<p>Two separate experimental searches for second-order weak nuclear decays to excited final states were conducted. Both experiments were carried out at the Kimballton Underground Research Facility to provide shielding from cosmic rays. The first search is for the two-neutrino double-beta decay of 96Zr to excited final states of the daughter nucleus, 96Mo. As a by product of this experiment, the beta decay of 96Zr was also investigated. Two coaxial high-purity germanium detectors were used in coincidence to detect gamma rays produced by the daughter nucleus as it de-excited to the ground state. After collecting 1.92 years of data with 17.91 g of enriched 96Zr, half-life limits at the level of 10^20 yr were produced. Measurements of this decay are important to test neutrinoless double-beta decay nuclear matrix element calculations, which are necessary to extract the neutrino mass from a measurement of the neutrinoless double-beta decay half-life. </p><p>The second experiment is a search for the resonantly-enhanced neutrinoless double-electron capture decay of 156Dy to excited states in 156Gd. Double-electron capture is a possible experimental alternative to neutrinoless-double beta decay, which could distinguish the Dirac or Majorana nature of the neutrino. Two clover high-purity germanium detectors were used in coincidence to investigate the decay. A 213.5 mg enriched 156Dy sample was observed for 0.635 year, producing half-life limits of 10^17 yr. The limits produced by both of these experiments are currently the most stringent limits available for these decays.</p> / Dissertation

CP violation is an important condition to explain the preponderance of baryons in our universe, yet the available CP violation in the Standard Model (SM) via the so-called Cabibbo-Kobayashi-Maskawa mechanism seems to not provide enough CP violation. Thus searching for new sources of CP violation is one of the central tasks of modern physics. In this thesis, we focus on a new possible source of CP violation which generates triple-product correlations in momenta which can appear in neutron and nuclear radiative β decay. We show that at low energies such a CP violating correlation may arise from the exotic coupling of nucleon, photon and neutrino that was proposed by Harvey, Hill, and Hill (HHH). One specialty of such an exotic HHH coupling is that it does not generate the well-known CP-violating terms such as ``D-term'', ``R-term'', and neutron electric dipole moment, in which particle's spins play critical role. We show that such a new HHH-induced CP violating effect is proportional to the imaginary part of c5gv, where gv is the vector coupling constant in neutron and nuclear β decay, and c5 is the phenomenological coupling constant that appears in chiral perturbation theory at O(M-2) with M referring to the nucleon or nuclear mass. We consider a possible non-Abelian hidden sector model, which is beyond the SM and may yield a nontrivial Im(c5). The available bounds on both Im(c5) and Im(gv) are considered, and a better limit on Im(c5) can come from a direct measurement in radiative beta decay. We calculate the competitive effect that arises from the general parameterization of the weak interaction that was proposed by Lee and Yang in 1956. We also show that in the proposed measurements, the CP-violating effect can be mimicked by the SM via final-state interactions (FSI). For a better determination of the bound of Im(c5), we consider the FSI-induced mimicking effect in full detail in O(α) as well as in leading recoil order. To face ongoing precision measurements of neutron radiative β decay of up to 1% relative error, we sharpen our calculations of the CP conserving pieces of neutron radiative β decay by considering the largest contributions in O(α2): the final-state Coulomb corrections as well as the contributions from two-photon radiation.

While neutrino oscillations indicate that neutrino flavors mix and that neutrinos have mass, they do not supply information on the absolute mass scale of the three flavors of neutrinos. Currently, the only viable way to determine this mass scale is through the observation of the theoretically predicted process of neutrinoless double-beta decay (0νββ). This yet-to-be-observed decay process is speculated to occur in a handful of nuclei and has predicted half-lives greater than 10²⁵ years. Observation of 0νββ is the goal of several large-scale, multinational efforts and consists of detecting a sharp peak in the summed β energies at the Q-value of the reaction. An exceptional candidate for the observation of 0νββ is ⁷⁶Ge, which offers an excellent combination of capabilities and sensitivities, and two such collaborations, MAJORANA and GERDA, propose tonne-scale experiments that have already begun initial phases using a fraction of the material. The absolute scale of the neutrino masses hinges on a matrix element, which depends on the ground-state wave functions for both the parent (⁷⁶Ge) and daughter (⁷⁶Se) nuclei in the 0νββ decay and can only be calculated from nuclear structure models. Efforts to provide information on the applicability of these models have been undertaken at the University of Kentucky Accelerator Laboratory using gamma-ray spectroscopy following inelastic scattering reactions with monoenergetic, accelerator-produced fast neutrons. Information on new energy levels and transitions, spin and parity assignments, lifetimes, multipole mixing ratios, and transition probabilities have been determined for ⁷⁶Se, the daughter of ⁷⁶Ge 0νββ, up to 3.0 MeV. Additionally, inaccuracies in the accepted level schemes have been addressed. Observation of 0νββ requires precise knowledge of potential contributors to background within the region of interest, i.e., approximately 2039 keV for ⁷⁶Ge. In addition to backgrounds resulting from surrounding materials in the experimental setup, ⁷⁶Ge has a previously observed 3952-keV level with a de-exciting 2040-keV γ ray. This γ ray constitutes a potential background for 0νββ searches, if this level is excited. The cross sections for this level and, subsequently, for the 2040-keV γ ray has been determined in the range from 4 to 5 MeV.

This dissertation reports on new information in the [beta minus] decay of the neutron-rich nucleus 81Zn, which populates states in its daughter nucleus 81Ga. This includes new [gamma]-ray transitions in the daughter nucleus, 81Ga, as well as a [beta]-delayed neutron branching ratio. This isotope was produced at the Holifield Radioactive Ion Beam Facility of Oak Ridge National Laboratory through the Isotope Separation Online technique. They are fission fragments from proton-induced fission on a uranium carbide target. These fission fragments are ionized and both mass and isotopically separated before arriving at the Low Energy Radioactive Ion Beam Spectroscopy Station (LeRIBSS). The [gamma]-ray and [beta] electron emissions from the decays are measured and analyzed in this work. A new [beta]-delayed neutron branching ratio is reported for this decay, which is in agreement with recent theoretical values. The core excited states in the daughter nucleus, 81Ga, populated through allowed Gamow-Teller decays are analyzed. A trend in core excited states with other N=50 isotones indicates an increasing gap between a deeply bound neutron hole and the valence neutron above the N=50 gap upon moving towards doubly magic 78Ni. This dissertation also reports on additions to the decay schemes of 79Zn and 80Zn decays. Their decay level schemes have been expanded upon and an improved picture of the total allowed Gamow-Teller decay strength is known from 79Zn to 81Zn. This work presents an improved, albeit still incomplete, picture of the energy of states populated through Gamow-Teller decays from below to above the N=50 shell gap in zinc isotopes.

Thesis (Ph. D.)--University of Washington, 2004. / Vita. Includes bibliographical references (p. 126-132).

Le démonstrateur de SuperNEMO est un détecteur de nouvelle génération pour la recherche de la décroissance double bêta sans émission de neutrinos. Comme son prédécesseur NEMO3, la technique expérimentale utilisée associe un trajectographe et un calorimètre afin de pouvoir identifier les électrons des décroissances double bêta tout en permettant la différenciation des différentes composantes du bruit de fond. Le démonstrateur est en cours d’installation au Laboratoire Souterrain de Modane et commencera à prendre des données à la fin de l’année 2017 afin d’atteindre une sensibilité supérieure à 1026 ans sur la demi-vie de la décroissance ββ0ν du 82Se dans la version finale du détecteur (100 kg d’isotopes pour une exposition totale de 5 ans).Ce travail de thèse a consisté à étudier la réponse en énergie et en temps des modules optiques du calorimètre (association d'un scintillateur plastique et d'un photomultiplicateur). Une simulation optique basée sur le logiciel GEANT4 a été développée afin de reproduire l'ensemble des phénomènes optiques ayant lieu au sein du scintillateur et du photomultiplicateur : scintillation, atténuation de Birks, émission Cerenkov, propagation et collection des photons. Ces travaux ont abouti à la mise au point de termes correctifs de hautes précisions sur l’énergie afin que le Monte Carlo de SuperNEMO soit au plus proche des données. Ces corrections ont alors été appliquées dans le cas du démonstrateur afin d’étudier l'impact sur la sensibilité au processus ββ0ν du 82Se. Ces simulations optiques ont également été étendues jusqu’à la modélisation de la forme temporelle des signaux du calorimètre. / The SuperNEMO demonstrator is a next generation experimental device, looking for neutrinoless double beta decay. Like its predecessor NEMO3, the experimental technique employed is based on a combination of a tracker and a calorimeter to identify the electrons from the double beta decay process while allowing the differentiation and identification of the different background components. The SuperNEMO’s demonstrator is currently being installed at the Modane Underground Laboratory and will begin to register data by the end of 2017. The aim is to reach a sensivity greater than 1026 years on the half-life of the 82Se ββ0ν process in the final version of the detector (100 kg of isotopes for a 5 years’ total exposure).This thesis contribution to the SuperNEMO, consisted in studying the energy and time response of the calorimeter optical modules (association of a plastic scintillator and a photomultiplier). To do so, an optical simulation based on the GEANT4 software was developed, which enabled to reproduce and simulate all the optical phenomena inside a scintillator and a photomultiplier: scintillation, Birks attenuation, Cerenkov emission, propagation and photon collection. The outcome and result of this thesis has been to develop high-precision corrective factors on the energy linked, so that the Monte-Carlo’s SuperNEMO is closest to the real data experimental records. These corrections were applied to the demonstrator simulation in order to study the impact on the ββ0ν sensitivity. These optical simulations have also been extended to the modeling of the temporal shape of the calorimeter signals.

>Magister Scientiae - MSc / The study of ²²Na beta decay offers an opportunity to test the Standard Model of Particle Physics via measurements of the β−γ angular correlation. A previous measurement of this correlation yielded a non-zero value, indicating the need for a higher-order matrix element to the decay, beyond the allowed V − A approximation. On assuming the Conserved Vector Current (CVC) hypothesis for weak interactions and using the magnetic dipole M1 width of the analog 2+ state in ²²Na, one obtains an unexpectedly large 'second-class' form factor for 22Na β decay that is in disagreement with the Standard Model prediction. This thesis describes an analysis of data obtained from a previous ²¹Ne(p, γ) experiment to obtain the M1 width of the 2+ state of interest in ²²Na. This work aims to use the M1 width and the independently measured of the β − γ angular correlation to obtain a higher-order Standard-Model-allowed weak magnetism form factor for the decay, in an attempt to explain the observed anomaly mentioned above. / National Research Foundation (NRF)

L'observation de la désintégration double bêta sans émission de neutrino (0ν2β) fournirait des informations essentielles sur la nature du neutrino et son échelle de masse absolue. Ce processus consiste en la transformation simultanée de deux protons en deux neutrons avec l'émission de deux électrons et aucun neutrino. Cette transition n'est possible que si les neutrinos sont égaux aux antineutrinos (nature Majorana du neutrino). Les recherches pour une désintégration à ce point rare représentent un défi technique complexe, car les expériences de prochaine génération visent des sensibilités de l'ordre de 10^27-10^28 ans afin d'avoir un potentiel de découverte élevé. Cette thèse est focalisée sur les projets LUMINEU et CUPID-Mo, développant la technique des bolomètres scintillants pour la recherche de désintégration 0ν2β avec le radio-isotope 100Mo.Les bolomètres sont des détecteurs cryogéniques mesurant l'énergie des particules déposées via un changement de température dans l'absorbeur. Si des cristaux scintillants sont utilisés comme absorbeurs, les signaux lumineux peuvent être enregistrés avec un bolomètre auxiliaire, sensible à l'énergie totale déposée par les photons de scintillation. Une telle configuration permet de séparer les particules α des γ/β, en rejetant le fond le plus difficile. La technologie des bolomètres scintillants est décrite en détail comme une option pour une future expérience cryogénique à l'échelle d'une tonne, appelée CUPID, qui peut couvrir complètement la région de masses de neutrinos dans la hiérarchie inversée. / Neutrinoless double beta (0ν2β) decay is a process of great interest for neutrino physics: its observation would provide essential information on neutrino nature and its absolute mass scale. This process consists of the simultaneous transformation of two protons into two neutrons with the emission of two electrons and no neutrino, implying the violation of the total lepton number. Such transition is possible only if neutrinos are equal to antineutrinos (Majorana particles). The searches for such a rare decay are becoming a complicated technical challenge, as next generation of 0ν2β experiments aim at sensitivities of the order of half-life at 10^27-10^28 yr. This thesis is focused on LUMINEU and CUPID-Mo projects, developing the scintillating bolometers technique for 0ν2β decay search with 100Mo with Li2MoO4 crystals. Bolometers are cryogenic detectors measuring the deposited particle energy as a change of temperature in the absorber. The use of scintillating crystals allows to perform discrimination of α particles from γ/β ones due to different light output of these two particle types, rejecting the most challenging background. The scintillating bolometers technology is described in details as an option for a future ton-scale cryogenic experiment, named CUPID, which can completely cover the inverted hierarchy region of neutrino masses.

Les neutrinos sont les particules fondamentales de matière les plus abondantes dans l’univers. Ils ont été détectés pour la première fois en 1956. Depuis lors, plusieurs expériences ont tenté de percer leurs mystères. Ils n’interagissent que par interaction faible, ils sont donc difficiles à détecter. On sait aujourd’hui qu’ils ont une masse très faible, et qu’ils peuvent osciller entre trois saveurs leptoniques. Cependant, de nombreuses questions perdurent sur leur masse, leur nature ou encore l’existence de neutrinos stériles. Cette thèse appréhende ces deux dernières questions à l’aide de deux expériences différentes : SuperNEMO et SoLid. Le but de l’expérience SuperNEMO est de rechercher la nature du neutrino, c’est-à-dire s’il est sa propre anti-particule (particule de Majorana) ou non (particule de Dirac). Pour cela, on cherche à détecter des doubles désintégrations bêta sans émission de neutrinos car ce processus n’est possible que si les neutrinos sont des particules de Majorana. Des feuilles sources de l’émetteur double bêta ⁸²Se seront installées au centre du démonstrateur SuperNEMO qui est actuellement en construction au Laboratoire Souterrain de Modane. Ce détecteur est composé d’une chambre à fils pour détecter les traces des deux électrons émis lors des désintégrations et d’un calorimètre pour mesurer leurs énergies. La mesure de la double désintégration bêta sans émission de neutrinos est très compliquée car si ce processus existe, il est extrêmement rare. Par conséquent, un travail important est fait pour réduire le bruit de fond des rayons cosmiques ou de la radioactivité naturelle. Dans cette thèse, des simulations des différents bruits de fonds ont été faites pour comprendre leur impact sur la mesure de l’énergie des électrons issus de la double désintégration bêta du ⁸²Se. Il est montré que la radioactivité du verre des photomultiplicateurs ne sera pas négligeable mais qu’elle pourra être mesurée précisément dans certains canaux d'analyse. Des feuilles de cuivre ont aussi été simulées à la place des sources de ⁸²Se pour montrer qu’elles peuvent aider à contrôler le bruit de fond efficacement. Suite à ces travaux, il a été décidé d’installer des feuilles de cuivre parmi les sources de ⁸²Se. La deuxième expérience sur laquelle porte cette thèse est l’expérience SoLid qui cherche à prouver l’existence de neutrinos stériles. Plusieurs anomalies expérimentales pourraient être expliquées par des oscillations d'antineutrinos de réacteurs vers des neutrinos stériles. Le détecteur SoLid cherche à mettre en évidence un signal d'oscillation auprès du réacteur BR2 en Belgique en mesurant le flux d’antineutrinos en fonction de leur énergie et de la distance parcourue, grâce à une grande segmentation. La détection des antineutrinos de réacteur se fait par désintégration bêta inverse. L’interaction d’un antineutrino se traduit donc par l’émission en coïncidence d’un positron et d’un neutron. Les positrons sont détectés dans des cubes de plastique scintillant en PVT et les neutrons sont détectés par des feuilles de ⁶LiF:ZnS posées sur chacun des cubes. Un premier prototype, SM1, a montré l’intérêt de cette technologie notamment pour discriminer les bruits de fonds. Une partie des travaux de cette thèse a consisté à développer et exploiter un banc de test afin d'optimiser la collection de lumière du détecteur pour améliorer la résolution en énergie de SoLid. En testant différents matériaux et différentes configurations du détecteur, les mesures sur le banc de test ont montré qu’une résolution en énergie de 14 % pouvait être atteinte pour le détecteur SoLid (contre 20 % pour le prototype SM1). Les améliorations proposées ont été prises en compte dans la construction du détecteur SoLid qui s’est achevée en 2017. Une analyse des premières données du détecteur est également présentée pour montrer la sensibilité de SoLid à la détection des antineutrinos de réacteur. / Neutrinos are the most abundant fundamental particles of matter in the Universe. They were detected for the first time in 1956. Since then, several experiments have tried to unveil their mysteries. They only interact weakly so they are difficult to detect. It is known that their masses are very low and that they can oscillate between three leptonic flavours. However, several questions remain about their masses, their nature or the existence of sterile neutrinos. This thesis addresses the last two questions with two different experiments: SuperNEMO and SoLid. The goal of the SuperNEMO experiment is to understand the nature of neutrinos, whether it is its own antiparticle (Majorana particle) or not (Dirac particle). This is investigated by searching for neutrinoless double beta decay as this process is possible only if neutrinos are Majorana particles. Source foils of the double beta emitter ⁸²Se are installed at the center of the SuperNEMO demonstrator which is being assembled at the Modane Underground Laboratory. This detector is composed of a wire chamber to detect the tracks of the two electrons emitted in the decays and a calorimeter to measure their energies. Neutrinoless double beta decay measurement is very difficult because if this process exists, it is extremely rare. An important work has thus to be done to decrease backgrounds from cosmic rays or natural radioactivity. In this thesis, different backgrounds have been simulated to understand their impact on the measurement of the energy of the two electrons from ⁸²Se double beta decay. It is shown that radioactivity from photomultipliers glasses will not be negligible but it will be possible to measure it precisely in dedicated channels. Copper foils have also been simulated in the source strips to demonstrate that they can help to control efficiently the backgrounds. Following this work, it has been decided to install copper foils in addition to ⁸²Se foils. The second experiment investigated in this thesis is the SoLid experiment which is looking for the existence of sterile neutrinos. Several experimental anomalies could be explained by oscillations of reactor antineutrinos toward sterile neutrinos. The SoLid detector is looking for an oscillation signal at the Belgian BR2 reactor by measuring the antineutrino flux as a function of their energy and their traveling distance thanks to a fine segmentation. The reactor antineutrinos are detected via inverse beta decay. The antineutrino interaction signal is thus the emission in coincidence of a positron and a neutron. Positrons are detected by plastic scintillator cubes in PVT and neutrons are detected by ⁶LiF:ZnS sheets placed on 2 faces of each cube. A first prototype, SM1, has demonstrated the advantages of this technology, particularly to discriminate backgrounds. A part of the work of this thesis consisted in developing and exploiting a test bench to optimize the light collection of the detector in order to improve the energy resolution of the SoLid detector. By testing different materials and configurations, the test bench measurement demonstrated that an energy resolution of 14 % can be achieved for SoLid phase I, while it was 20 % for the SM1 prototype. The improvements proposed have been taken into account for the SoLid detector construction that was achieved in 2017. An analysis of the first detector data is also presented to show SoLid sensitivity to reactor antineutrino detection.

京都大学 / 0048 / 新制・課程博士 / 博士(理学) / 甲第22627号 / 理博第4616号 / 新制||理||1663(附属図書館) / 京都大学大学院理学研究科物理学・宇宙物理学専攻 / (主査)准教授 市川 温子, 教授 中家 剛, 准教授 窪 秀利 / 学位規則第4条第1項該当 / Doctor of Science / Kyoto University / DFAM