Thesis (MSc)--Stellenbosch University, 2012. / ENGLISH ABSTRACT: Nine 100x100x600 mm3 plastic scintillators, formerly built for the neutron time of ight measurements at iThemba LABS, were refurbished. The position resolution of these detectors was determined using muon cosmic rays and coincident measurement techniques. Average position resolution of 4.28 cm (FWHM) was found. In order to predict the time spectrum of the large-volume detector Monte Carlo simulations have been performed. These simulations aimed at anticipating the separation of statistical neutrons, prompt gamma rays and uncorrelated gamma rays from the fast neutrons emitted in the reaction of interest. One of the neutron detectors was tested using fast neutrons from the 232Th( ,xn) reaction at 42 MeV. Statistical neutrons from fusion evaporation reactions were produced in 152Sm(12C,xn) fusion evaporation reaction. Coincidences between neutrons and gamma rays were successfully identi ed. Prompt gamma rays and uncorrelated gamma rays were also identi ed. / AFRIKAANSE OPSOMMING: Nege 100x100x600 mm3 plastiese scintillators, wat aanvanklik gebou was vir neutron vlugtyds meetings by iThemba LABS, was hernu. Die posisie resolusie van die detektore was bepaal deurmiddel van muon kosmiese straling en koïnsidensie meet tegnieke. Posisie resolusie van 4.28 cm (FWHM) was verkry. Monte Carlo simulasies is gebruik om die posisie resolusie van'n groot volume detektor te voorspel. Hierdie simulasies is daarop gemik om onderskeid te maak tussen statistiese neutrone, gelyktydige gamma strale en ongekorreleerde gamma strale vanaf vinnige neutrone in die reaksie van belang uitgestraal word. Een neutron detektor was getoets deur gebruik te maak van vinnige neutrone wat uit die reaksie 232Th( ,xn) by 42 MeV ontstaan. Statistiese neutrone vanaf splitsings verdampingsreaksies, gelyktydige gamma strale en ongekorreleerde gamma strale was geidenti seer. Statistiese neutrone van samesmelting verdamping reaksies was geproduseer in die reaksie 152Sm(12C,xn). Toeval tussen neutrone en gamma strale was suksesvol geïdenti seer, gevra gamma strale en ongekorreleerd gamma strale was ook geïdenti seer.

Two measurements have been made, addressing gaps in knowledge for 235U(n,f) and 238U(n,f). The energy distribution for prompt fission neutrons is not well-understood below 1 MeV in 235U(n,f). To measure the 235U(n,f) prompt fission neutron distribution, a pulsed neutron beam at the WNR facility in Los Alamos National Laboratory was directed onto a 235U target with neutron detectors placed 1 m from the target. These neutron detectors were designed specifically for this experiment and employed a unique geometry of scintillating plastic material that was designed to reject backgrounds. Fission fragments were detected using an avalanche counter. Coincidences between fission fragment production and neutron detector events were analyzed, using a double time-of-flight technique to determine the energy of the prompt fission neutrons. A separate measurement was made, investigating the neutron-induced fission cross section for 238U(n,f). This measurement also used the pulsed neutron beam at the WNR facility. The neutron flux was normalized to the well-known hydrogen standard and the fission rate was observed for beam neutrons in the energy range of 130-300 MeV. Using an extrapolation technique, the energy dependence of the cross section was determined. These new data filled a sparsely populated energy region that was not well-studied and were measured relative to the hydrogen standard, unlike the majority of available data. These data can be used to constrain the fission cross section, which is considered a nuclear reaction standard.

Les détecteurs de radiations nucléaires sont des outils importants dans de nombreux domaines tels que dans les réacteurs nucléaires, la sécurité nationale, mais ils sont également primordiaux dans des applications médicales. Les progrès récents dans la technologie des semi-conducteurs permettent la réalisation de détecteurs très efficaces et quasi-insonores qui permettent la détection de différents types de radiations nucléaires. Le carbure de silicium (SiC) est une bande semi-conductrice large, grâce à sa conductivité thermique élevée et à une résistance élevée aux rayonnements, il est adapté pour les environnements difficiles où peuvent exister des flux élevés de température et de rayonnement. Le but du projet européen (I_SMART) est ainsi de prouver la fiabilité de nouvelles méthodes de réalisation de détecteurs de radiations nucléaires et d'étudier leur performance dans différents types d'irradiation (neutrons rapides et thermiques) et à différentes températures. Différentes méthodes ont été utilisées pour réaliser les détecteurs de rayonnement SiC. Par exemple l'implantation d'ions de bore a été utilisé pour créer la couche de conversion de neutrons soit dans le contact métallique ou directement en SiC. Les détecteurs fabriqués ont été testés dans le réacteur nucléaire BR1, mettant en lumière la présence de neutrons thermiques. En outre, ces détecteurs détectent des neutrons rapides sous n’importe quelle température. En outre, les détecteurs utilisés montrent leur stabilité sous différents flux de neutrons qui indiquent la fiabilité de ces nouveaux modes de réalisation de détecteurs de rayonnement qui pourraient remplacer ceux utilisés actuellement. / Nuclear radiation detectors are important tools in many fields such as in nuclear reactors, homeland security and medical applications. Recent advances in semiconductor technology allow construction of highly efficient low noise detectors for different nuclear radiations. Silicon carbide (SiC) is a wide band gap semiconductor with a high thermal conductivity and high radiation resistance. It is suitable for a harsh environment where high temperatures and radiation fluxes may exist. In the framework of the European project (I_SMART) the purpose of this work is to demonstrate the reliability of new methods of realizing nuclear radiation detectors and to study their performance under different types of irradiation (fast and thermal neutrons) and at elevated temperatures. Different methods have been used to realize SiC based-radiation detectors. For instance boron ion implantation has been used to create the neutron converter layer either in the metallic contact or directly in the SiC. The fabricated detectors have been tested in the BR1 nuclear reactor revealing the thermal neutron detection and the feasibility of gamma discrimination from thermal neutrons using one single detector. Such detectors are sensitive to fast neutrons with a stable response under elevated temperatures (up to 150 °C). Furthermore, the studied detectors show stability under different neutron fluxes, indicating a reliability of such new methods of realizing radiation detectors which could replace those of the current state of the art.

Interactions between an intense laser pulse and cluster targets are investigated using the recent experimental results of the cluster fusion experiments on the Texas Petawatt Laser (TPW). We achieved about 2x10⁷ DD fusion neutrons per shot on the TPW by optimizing the laser and gas jet parameters. A few different types of cluster targets were used on the TPW including deuterium clusters, deuterated methane clusters, deuterium cluster + helium-3 mixture, and deuterated methane cluster + helium-3 mixture. We designed our own neutron detectors and proton detectors for the measurements of the fusion yields. The calibration method of neutron detectors is described in detail. Through the yield measurements of the 2.45 MeV neutrons from the DD fusion reactions and 14.7 MeV protons from the D-³He fusion reactions in the deuterium-helium-3 mixture target, we successfully measured the ion temperature of the fusion plasma at the time of the fusion reactions. / text

Made available in DSpace on 2014-10-09T12:43:27Z (GMT). No. of bitstreams: 0 / Made available in DSpace on 2014-10-09T13:56:10Z (GMT). No. of bitstreams: 1 06629.pdf: 11734475 bytes, checksum: 26ac38190c26794def0e5ba95d87d535 (MD5) / Tese (Doutoramento) / IPEN/T / Instituto de Pesquisas Energeticas e Nucleares - IPEN/CNEN-SP

Made available in DSpace on 2014-10-09T12:42:41Z (GMT). No. of bitstreams: 0 / Made available in DSpace on 2014-10-09T13:57:18Z (GMT). No. of bitstreams: 1 05028.pdf: 9521463 bytes, checksum: 8a386f78270b1c225d259433bbd3167d (MD5) / Dissertacao (Mestrado) / IPEN/D / Instituto de Pesquisas Energeticas e Nucleares - IPEN/CNEN-SP

Made available in DSpace on 2014-10-09T12:43:27Z (GMT). No. of bitstreams: 0 / Made available in DSpace on 2014-10-09T13:56:10Z (GMT). No. of bitstreams: 1 06629.pdf: 11734475 bytes, checksum: 26ac38190c26794def0e5ba95d87d535 (MD5) / Tese (Doutoramento) / IPEN/T / Instituto de Pesquisas Energeticas e Nucleares - IPEN/CNEN-SP

Made available in DSpace on 2014-10-09T12:42:41Z (GMT). No. of bitstreams: 0 / Made available in DSpace on 2014-10-09T13:57:18Z (GMT). No. of bitstreams: 1 05028.pdf: 9521463 bytes, checksum: 8a386f78270b1c225d259433bbd3167d (MD5) / Dissertacao (Mestrado) / IPEN/D / Instituto de Pesquisas Energeticas e Nucleares - IPEN/CNEN-SP

Nowadays we are all witnesses of a competition of facilities at different countries to study unknown regions of neutron rich nuclei. Much efforts are devoted to understand the role of neutron excess and its influence on nuclei in vicinity of closed neutron shells. One of the means to investigate nuclear structure is in beta-decay. Once a nucleus is proven to exist, its beta-decay properties, such as T1/2 and Pn (probability of beta-delayed neutron emission), which are relatively easy to measure, can provide the first hints on the nuclear structure. On the r-process site, "waiting points"(nuclei on closed neutron shells) has significant effects on the r-process dynamics and the abundance distribution. The actual side and the astrophysical conditions under which the nuclear synthesis takes place are still not certainly known - since r-process nuclei are difficult to produce and to study experimentally, input parameters for r-process calculations are mostly derived from theoretical models. As it has been seen lately, most of the theories have failed to reproduce newly measured data sets near shell closures. With new experimental data already (or shortly) available theoretical approaches can be adjusted. Since a beta-delayed neutron emission becomes strong if not dominating decaying channel for nuclei far stability, a proper neutron detector to study their properties is indispensable. To conduct the appropriate investigations, in the frame of the present thesis, in close collaboration with JINR (Dubna) a new detection system was constructed. It consists of 80 ³He-filled counters, 4π beta detector and a HPGe in order to measure simultaneously beta, gamma, neutron activity. The development of such a detection system system, currently installed at ALTO ISOL facility, was the first objective of the thesis. Then, during two experimental campaigns conducted to investigate beta decay properties of neutron rich nuclei in the neighborhood of N=50, N=82 the workability of the newly produced detection system was proven. In the vicinity of ⁷⁸Ni: half- lives and probability of beta-delayed neutron emission for ⁸º,⁸²,⁸³,⁸⁴Ga were measured. We were the first to observe the structure of ⁸¹,⁸² Ge via beta neutron gated gamma spectra. Thanks to the neutron detection channel the absolute intensities of beta decay were proposed for the first time. In the vicinity of ¹³²Sn the half lives of ¹²³Ag, ¹²⁴Ag, ¹²⁵Ag and ¹²⁷In, ¹²⁸In was measured. For the first time the beta delayed neutron emission was observed for ¹²⁶Cd, its Pn value also measured. Based on the data obtained we come to the conclusion that to figure out the relative contribution of allowed and forbidden decays more theoretical efforts should be done crossing the N=50 shell. Whereas in the vicinity of N=82 shell more experimental challenge are required.

Aujourd'hui, nous sommes tous témoins d'une compétition des installations en pays différents pour étudier les régions inconnues de noyaux riches en neutrons. Beaucoup d'efforts sont consacrés à comprendre le rôle de l'excès de neutrons et son influence sur les noyaux dans les environs de coquilles de neutrons fermées. Un des moyens pour étudier la structure nucléaire est via la désintégration bêta. Une fois un noyau est prouvé d'exister, ses propriétés de désintégration bêta, comme T1/2 et Pn (probabilité de l'émission de neutrons de bêta-retardés), qui sont relativement faciles à mesurer, peuvent fournir les premiers indices sur la structure nucléaire. Sur le site de processus-r des «points d'attente» (noyaux sur des coquilles de neutrons fermés) ont des effets importants sur la dynamique processus-r ainsi que sur la distribution de l'abondance des éléments. Les conditions astrophysiques exactes en vertu de desquelles la synthèse nucléaire a lieu ne sont pas connus avec certitude. Parce que les noyaux participant en processus-r sont difficiles à synthétiser même aujourd'hui et à étudier expérimentalement, les paramètres nécessaires pour les calculs du processus-r sont principalement dérivés de modèles théoriques. Comme on l'a vu récemment, la plupart des théories n'ont pas réussi à reproduire des ensembles de données nouvellement mesurées près de fermetures de couche. Avec de nouvelles données expérimentales déjà (ou bientôt) disponibles les approches théoriques peuvent être ajustées. Comme émission de neutrons retardée bêta devient plus importante voie le canal dominant en désintégration des noyaux loin d'un stabilité, l'utilisation d'un détecteur de neutrons approprié afin d'étudier leurs propriétés est indispensable. C'est pour mener la recherche appropriée que dans le cadre de la thèse, en étroite collaboration avec le JINR (Dubna) un nouveau système de détection a été construit. Il se compose de 80 compteurs de ³He, un détecteur 4π de bêta et un HPGe afin de mesurer simultanément l'activité de gamma, bêta et neutrons. Le développement d'un tel système de détection, actuellement installé sur ALTO, a été le premier objectif de la thèse. Puis, au cours de deux campagnes expérimentales menées pour examiner les propriétés de désintégration bêta de noyaux riches en neutrons dans le proximité de N = 50, N = 82 la capacité de travail du système de détection produit a été prouvée. Dans le région de ⁷⁸Ni : le temps de vie et de la probabilité de l'émission de neutrons bêta retardés pour ⁸º,⁸²,⁸³,⁸⁴Ga ont été mesurés. Nous sommes les premiers à observer la structure de ⁸¹,⁸² Ge via spectroscopie gamma spectre conditionnée par bêta et par neutron. Grâce à la détection des neutrons les intensités absolues de la désintégration bêta ont été proposées pour la première fois. Dans le région de ¹³²Sn les temps de vie de ¹²³Ag, ¹²⁴Ag, ¹²⁵Ag et ¹²⁷In, ¹²⁸In ont été mesurées. Pour la première fois l'émission de neutrons retardés bêta a été observée pour le cas de ¹²⁶Cd, sa valeur Pn également mesurée. Sur la base des données obtenues, nous arrivons à la conclusion que, pour déterminer la contribution relative de désintégrations permises et interdites les efforts théoriques doivent être faites en traversant la couche N = 50. Alors que dans le région de N = 82 plus de données expérimentales sont nécessaires. / Nowadays we are all witnesses of a competition of facilities at different countries to study unknown regions of neutron rich nuclei. Much efforts are devoted to understand the role of neutron excess and its influence on nuclei in vicinity of closed neutron shells. One of the means to investigate nuclear structure is in beta-decay. Once a nucleus is proven to exist, its beta-decay properties, such as T1/2 and Pn (probability of beta-delayed neutron emission), which are relatively easy to measure, can provide the first hints on the nuclear structure. On the r-process site, "waiting points"(nuclei on closed neutron shells) has significant effects on the r-process dynamics and the abundance distribution. The actual side and the astrophysical conditions under which the nuclear synthesis takes place are still not certainly known - since r-process nuclei are difficult to produce and to study experimentally, input parameters for r-process calculations are mostly derived from theoretical models. As it has been seen lately, most of the theories have failed to reproduce newly measured data sets near shell closures. With new experimental data already (or shortly) available theoretical approaches can be adjusted. Since a beta-delayed neutron emission becomes strong if not dominating decaying channel for nuclei far stability, a proper neutron detector to study their properties is indispensable. To conduct the appropriate investigations, in the frame of the present thesis, in close collaboration with JINR (Dubna) a new detection system was constructed. It consists of 80 ³He-filled counters, 4π beta detector and a HPGe in order to measure simultaneously beta, gamma, neutron activity. The development of such a detection system system, currently installed at ALTO ISOL facility, was the first objective of the thesis. Then, during two experimental campaigns conducted to investigate beta decay properties of neutron rich nuclei in the neighborhood of N=50, N=82 the workability of the newly produced detection system was proven. In the vicinity of ⁷⁸Ni: half- lives and probability of beta-delayed neutron emission for ⁸º,⁸²,⁸³,⁸⁴Ga were measured. We were the first to observe the structure of ⁸¹,⁸² Ge via beta neutron gated gamma spectra. Thanks to the neutron detection channel the absolute intensities of beta decay were proposed for the first time. In the vicinity of ¹³²Sn the half lives of ¹²³Ag, ¹²⁴Ag, ¹²⁵Ag and ¹²⁷In, ¹²⁸In was measured. For the first time the beta delayed neutron emission was observed for ¹²⁶Cd, its Pn value also measured. Based on the data obtained we come to the conclusion that to figure out the relative contribution of allowed and forbidden decays more theoretical efforts should be done crossing the N=50 shell. Whereas in the vicinity of N=82 shell more experimental challenge are required.