia no que se refere à escolha adequada das doses a que os pacientes são submetidos. Os dados de saída dos detectores de radiação são apenas espectros de altura de pulso (PHD), ao invés de espectros de energia, que correspondem a informações distorcidas sobre a fonte e seus decaimentos devido a diversos erros associados ao processo de cintilação do cristal e à eletrônica. Os resultados medidos foram obtidos com o uso de um detector cintilador de NaI(Tl) e as simulações Monte Carlo foram feitas com o uso do programa EGSnrc. A partir das características do detector obtidas experimentalmente, nossas simulações puderam ser validadas para se aproximarem o mais próximo possível do caso real em laboratório. Dessas medidas experimentais de fontes radioativas de calibração e simulações, foi montada uma matriz resposta inversa que transforma PHD em espectro de energia de fótons. Uma vez que a faixa energética das fontes radioativas medidas teve um limite de 1.6MeV, a matriz resposta também o apresenta, mas que pode ser contornado de acordo com a geometria usada para a obtenção do PHD a ser corrigido. Observa-se que a resposta do detector é diretamente proporcional à energia e assim, dependendo da energia incidente a ser estudada, dois tipos de matriz resposta inversa podem ser aplicadas. Os resultados desta transformação de PHD para espectro de energia de fótons são apresentados. / The accurate knowledge of the photon energy spectrum in radiotherapy is of extremely importance when it comes to the appropriate choice for doses whose patients are submitted. The output data from the radiation detectors is described as pulse high distributions, instead of energy spectra, that correspond to distorted information about the source and its decays due to many errors associated to the crystal scintillation process and the electronics. The measured results were obtained with a NaI(Tl) scintillation detector and Monte Carlo simulations were performed by the EGSnrc program. From the detector characteristics obtained experimentally, the simulations were validated so they could approximate the more real as possible as in laboratory. Using these simulated and experimental calibration sources, an inverse response matrix was built and transforms pulse high distributions in photons energy spectrum. Once the correction energy limit due to the radiation sources used is approximately 1.6 MeV, so the response matrix has a limit, but it can be overcame by the beam incident angle and the geometry used when the pulse high distributions to be corrected is going to be measured. One can realize that the detector response is directly proportional to the incident energy and, when it is intense as in a LINAC or weak as in a calibration source, different types of matrix can be applied. The results from these transformations are presented.

We present a preliminary design for a novel neutron detection system that is compact, lightweight, and low power consuming, utilizing the CubeSat platform making it suitable for space-based applications. This is made possible using the scintillating crystal lithium indium diselenide ((LiInSe2)-Li-6), the first crystal to include Li-6 in the crystalline structure, and a silicon avalanche photodiode (Si-APD). The schematics of this instrument are presented as well as the response of the instrument to initial testing under alpha, gamma and neutron radiation. A principal aim of this work is to demonstrate the feasibility of such a neutron detection system within a CubeSat platform. The entire end-to-end system presented here is 10 cm x 10 cm x 15 cm, weighs 670 grams and requires 5 V direct current at 3 Watts.

>Magister Scientiae - MSc / A (5 cm × 5 cm) cylindrical NE213 liquid organic scintillator and a (2.5 cm × 2.5 cm)cylindrical NE230 liquid organic scintillator were used as spectrometers. A series of measurements was made with both the NE213 and NE230 spectrometers, with the time-of- flight technique used for neutron energy selection. Pulse height spectra for quasi- monoenergetic neutron beams of ~5-64 MeV produced by bombarding either a (1 mm) lithium metal target, or a (10 mm) beryllium target, or a (10 mm) graphite target with 66 MeV proton beam were measured with both spectrometers. Deuteron events identified by pulse shape discrimination were selected for measurements with the NE230 spectrometer while proton events were selected for measurements with the NE213 spectrometer. Response of the scintillator to protons using NE213 and deuterons using NE230 were obtained from the measured pulse height spectra. Detector efficiency of the NE213 spectrometer as a function of neutron energy was determined for n-p elastic scattering. The detector efficiency of the NE230 was determined relative to the well-known efficiency of the NE213 spectrometer, selecting either all or n-d elastic events in the pulse height spectra measured with the NE230 spectrometer. The detection efficiency of the NE230 spectrometer was also determined from the available cross-section for n-d elastic scattering as exploratory work. Neutron fluence spectra could be determined using the appropriate neutron detection efficiency for each spectrometer and were compared with each other. The results showed good comparison and encouragement demonstrating the reliability of neutron fluence spectral measurements withthe NE230 spectrometer using the time-of-flight technique.

The GlueX experiment aims to study meson photoproduction while utilizing the coherent bremsstrahlung technique to produce a 9 GeV linearly polarized photon beam incident on a liquid $\mathrm{H_{2}}$ target. A Start Counter detector was fabricated to properly identify the accelerator electron beam buckets and to provide accurate timing information. The Start Counter detector was designed to operate at photon intensities of up to $\mathrm{10^{8}\gamma/s}$ in the coherent peak and provides a timing resolution $\mathrm{\sim 300\ ps}$ so as to provide successful identification of the electron beam buckets to within 99\% accuracy. Furthermore, the Start Counter detector provides excellent solid angle coverage, $\sim 90 \%\ \mathrm{of}\ 4 \pi\ \mathrm{hermeticity}$, and a high degree of segmentation for background rejection. It consists of a cylindrical array of 30 scintillators with pointed ends that bend towards the beam at the downstream end. Magnetic field insensitive silicon photomultiplier detectors were selected as the readout system. An initial measurement of the beam asymmetry $\Sigma$ in the exclusive reaction $\vec{\gamma}p \rightarrow \pi^{0}p$, where $\pi^{0} \rightarrow \gamma \gamma$ has been carried out utilizing the GlueX spectrometer during the Spring 2015 commissioning run. The tagged photon energies ranged from $2.5 \leq E_{\gamma} \leq 3.0\ \mathrm{GeV}$ in the coherent peak. These measurements were then compared to the world data set and show remarkable agreement with only two hours of physics production running.