Desenvolvemos urna teoria cinética para urna mistura de gases ionizados em presença de campos elétricos e magnéticos. As leis de Ohm, Fourier e Navier-Stokes são obtidas por dois métodos distintos que se baseiam na equação de Boltzmann. Verificamos que o emprego de teoremas de representação torna o método de Chapman-Enskog mais direto. Entretanto o método combinado mostrou-se extremamente simples, onde os coeficientes de transporte são determinados através da inversão de tensores de segunda e quarta ordens. Calculamos também a integral de colisão para as possíveis interações em gases ionizados tais como, entre partículas carregadas, partícula carregada e partícula neutra e entre partículas neutras. Como uma aplicação do método combinado, determinamos os coeficientes de condutividade elétrica, condutividade térmica, coeficiente termo-elétrico e o coeficiente de viscosidade cisalhante para um gás totalmente ionizado. Obtemos seus respectivos gráficos, considerando então um gás ionizado formado a partir do gás de hélio. / We develop a kinetic theory for ionized gases mixtures under the presence of electric and magnetic fields. The laws of Ohm, Fourier and Navier-Stokes are obtained by two different methods based on the Boltzmann equation. We verify that the use of representation theorems makes the Chapman-Enskog method more direct. However the combined method shows up as extremely simple where the transport coefficients are determined through inversion of second-order and fourth order tensors. We calculate also the collision integrals for possible interactions in ionized gases like: between charged particles, between charged particles and neutral particles and between neutral particles. As an application of the combined method, we determine the electrical and thermal conductivity coefficients, thermo-electric and shear viscosity coefficients for a completely ionized gas. We obtain their respective graphics considering an ionized gas of helium.

Electromagnetic acceleration has the potential for various applications stemming from space electric propulsion systems to future air breathing hypersonic augmentation.<p>Electromagnetic acceleration uses electromagnetic body force produced by the interactions of currents carried in plasma which is either externally applied or self-induced magnetic fields to accelerate the whole body of gas. Historically, these plasmas sources have been arc jets, shock tube and microwaves. Never has an electromagnetic accelerator been powered by an inductively coupled plasma (ICP) source.<p>The von Karman Institute has experimentally investigated the acceleration of an electrically conductive fluid produce by a subsonic ICP source. This ICP source was powered with a 15 kW and 27.1 MHz radio frequency facility called the Minitorch. The electromagnetic acceleration was accomplished with the design, fabrication and testing of a linear Hall current magnetofluiddynamic accelerator (MFDA) channel. The channel was geometrically orientated into the Hall configuration to accounts for the large Hall Effect. This channel used a single pair of copper annulus electrodes powered by a 10 kW direct current power supply. The channel was water cooled and contained various diagnostics to provide greater insight to the electromagnetic acceleration process. This was the first successful magnetofluiddynamic acceleration of an ICP source and validates the proof of concept.<p>One-dimensional MFD modeling was formulated and used to determine the necessary performance requirements of the MFDA channel E and B field subsystems. An interaction parameter of approximately 2.25 was required for the doubling of an inlet velocity of 300 m/sec. The required subsystem need to provide a current density was 6 Amps/cm2 with a magnetic field strength of 0.50 Tesla over an acceleration length of 0.1 meters. Additional the most critical constraint was the thermal management subsystem which was designed to overcome large heat transfer fluxes to achieve a steady state condition over a test run of 10 minutes.<p>The dynamic pressure measured increase the inlet velocity 101% for an argon plasma flowing at 1.01 g/s at a magnetic field strength of 0.49 Tesla. his strong acceleration of the plasma was most notable near the region of the electrodes at the exit of the 0.1 m long channel. The central region of the plasma has less dynamic pressure increase corresponding to only a maximum of 15% increase in velocity at a magnetic strength of 0.49 Tesla. Experimental results showed that axial discharge voltages increased with increased magnetic fields, indicating a strong Hall Effect in the accelerator as expected.<p>Theoretical analysis was accomplished using the one-dimensional equation of motion and was compared to utilizing only the momentum equation. Experimental force fluxes were compared to the calculated values of the one-dimensional equation of motion and momentum equation. The reference area for the current density was selected from intensity measurement using a high speed camera with the MFDA channel on. There was significant error in the analysis concerning using the momentum Lorentz force only versus the one-dimensional equations of motion; which included joule heating. This analysis summarized the necessity to include joule heating in the formulation of the problem. / Doctorat en sciences appliquées / info:eu-repo/semantics/nonPublished

An artificially structured boundary (ASB) produces a short-range, static electromagnetic field that can reflect charged particles. In the work presented, an ASB is considered to consist of a spatially periodic arrangement of electrostatically plugged magnetic cusps. When used to create an enclosed volume, an ASB may confine a non-neutral plasma that is effectively free of applied electromagnetic fields, provided the spatial period of the ASB-applied field is much smaller than any one dimension of the confinement volume. As envisioned, a non-neutral positron plasma could be confined by an ASB along its edge, and the space-charge of the positron plasma would serve to confine an antiproton plasma. If the conditions of the two-species plasma are suitable, production of antihydrogen via three-body recombination for antimatter gravity studies may be possible. A classical trajectory Monte Carlo (CTMC) simulation suite has been developed in C++ to efficiently simulate charged particle interactions with user defined electromagnetic fields. The code has been used to explore several ASB configurations, and a concept for a cylindrically symmetric ASB trap that employs a picket-fence magnetic field has been developed. Particle-in-cell (PIC) modeling has been utilized to investigate the confinement of non-neutral and partially neutralized positron plasmas in the trap.

Magnetic plasma expulsion uses a magnetic field distortion to redirect incident charged particles around a certain area for the purposes of shielding. Computational studies are carried out and for certain values of magnetic field, magnetic plasma expulsion is found to effectively shield a sizable area. There are however many plasma behaviors and interactions that must be considered. Applications to a new cryogenic antimatter trap design are discussed.

Laser Induced Breakdown Spectroscopy (LIBS) is showing great potential as an atomic analytical technique. With its ability to rapidly analyze all forms of matter, with little-to-no sample preparation, LIBS has many advantages over conventional atomic emission spectroscopy techniques. With the maturation of the technologies that make LIBS possible, there has been a growing movement to implement LIBS in portable analyzers for field applications. In particular, LIBS has long been considered the front-runner in the drive for stand-off detection of trace deposits of explosives. Thus there is a need for a better understanding of the relevant processes that are responsible for the LIBS signature and their relationships to the different system parameters that are helping to improve LIBS as a sensing technology. This study explores the use of LIBS as a method to detect random trace amounts of specific organic materials deposited on organic or non-metallic surfaces. This requirement forces the limitation of single-shot signal analysis. This study is both experimental and theoretical, with a sizeable component addressing data analysis using principal components analysis to reduce the dimensionality of the data, and quadratic discriminant analysis to classify the data. In addition, the alternative approach of ‘target factor analysis’ was employed to improve detection of organic residues on organic substrates. Finally, a new method of characterizing the laser-induced plasma of organics, which should lead to improved data collection and analysis, is introduced. The comparison between modeled and experimental measurements of plasma temperatures and electronic density is discussed in order to improve the present models of low-temperature laser induced plasmas.

The Cosmic Microwave Background (CMB) serves as a powerful backlight, illuminating thestructures throughout the universe. As the CMB photons travel to our telescopes from the surface of last scattering, their interactions with matter imprint detectable signatures in the CMB spectrum, known as the CMB secondary anisotropies. Among these late-time phenomena, the Sunyaev–Zel’dovich (SZ) effect—caused by scattering of the CMB photons off free electrons—is one of the most powerful, providing a unique window into the pressure and density of the electron gas. As the ionized gas and its feedback on the underlying dark matter distribution via high-energy processes present a significant obstacle to obtain precise cosmological constraints from the matter power spectrum, the SZ effect serves as an invaluable tool to address these challenges. This thesis uses the measurements of the CMB secondary anisotropies, particularly the SZ effect, from the state-of-the-art experiments, the Planck satellite and the ground-based Atacama Cosmology Telescope (ACT), in combination with Large-Scale Structure data to probe the ionized gas in distant galaxies. Chapter 2 presents the second measurement of the kinetic SZ effect in the unWISE galaxies with Planck using the projected-fields estimator. This work concludes that the ionized gas abundance in these galaxies matches the primordial-CMB predictions. Chapter 3 describes the work done to model the galaxy-halo connection of the unWISE catalog with Planck CMB lensing data using the halo model framework. It constrained the halo masses of these samples to ≈ 2 ×10¹³ _⊙/ℎ, and found that they are dominated by central galaxies, rather than satellites. These constraints can be directly used in other cross-correlations of unWISE with, e.g., the tSZ or the kSZ effect in the halo model with the upcoming CMB experiments. Chapter 5 discusses the ongoing work of cross-correlating the Dark Energy Survey Maglim galaxies with the thermal SZ maps from ACT. It measures very extended pressure profiles around Maglim, which suggest strong feedback activity in low mass objects, pushing the ionized gas far outside of the halo. This thesis also presents novel techniques to tackle the key systematics in cosmological cross-correlations. The analysis of Maglim galaxies employs the new Cosmic Infrared Background (CIB) cleaning technique, the moment-deprojection method, which ensures that the measurement is robust to this foreground. Chapter 4 discusses three new methods to remove the CIB and tSZ contamination, using the external Large-Scale Structure data which show a large correlation with both fields (e.g., the unWISE catalog). With the new methods presented, it is possible to remove those contaminants to enhance the measurements of the blackbody component of a CMB map. The results presented in this thesis offer a unique window into the baryons residing in distant galaxies through the SZ effect, confirming there is no missing baryons, and indicating that the feedback is stronger than predicted in simulations. These analyses lay the groundwork for cross-correlations of the upcoming high-resolution, low-noise CMB experiments such as the Simons Observatory, and high density galaxy surveys, including DESI, Euclid, or LSST. The upcoming measurements will yield precise constraints on gas physics, transforming our understanding of galaxy formation, and enabling cosmological constraints from the matter power spectrum, where baryons currently represent the primary uncertainty.

Spider pulsars are compact binary systems consisting of a millisecond pulsar and a low-mass companion. Their X-ray emission, modulated on the orbital period, is interpreted as synchrotron radiation from high-energy electrons accelerated at the intrabinary shock. In this dissertation, we conduct global two-dimensional particle-in-cell simulations of the intrabinary shock, assuming the shock wraps around the companion star. When the pulsar spin axis is nearly aligned with the orbital angular momentum, the magnetic energy of the relativistic pulsar wind, composed of magnetic stripes of alternating field polarity, efficiently converts to particle energy at the intrabinary shock via shock-driven reconnection. The highest energy particles accelerated by reconnection can stream ahead of the shock and be further accelerated by the upstream motional electric field. In the downstream, further energization is governed by stochastic interactions with the plasmoids or magnetic islands generated by reconnection. Our results show that the synchrotron spectrum is nearly flat, 𝐹_𝜈 ∝, and the light curve displays two peaks just before and after the pulsar eclipse (superior conjunction), separated in phase by approximately 0.8 rad, with the peak flux exceeding that at inferior conjunction by a factor of ten. Additionally, we consider radiative losses in the form of synchrotron cooling using the reduced Landau-Lifshitz model. We examine three cooled scenarios, with a synchrotron burnoff limit (𝜰_rad) of 120, 60, and 30, comparing these simulations to an uncooled case to understand the impact of radiative losses on particle acceleration and emission.

A comprehensive investigation was reported into the synthesis, characterization and photoluminescence properties of calcium metaniobates and associated alkali earth alloy systems. Previous studies have shown that calcium metaniobate exhibits a strong self-activated blue luminescence at room temperature in stark contrast to the pyroniobates which are known to exhibit a temperature dependent luminescence that quenches above 100 K. The mechanism of this behavior has been studied by measuring the spectral characteristics of the photoluminescence and photoluminescence excitation spectra on the crystalline and morphological properties of the powders as determined from x-ray diffraction and scanning electron microscopy. By correlating the synthesis parameters with the physical, chemical and optical properties of calcium metaniobate, the optimum conditions for efficient blue-visible emission and chemical stability under vacuum ultraviolate (VUV) radiation has been determined. These materials have the potential to replace Barium Magnesium Aluminate, which is currently used as the blue phosphor in plasma displays.

The chamber walls in inertial fusion reactors must be protected from the photons and ions resulting from the target explosions. One way this can be accomplished is through a sacrificial liquid wall composed of either liquid jets or thin liquid films. The x-rays produced by the exploding targets deposit their energy in a thin liquid layer on the wall surface or in the surface of liquid jets arrayed to protect the wall. The partially vaporized liquid film/jet forms a protective cloud that expands toward the incoming ionic debris which arrives shortly (a few s) thereafter. The charged particles deposit their energy in the vapor shield and the unvaporized liquid, thereby leading to further evaporation. Re-condensation of the vapor cloud and radiative cooling of the expanding plasma allow the energy deposited in the liquid to be recovered prior to the next target explosion (100ms). Chamber clearing prior to the next explosion represents a major challenge for all liquid protection systems, inasmuch as any remaining liquid droplets may interfere with beam propagation and/or target injection. Therefore, the primary objective of this research is to experimentally examine the interaction between liquid droplets and low- temperature, low-pressure plasmas under conditions similar to those expected following inertial fusion target explosions and the subsequent expansion. The data obtained in this research will be useful in validating mechanistic chamber-clearing models to assure successful beam propagation and target injection for the subsequent explosion.

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