<p> The isotopic composition and concentration of dissolved helium have been measured in over 250 samples of Atlantic and Pacific seawater. The helium isotope ratios were measured using a double collection "static" mass spectrometer specifically designed and constructed for this purpose. The helium and neon contents of 118 of these samples were determined using the isotope dilution technique, and the helium contents of the remaining samples were determined by peak-height comparison with standard air aliquots. Krypton and xenon concentrations were measured by isotope dilution for the Pacific samples. </p> <p> Two sources of excess nonatmospheric ³He are discerned in the Atlantic Ocean: a primordial component and a component produced by in situ decay of bomb-produced tritium. The former component occurs in three distinct features; two emanating from the south at 1000 m and greater than 4000 m depths, and one emanating from the north at about 3000 m depth. The spatial properties of these features are studied in the framework of simple models. The latter, or "tritiugenic" component is coupled with tritium concentrations measured by others to obtain Tritium-helium Ages, the characteristics of which are compared with hydrographic features. For example, the spreading velocity of the Mediterranean Water is determined to be ⪝ 1.5cm sec⁻¹ in the North-Western Atlantic. </p> <p> The helium and neon concentrations measured in Atlantic Waters indicate that significant variations occur for helium contents, both as a function of depth and latitude. The Antarctic Bottom Water appears to be a source of excess helium. </p> <p> In the Pacific, the distribution of excess ³He is shown to be consistent with injection of primordial ³He into the Deep and Bottom Waters from the East Pacific Rise. The characteristic mid-depth maximum seen in the helium isotope ratio anomaly profiles is shown to be a circulational feature. Upper and lower limits on the amount of excess nonatmospheric ⁴He are set at 5.5 and 2.6% respectively. Application of the simple one-dimensional diffusive-advective model indicate an upward flux of 6±2 and 1.1 ± 0.5 × 10⁶ atoms/cm²/sec for ³He and ⁴He respectively. </p> Pacific seawater is, on the average, 16 and 31% supersaturated in krypton and xenon respectively. Although there is no known process that is capable of such enrichments, the spatial distribution of the krypton and xenon concentrations indicate that a significant amount of the enrichment occurs in situ in Pacific Deep Waters. </p> / Thesis / Doctor of Philosophy (PhD)

Thesis (Ph.D.)--McMaster University (Canada), 1991. / Source: Dissertation Abstracts International, Volume: 54-02, Section: B, page: 0821.

Thesis (Ph.D.)--McMaster University (Canada), 1995. / Source: Dissertation Abstracts International, Volume: 56-12, Section: B, page: 6770. Adviser: G. J. Schrobilgen.

The yields of xenon and krypton from the neutron- induced fission of Am241 and Am242 have been measured with a mass spectrometer. This was accomplished by irradiating samples of Am241 for different lengths of time so that the effect of the growth of highly fissionable Am242 could be determined. These studies reveal that both the degree of fine structure in the mass yield curve and the fission-product charge distribution are dependent on the energy of the incident neutrons. This has not been previously observed for any fissioning nuclide. These studies also reveal effects of the 50-neutron shell and of the neutron-proton ratio of the fissioning nuclide on the mass yield curve. / Thesis / Doctor of Philosophy (PhD)

No description available.

Les travaux de cette thèse concernent la compréhension à l'échelle atomique des processus physico chimiques intervenant aux interfaces et dans des phases diluées. Pour commencer, nous avons étudié l'interaction entre la molécule 1,4-diazabicyclo [2.2.2]octane (DABCO) et un atome de gaz rare (He, Ne, Ar, Kr). Nous avons effectué une analyse systématique de ces systèmes, et nous en avons conclu que la méthode MP2 associée à une base diffuse est suffisamment précise pour décrire le système DABCO – Ar. Les surfaces d'énergie potentielle des complexes DABCO – gaz rare ont été calculées, ce qui nous a permis de réattribuer les spectres expérimentaux de ces espèces. Ensuite, nous nous sommes concentré sur les complexes DABCO – Arn (avec n = 2, 3, 4) neutres et ioniques. Nous avons montré que le DABCO interagi avec les atomes d'argon, et subit des déformations dues à l'effet de cette interaction faible sur ses modes de vibration. Par la suite, nous avons étudié les plus bas états électroniques du DABCO – Arn (n = 1, 2, 3). Nos résultats pourront être étendus à l'interprétation qualitative des études spectroscopiques et dynamiques des molécules de DABCO absorbés dans de grands agrégats d'argon. Enfin, nous avons étudié l'interaction entre l'imidazole et une couche d'or en présence de CO2. Nous avons montré que la molécule d'imidazole se fixe à l'agrégat d'or par une liaison covalente entre l'atome d'azote et un atome d'or, ainsi que des interactions faibles de type van der Waals entre les atomes d'hydrogène et la surface d'or. Nous avons déterminé que le site préférentiel pour l'interaction imidazole – or est le site top. Cette interaction permet un transfert de charge de l'imidazole vers la surface d'or, ce qui affecte la capture du CO2 (environ 50% plus faible par rapport à l'interaction Im(seule) – CO2). Mais l'augmentation du nombre de molécules d'imidazole à la surface de la couche d'or pourrait permettre une liaison plus forte entre le CO2 et l'imidazole / This thesis concern the understanding at the atomic level of physicochemical processes occurring at interfaces and dilute phases. First, we studied the interaction between the 1,4- diazabicyclo [2.2.2] octane (DABCO) molecule and a rare gas atom (He, Ne, Ar, Kr). We conducted a systematic analysis of these complexes, and we concluded that the MP2 method with a diffuse basis set is accurate to describe the system DABCO – Ar. The potential energy surfaces of DABCO – rare gas complexes were calculated, which allowed us to reatribuate the experimental spectra of these species. Then, we focused on DABCO – Arn (n = 2, 3, 4) neutral and ionic clusters. We have shown that the DABCO interacted with argon atoms and undergoes deformation due to the effect of the weak interaction on his vibrational modes. Subsequently, we studied the lowest electronic states of DABCO – Arn (n = 1, 2, 3). Our results can be extended to the qualitative interpretation of spectroscopic and dynamic studies of absorbed DABCO in large argon clusters. Finally, we studied the interaction between imidazole and a gold surface with CO2. We have shown that the imidazole molecule binds to the gold surface by a covalent bond between the nitrogen atom and a gold atom, and van der Waals interactions between hydrogen atoms and the gold surface. We determined that the preferred site for the imidazole – gold interaction is the top site. This interaction allows a charge transfer from the imidazole to the gold surface, which affects the capture of CO2 (about 50% lower compared to the interaction Im – CO2). But increase number of imidazole molecules on the gold surface could lead to a stronger bond between CO2 and imidazole

Dans cette thèse nous étudions le comportement thermique de matériaux cristallins, par le biais de la simulation Monte Carlo. Cette méthode est l'une des plus efficaces pour traiter ce genre de problématique.Nous présentons notre algorithme basé sur l'optimisation de la procédure de Verlet. Il nous a permis d'étudier le comportement thermiqued'un cristal jusqu'à la fusion, avec des simulations très longues et contenant des nombres importants d'atomes (plusieurs milliers) pour de meilleures statistiques sans avoir des temps CPU prohibitifs.Nous avons appliqué cet algorithme aux cristaux de gaz rares en utilisant le potentiel de Lennard-Jones (LJ), avec les paramètres calculés par Bernardes (les plus utilisés) en 1958.Or nos résultats montrent que ces paramètres conduisentà une surestimation des températures de fusion de ces cristaux par rapport aux températures de fusion expérimentalement mesurées. Nous avons donc proposé unemodification des paramètres qui permet un meilleur accord avec l'expérience.Nous avons aussi étudié la fusion des semi-conducteurs et des métaux en prenant le cas du silicium de structure diamant et le cas de l'argent de structurecubique à faces centrées.L'objectif étant de comprendre le comportement thermique et la fusion de ces matériaux tridimensionnels avant d'examiner les cas des cristauxbidimensionnels et semi-infinis. Ces matériaux, dans l'état massif, ont été expérimentalement bien étudiés. Malgré ceci, il n'y a pas derésultats théoriques et de simulations satisfaisants sur la transition de fusion. L'un des problèmes majeurs dans l'étude de fusion est le choix d'un potentiel capable de reproduire, aux basses températures, des structures de réseaux autres que le réseau FCC. Nous avons choisi les potentiels de Stillinger-Weber et de Tersoff pour Si, et les potentiels de Gupta et EAM (embedded atom method) pour Ag.Les résultats obtenus pour les deux potentiels sont similaires et meilleurs que les résultats publiés dans la littérature. Ils sont en accord avec l'expérience.Nous avons aussi traité le cas d'un problème très étudié, mais restant controversé: le comportement de la surface (111) d'un cristal d'argent. Expérimentalement,certaines études ont montrée que la distance entre la surface et la deuxième couche atomique subit une contraction aux basses températures. Au fur et à mesure que latempérature augmente, cette distance rattrape celle entre deux couches intérieures et puis la dépasse: ce résultat est connu sous le nom d'anomalie de dilatationthermique. Nous avons étudié ce problème en prenant deux potentiels multi-corps EAM et Gupta. Les résultats montrent que le potentielEAM décrit mieux cette anomalie, qui a lieu après la fusion de la surface, que le potentiel de Gupta.Par conséquent, l'anomalie de dilatation évoquée n'a pas lieu avec le potentiel de Gupta.Finalement, nous avons étudié la stabilité thermique d'une feuille de Silicène libre, c'est-à-dire non supportée par un substrat. Cematériau attire l'attention de nombreux chercheurs du fait de ses propriétés électroniques et thermiques qui semblent comparables à celles du graphène,de même structure en nids d'abeille mais avec des atomes de carbone. C'est l'un des matériaux les plusétudiés actuellement en raison des propriétés remarquables pour des applications. En utilisant le potentiel de Tersoff avec deux jeux de paramètres,nous avons montré que la structure 2D du silicène est stable jusqu'à la fusion qui a lieu à une température élevée, malgré la basse dimension du matériau. Il est à noter que le matériaun'a pas le même comportement selon le jeu de paramètres utilisé. En outre, nous n'avons pasobservé le "buckling" avec le potentiel de Tersoff. Le potentiel de Stillinger-Weber donne, en revanche, un buckling mais la structure se déforme vers une structure tri-dimensionnelle à la fusion.La conclusion générale et les perspectives sont présentées en fin de mémoire. / In this thesis we study thermal properties and melting behavior of crystals using Monte Carlo simulations. The Monte Carlo method is very difficult to implementfor melting investigation, unlike for problems where particles (such as spins) are localized on lattice sites. However, once it is well conceived, it is among themost efficient numerical techniques, to be able to study melting.We have created a high-performance algorithm based on an optimized Verlet procedure, which allowed us to investigate thermalproperties up to the melting. This optimization was necessary for treating an important number of atoms in very long runsto have good statistics, without prohibitive CPU time.We applied our algorithm to rare-gas crystals using the Lennard-Jones potential with parameters given by Bernardes which are widely used in the literature since 1958.Our results, thanks to their precision, show that we should modify these parameters in order to have a good agreement with experimental data.We studied melting of bulk semiconductors and metals by considering the case of Si and Ag. These materials have been chosen to serve our project about Silicene. Silicon has a diamond structure, and silver has the FCC lattice structure, both of them have been well experimentallystudied with well-known experimental melting temperatures. In spite of this, no good simulations have been done. For Si, one of the major problems is thechoice of a potential which stabilizes the diamond structure at finite temperatures. We have applied our algorithm to these materials using the multi-body Stillinger-Weber and Tersoff potentials for Si and the Gupta and EAM(embedded atom method) potentials for Ag. We obtained results much more precise than in early simulations and in good agreement with experiments.We also studied the Ag(111) surface trying to elucidate the long-standing controversy whether or not there is the ``anomalous'' thermal expansion whichhappens, for certain metals, when the inter-layer distances between the topmost atomic planes changes from a contracted situation to an expansion with respect tothe bulk distance. We showed that, depending on the potential, the anomalous crossover exists and the surface melting can occur at a temperature very far belowthat of the bulk melting. This is the case of EAM potential, but not the Gupta potential where surface melting occurs just belowbulk the melting.Finally, we studied the thermal stability of a stand-alone silicene sheet. Silicene is the Si counterpart of 2D carbon sheet called ``graphene". Siliceneattracts the attention of many researchers, because of its electronic and thermal properties which seem to be comparable to those of graphene which is actually oneof the most studied materials, due to its unusual properties susceptible for revolutionary device applications. Furthermore, because it is a Si-based material, thecompatibility, with the actual Si-based electronic industry, is expected to be better than for graphene. We show that, using the Tersoff potential with twosets of parameters (the original and the modified ones), the silicene 2D honeycomb structure is stable up to high temperatures without buckling. We have tested the Stillinger-Weberpotential: it yields a buckled honeycomb sheet at low temperatures but the 2D structure is destroyed in favor of a tri-dimensional structureat the melting. Discussion on this point is given.A general conclusion with some open perspectives is given at the end.

A collection of >3000 MOFs with experimentally confirmed structures were screened for performance in three binary separations: Ar/Kr, Kr/Xe, and Xe/Rn. 70 materials were selected for further analysis, and calculations were performed to account for inaccessible regions. Single component GCMC calculations were performed to parameterize IAST calculations on these 70 materials, and the curve fitting problem in IAST was discussed. IAST calculations were confirmed with extensive binary GCMC calculations. For each binary separation, materials were identified with predicted performance that surpasses the state of the art. "Reverse selective" materials, for which a smaller gas species is preferably adsorbed over a larger species, were explained on the basis of surface fractal geometry, computed via a corrected surface area calculation. The effect of temperature on separation performance was also examined.

In this thesis we study thermal properties and melting behavior of crystals using Monte Carlo simulations. The Monte Carlo method is very difficult to implementfor melting investigation, unlike for problems where particles (such as spins) are localized on lattice sites. However, once it is well conceived, it is among themost efficient numerical techniques, to be able to study melting.We have created a high-performance algorithm based on an optimized Verlet procedure, which allowed us to investigate thermalproperties up to the melting. This optimization was necessary for treating an important number of atoms in very long runsto have good statistics, without prohibitive CPU time.We applied our algorithm to rare-gas crystals using the Lennard-Jones potential with parameters given by Bernardes which are widely used in the literature since 1958.Our results, thanks to their precision, show that we should modify these parameters in order to have a good agreement with experimental data.We studied melting of bulk semiconductors and metals by considering the case of Si and Ag. These materials have been chosen to serve our project about Silicene. Silicon has a diamond structure, and silver has the FCC lattice structure, both of them have been well experimentallystudied with well-known experimental melting temperatures. In spite of this, no good simulations have been done. For Si, one of the major problems is thechoice of a potential which stabilizes the diamond structure at finite temperatures. We have applied our algorithm to these materials using the multi-body Stillinger-Weber and Tersoff potentials for Si and the Gupta and EAM(embedded atom method) potentials for Ag. We obtained results much more precise than in early simulations and in good agreement with experiments.We also studied the Ag(111) surface trying to elucidate the long-standing controversy whether or not there is the ''anomalous'' thermal expansion whichhappens, for certain metals, when the inter-layer distances between the topmost atomic planes changes from a contracted situation to an expansion with respect tothe bulk distance. We showed that, depending on the potential, the anomalous crossover exists and the surface melting can occur at a temperature very far belowthat of the bulk melting. This is the case of EAM potential, but not the Gupta potential where surface melting occurs just belowbulk the melting.Finally, we studied the thermal stability of a stand-alone silicene sheet. Silicene is the Si counterpart of 2D carbon sheet called ''graphene". Siliceneattracts the attention of many researchers, because of its electronic and thermal properties which seem to be comparable to those of graphene which is actually oneof the most studied materials, due to its unusual properties susceptible for revolutionary device applications. Furthermore, because it is a Si-based material, thecompatibility, with the actual Si-based electronic industry, is expected to be better than for graphene. We show that, using the Tersoff potential with twosets of parameters (the original and the modified ones), the silicene 2D honeycomb structure is stable up to high temperatures without buckling. We have tested the Stillinger-Weberpotential: it yields a buckled honeycomb sheet at low temperatures but the 2D structure is destroyed in favor of a tri-dimensional structureat the melting. Discussion on this point is given.A general conclusion with some open perspectives is given at the end.

L'importance des effets relativistes dans la chimie a été reconnu depuis les années 1980. Par exemple, sans la relativité (a) l'or aurait la même couleur que l'argent (b) le mercure ne serait pas liquide à la température ambiante et (c) nos voitures ne démarrent pas avec une batterie de plomb. Pour une description théorique de la structure et la réactivité des éléments lourds, la relativité est un ingrédient essentiel. Le hamiltonien pour les calculs moléculaires relativistes à 4 composantes est construit en remplaçant la partie mono-électronique de l'hamiltonien électronique non-relativiste par le hamiltonien de Dirac. La partie bi-électronique est approchée par le terme de r Coulomb comme dans le cas non relativiste, ce qui donnel'hamiltonien de Dirac-Coulomb (DC). Pour réduire le coût de calcul, on peut utiliser des hamiltoniens relativistes à 2 composantes. Parmi eux, l'hamiltonien exact à 2 composantes (X2C) est le plus précise. La corrélation électronique est, cependant, une contribution très importante pour obtenir une description théorique à la fois qualitative et quantitative des spectroscopies moléculaires, réactions, etc. Dans cette thèse, nous avons étudié l'interaction entre la relativité et de la corrélation. à la fois par des développements méthodologiques et par des applications moléculaires. Dans la première partie de la thèse, nous avons calculé les constantes spectroscopiques dimères des gaz rares lourds. La liaison faible de ces dimères ne peut être décrit que par l'inclusion de la corrélation électronique. Les dimères des gaz rares les plus lourds, le radon et l'eka-radon, nécessite de plus un traitement adéquat de la relativité. Nos calculs sont basés sur l'hamiltonien X2Cmmf, à la fois avec des méthodes de corrélation basés sur une fonction d'onde et séparation de porte (srDFT). La deuxième partie de cette thèse concerne la simulation de la spectroscopie des rayons X, où l'on sonde la région du cœur d'une molécule, ou la relativité joue un rôle très important. Nous avons étudié la spectroscopie L-edge de la série isoélectronique: UO22 +, UNO+, et UN2, où le couplage spin-orbite joue un rôle majeur. Au niveau des méthodes, nous avons considéré MP2 à couches ouvertes et la théorie de la fonctionnelle de la densité dépendante de temps (TDDFT). Dans un autre étude, nous avons simulé la spectroscopie K-edge de la série H2X (X = O, S, Se, Te) et XH3 (X = N, P, As) ainsi que les molécules N2 et N2O2. Pour ces systèmes, l'interaction spin-orbite est moins important. Par conséquent, nous avons utilisé un hamiltonien DC sans spin (SF). Certains des systèmes pris en compte dans ce travail sont de caractère multi-référentielles ; nous avons utilisé la methode Coupled Cluster Multi-référentielle de type State Universal et adapté au groupe unitaire (UGA-SUMRCC) comme une méthode de corrélation. Dans la troisième et partie principale de la thèse, l'attention est de nouveau sur la relativité et de la corrélation, mais pour le calcul des propriétés électriques et magnétiques moléculaires. Nous avons développé et mis en œuvre un module pour le calcul des valeurs moyennes au niveau relativiste à 4-composantes coupled cluster monoréferentiel. Les propriétés qui sondent la densité électronique près de noyaux (lourds), telles que la résonance paramagnétique électronique (RPE), les paramètres des gradients de champ électrique et la non-conservation de la parité (NCP) des molécules chirales ,sont parfaitement adaptés pour l'application de cette méthode. Pour l'instant, nous avons étudié que la NCP. Ce module dans le logiciel DIRAC pour les calculs moléculaires relativistes fournit un cadre propice pour la mise en œuvre de méthodes de CC relativistes employant la symétrie de groupes doubles et de permutation de manière très efficace. En perspective, nous ciblons la mise en œuvre de la réponse linéaire CC pour le calcul des énergies d'excitation et propriétés moléculaires de second ordre tels que les paramètres de RMN. / The importance of relativistic effects in chemistry has been recognized since the 1980s. Without relativity (a) gold would have the same colour as silver (b) mercury would not be liquid at room temperature (c) our cars would not start (lead-battery). For a theoretical description of the structure and reactivity of heavy-elements, relativity is considered as an essential ingredient. The Hamiltonian for the 4-component relativistic molecular calculations is constructed by replacing the one-electronic part of the non-relativistic molecular Hamiltonian by the Dirac Hamiltonian. The two-electronic part of the Hamiltonian is approximated by the Coulombic repulsion term as in the non-relativistic case. The resulting Hamiltonian is called the Dirac-Coulomb (DC) Hamiltonian. For chemical applications there exist a class of relativistic Hamiltonians, where one-electronic part of the DC Hamiltonian is transformed to a 2-component one. Among them the eXcact 2-component (X2C) Hamiltonian is the most accurate one. Electron correlation, however, is a very important contribution to achieve a both qualitative and quantitative correct description of molecular spectroscopies, reactions etc. It is, therefore, essential to study the interplay between relativity and correlation. In this thesis, we have studied this interplay both in terms methodological developments and molecular applications. In the first part of the thesis we have studied the spectroscopic constants of the heavy rare gas dimers. The weak bonding of those dimers can only be described by the inclusion of electron correlation. The heavier analogues in the rare gas series i.e, Radon and eka-Radon, in addition require adequate treatment of relativity. Our calculations are based on the eXact 2-Component molecular-mean field (X2Cmmf) Hamiltonian both with wave function methods and range-separated DFT methods. The second part of this thesis simulates X-ray spectroscopy, where one probes the core region of a molecule. In the core region relativity plays a very significant role. Removal and excitation of electrons from that region involve various processes, which are beyond a mean-field description. We have studied L-edge spectroscopy of the isoelectronic series: UO22+, UNO+, and UN2, where spin-orbit coupling plays a major role. For the theory we have considered single reference open-shell MP2 and Time Dependent Density functional Theory (TDDFT). In another work, we have studied K-edge spectroscopy of the H2X (X= O, S, Se, Te) and XH3 (X= N, P, As) series as well as N2, N2O2 molecules. For this study spin-orbit coupling is less important, therefore, we have treated them with the Spin-Free (SF) DC Hamiltonian. Some of the systems considered in this work are Multi-Reference in nature; we have used Unitary Group Adapted (UGA) State Universal Multi-reference Coupled Cluster (UGA-SUMRCC) theory as a correlation method. In the third and major part of the thesis, the thrust is again on relativity and correlation, but for the calculation of molecular electric and magnetic properties. We have developed and implemented a module for the calculation of expectation values at the 4-component Relativistic Single Reference Coupled Cluster level. Properties that probe the electron density near (heavy) nuclei, such as Electron Paramagnetic Resonance (EPR) parameters, electric field gradients and parity non-conservation (PNC) in chiral molecules are ideally suited for the application of this method. However, we have only studied PNC so far. This module in the DIRAC software for relativstic molecular calculations provides a convenient framework for the implementation of relativistic CC methods employing double group and permutation symmetry very efficiently. In the near future we therefore target the implementation of Linear Response CC for the calculation of excitation energies and second-order molecular properties such as NMR parameters.