548 resultados para Para magnetism


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How do the magnetic fields of massive stars evolve over time? Are their gyrochronological ages consistent with ages inferred from evolutionary tracks? Why do most stars predicted to host Centrifugal Magnetospheres (CMs) display no H$\alpha$ emission? Does plasma escape from CMs via centrifugal breakout events, or by a steady-state leakage mechanism? This thesis investigates these questions via a population study with a sample of 51 magnetic early B-type stars. The longitudinal magnetic field \bz~was measured from Least Squares Deconvolution profiles extracted from high-resolution spectropolarimetric data. New rotational periods $P_{\rm rot}$ were determined for 15 stars from \bz, leaving only 3 stars for which $P_{\rm rot}$ is unknown. Projected rotational velocities \vsini~were measured from multiple spectral lines. Effective temperatures and surface gravities were measured via ionization balances and line profile fitting of H Balmer lines. Fundamental physical parameters, \bz, \vsini, and $P_{\rm rot}$ were then used to determine radii, masses, ages, dipole oblique rotator model, stellar wind, magnetospheric, and spindown parameters using a Monte Carlo approach that self-consistently calculates all parameters while accounting for all available constraints on stellar properties. Dipole magnetic field strengths $B_{\rm d}$ follow a log-normal distribution similar to that of Ap stars, and decline over time in a fashion consistent with the expected conservation of fossil magnetic flux. $P_{\rm rot}$ increases with fractional main sequence age, mass, and $B_{\rm d}$, as expected from magnetospheric braking. However, comparison of evolutionary track ages to maximum spindown ages $t_{\rm S,max}$ shows that initial rotation fractions may be far below critical for stars with $M_*>10 M_\odot$. Computing $t_{\rm S,max}$ with different mass-loss prescriptions indicates that the mass-loss rates of B-type stars are likely much lower than expected from extrapolation from O-type stars. Stars with H$\alpha$ in emission and absorption occupy distinct regions in the updated rotation-magnetic confinement diagram: H$\alpha$-bright stars are found to be younger, more rapidly rotating, and more strongly magnetized than the general population. Emission strength is sensitive both to the volume of the CM and to the mass-loss rate, favouring leakage over centrifugal breakout.

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The bond formation between an oxide surface and oxygen, which is of importance for numerous surface reactions including catalytic reactions, is investigated within the framework of hybrid density functional theory that includes nonlocal Fock exchange. We show that there exists a linear correlation between the adsorption energies of oxygen on LaMO3 (M = Sc–Cu) surfaces obtained using a hybrid functional (e.g., Heyd–Scuseria–Ernzerhof) and those obtained using a semilocal density functional (e.g., Perdew–Burke–Ernzerhof) through the magnetic properties of the bulk phase as determined with a hybrid functional. The energetics of the spin-polarized surfaces follows the same trend as corresponding bulk systems, which can be treated at a much lower computational cost. The difference in adsorption energy due to magnetism is linearly correlated to the magnetization energy of bulk, that is, the energy difference between the spin-polarized and the non-spin-polarized solutions. Hence, one can estimate the correction ...

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Understanding the magnetic properties of graphenic nanostructures is instrumental in future spintronics applications. These magnetic properties are known to depend crucially on the presence of defects. Here we review our recent theoretical studies using density functional calculations on two types of defects in carbon nanostructures: Substitutional doping with transition metals, and sp$^3$-type defects created by covalent functionalization with organic and inorganic molecules. We focus on such defects because they can be used to create and control magnetism in graphene-based materials. Our main results are summarized as follows: i)Substitutional metal impurities are fully understood using a model based on the hybridization between the $d$ states of the metal atom and the defect levels associated with an unreconstructed D$_{3h}$ carbon vacancy. We identify three different regimes, associated with the occupation of distinct hybridization levels, which determine the magnetic properties obtained with this type of doping; ii) A spin moment of 1.0 $\mu_B$ is always induced by chemical functionalization when a molecule chemisorbs on a graphene layer via a single C-C (or other weakly polar) covalent bond. The magnetic coupling between adsorbates shows a key dependence on the sublattice adsorption site. This effect is similar to that of H adsorption, however, with universal character; iii) The spin moment of substitutional metal impurities can be controlled using strain. In particular, we show that although Ni substitutionals are non-magnetic in flat and unstrained graphene, the magnetism of these defects can be activated by applying either uniaxial strain or curvature to the graphene layer. All these results provide key information about formation and control of defect-induced magnetism in graphene and related materials.

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Magnetism and magnetic materials have been playing a lead role in the day to day life of human beings. The human kind owes its gratitude to the ‘lodestone’ meaning ‘leading stone’ which lead to the discovery of nations and the onset of modern civilizations. If it was William Gilbert, who first stated that ‘earth was a giant magnet’, then it was the turn of Faraday who correlated electricity and magnetism. Magnetic materials find innumerable applications in the form of inductors, read and write heads, motors, storage devices, magnetic resonance imaging and fusion reactors. Now the industry of magnetic materials has almost surpassed the semiconductor industry and this speaks volumes about its importance. Extensive research is being carried out by scientists and engineers to remove obsolescence and invent new devices. Though magnetism can be categorized based on the response of an applied magnetic field in to diamagnetic, paramagnetic, ferromagnetic, ferrimagnetic and antiferromagnetic; it is ferrimagnetic, ferromagnetic and antiferromagnetic materials which have potential applications. The present thesis focusses on these materials, their composite structures and different ways and means to modify their properties for useful applications. In the past, metals like Fe, Ni and Co were sought after for various applications though iron was in the forefront because of its cost effectiveness and abundance. Later, alloys based on Fe and Ni were increasingly employed. They were used in magnetic heads and in inductors. Ferrites entered the arena and subsequently most of the newer applications were based on ferrites, a ferrimagnetic material, whose composition can be tuned to tailor the magnetic properties. In the late 1950s a new class of magnetic material emerged on the magnetic horizon and they were fondly known as metallic glasses. They are well known for their soft magnetic properties. They were synthesized in the form of melt spun ribbons and are amorphous in nature and they are projected to replace the crystalline counterparts.

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Thermoelectric materials are revisited for various applications including power generation. The direct conversion of temperature differences into electric voltage and vice versa is known as thermoelectric effect. Possible applications of thermoelectric materials are in eco-friendly refrigeration, electric power generation from waste heat, infrared sensors, temperature controlled-seats and portable picnic coolers. Thermoelectric materials are also extensively researched upon as an alternative to compression based refrigeration. This utilizes the principle of Peltier cooling. The performance characteristic of a thermoelectric material, termed as figure of merit (ZT) is a function of several transport coefficients such as electrical conductivity (σ), thermal conductivity (κ) and Seebeck coefficient of the material (S). ZT is expressed asκσTZTS2=, where T is the temperature in degree absolute. A large value of Seebeck coefficient, high electrical conductivity and low thermal conductivity are necessary to realize a high performance thermoelectric material. The best known thermoelectric materials are phonon-glass electron – crystal (PGEC) system where the phonons are scattered within the unit cell by the rattling structure and electrons are scattered less as in crystals to obtain a high electrical conductivity. A survey of literature reveals that correlated semiconductors and Kondo insulators containing rare earth or transition metal ions are found to be potential thermoelectric materials. The structural magnetic and charge transport properties in manganese oxides having the general formula of RE1−xAExMnO3 (RE = rare earth, AE= Ca, Sr, Ba) are solely determined by the mixed valence (3+/4+) state of Mn ions. In strongly correlated electron systems, magnetism and charge transport properties are strongly correlated. Within the area of strongly correlated electron systems the study of manganese oxides, widely known as manganites exhibit unique magneto electric transport properties, is an active area of research.Strongly correlated systems like perovskite manganites, characterized by their narrow localized band and hoping conduction, were found to be good candidates for thermoelectric applications. Manganites represent a highly correlated electron system and exhibit a variety of phenomena such as charge, orbital and magnetic ordering, colossal magneto resistance and Jahn-Teller effect. The strong inter-dependence between the magnetic order parameters and the transport coefficients in manganites has generated much research interest in the thermoelectric properties of manganites. Here, large thermal motion or rattling of rare earth atoms with localized magnetic moments is believed to be responsible for low thermal conductivity of these compounds. The 4f levels in these compounds, lying near the Fermi energy, create large density of states at the Fermi level and hence they are likely to exhibit a fairly large value of Seebeck coefficient.

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Magnetism and magnetic materials have been playing a lead role in the day to day life of human beings. The human kind owes its gratitude to the ‘lodestone’ meaning ‘leading stone’ which lead to the discovery of nations and the onset of modern civilizations. If it was William Gilbert, who first stated that ‘earth was a giant magnet’, then it was the turn of Faraday who correlated electricity and magnetism. Magnetic materials find innumerable applications in the form of inductors, read and write heads, motors, storage devices, magnetic resonance imaging and fusion reactors. Now the industry of magnetic materials has almost surpassed the semiconductor industry and this speaks volumes about its importance. Extensive research is being carried out by scientists and engineers to remove obsolescence and invent new devices. Though magnetism can be categorized based on the response of an applied magnetic field in to diamagnetic, paramagnetic, ferromagnetic, ferrimagnetic and antiferromagnetic; it is ferrimagnetic, ferromagnetic and antiferromagnetic materials which have potential applications. The present thesis focusses on these materials, their composite structures and different ways and means to modify their properties for useful applications.

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If magnetism is universal in nature, magnetic materials are ubiquitous. A life without magnetism is unthinkable and a day without the influence of a magnetic material is unimaginable. They find innumerable applications in the form of many passive and active devices namely, compass, electric motor, generator, microphone, loud speaker, maglev train, magnetic resonance imaging, data recording and reading, hadron collider etc. The list is endless. Such is the influence of magnetism and magnetic materials in ones day to day life. With the advent of nanoscience and nanotechnology, along with the emergence of new areas/fields such as spintronics, multiferroics and magnetic refrigeration, the importance of magnetism is ever increasing and attracting the attention of researchers worldwide. The search for a fluid which exhibits magnetism has been on for quite some time. However nature has not bestowed us with a magnetic fluid and hence it has been the dream of many researchers to synthesize a magnetic fluid which is thought to revolutionize many applications based on magnetism. The discovery of a magnetic fluid by Jacob Rabinow in the year 1952 paved the way for a new branch of Physics/Engineering which later became magnetic fluids. This gave birth to a new class of material called magnetorheological materials. Magnetorheological materials are considered superior to electrorheological materials in that magnetorheology is a contactless operation and often inexpensive.Most of the studies in the past on magnetorheological materials were based on magnetic fluids. Recently the focus has been on the solid state analogue of magnetic fluids which are called Magnetorheological Elastomers (MREs). The very word magnetorheological elastomer implies that the rheological properties of these materials can be altered by the influence of an external applied magnetic field and this process is reversible. If the application of an external magnetic field modifies the viscosity of a magnetic fluid, the effect of external magnetic stimuli on a magnetorheological elastomer is in the modification of its stiffness. They are reversible too. Magnetorheological materials exhibit variable stiffness and find applications in adaptive structures of aerospace, automotive civil and electrical engineering applications. The major advantage of MRE is that the particles are not able to settle with time and hence there is no need of a vessel to hold it. The possibility of hazardous waste leakage is no more with a solid MRE. Moreover, the particles in a solid MRE will not affect the performance and durability of the equipment. Usually MR solids work only in the pre yield region while MR fluids, typically work in the post yield state. The application of an external magnetic field modifies the stiffness constant, shear modulus and loss modulus which are complex quantities. In viscoelastic materials a part of the input energy is stored and released during each cycle and a part is dissipated as heat. The storage modulus G′ represents the capacity of the material to store energy of deformation, which contribute to material stiffness. The loss modulusG′′ represents the ability of the material to dissipate the energy of deformation. Such materials can find applications in the form of adaptive vibration absorbers (ATVAs), stiffness tunable mounts and variable impedance surfaces. MREs are an important material for automobile giants and became the focus of this research for eventual automatic vibration control, sound isolation, brakes, clutches and suspension systems

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La presente tesis es un estudio dedicado a la optimización y desarrollo de sistemas del tipo juntura túnel. La metodología utilizada para la realización de la tesis consistió, en primer lugar, en la optimización de las componentes independientes de la juntura túnel: electrodo y barrera aislante. Posteriormente se optimizaron los procesos de fabricación para el desarrollo y caracterización de dispositivos del tipo juntura túnel en su forma final. En la primera parte de la tesis se analizan detalladamente los resultados obtenidos de la caracterización eléctrica y topografica de barreras aislantes en sistemas electrodo - barrera. Los sistemas bicapas estudiados, GdBa_2Cu_3_7/SrTiO_3, Nb/Ba_0,05Sr_0,95TiO_3 y YBa_2Cu_3O_7/SrTiO_3, fueron caracterizados utilizando un microscopio de fuerza atómica en modo conductor. Se propuso un modelo fenomenológico basado en los resultados experimentales, que permitió la obtención de parámetros críticos para el desarrollo de dispositivos del tipo juntura túnel con nuevas funcionalidades. La información obtenida de la caracterización de los sistemas bicapas (homogeneidad de crecimiento, baja densidad de defectos y de pinholes) indican un muy buen control de los parámetros de crecimiento de las barreras. Por otro lado, se obtuvo un buen comportamiento aislante para espesores mayores a 2 nm sin la presencia de pinholes en la barrera. La similitud en la estequiometría de las barreras (SrTiO_3) permitió comparar los distintos sistemas estudiados en términos de conductividad eléctrica. Se verificó que el modelo fenomenológico permite comparar la conductividad eléctrica de los sistemas mediante uno de los parámetros definidos en el modelo fenomenológico (obtenido de los ajustes lineales de las curvas I(V)). De los 3 sistemas estudiados, las bicapas GdBa_2Cu_3O_7/SrTiO_3 presentaron un mayor valor de longitud de atenuación de los portadores de carga a través de la barrera y una muy baja densidad de defectos superficiales. Las bicapas YBa_2Cu_3O_7/SrTiO_3 y Nb/Ba_0,05Sr_0,95TiO_3 permitieron validar el modelo fenomenológico propuesto para el análisis de la respuesta corriente - voltaje obtenida con el microscopio de fuerza atómica en modo conductor. La segunda parte de la tesis abarca conceptos de magnetismo y microfabricación para el desarrollo de junturas túnel magnéticas. Durante la caracterización de las películas ferromagnéticas individuales de Co_90Fe_10 (CoFe) se logró aumentar valor del campo coercitivo de films de 10 nm de espesor al incrementar la temperatura de depósito. Esto se debe a un aumento del tamaño de grano de los films. El aumento de la temperatura del sustrato durante el crecimiento influye en la morfología y las propiedades magnéticas de los films de CoFe favoreciendo la formación de granos y la pérdida del eje preferencial de magnetización. Estos resultados permitieron la fabricación de sistemas Co_90Fe_10/M_gO/Co_90Fe_10 con distintas orientaciones relativas accesibles con campo magnético para el estudio del acople magnético entre los films de CoFe. La caracterización eléctrica de estos sistemas, particularmente la respuesta corriente - voltaje obtenida con el microscopio de fuerza atómica en modo conductor, indicó que las propiedades de transporte eléctrico de las junturas presentan un alto grado de reproducibilidad. Se analizó además la inuencia del sustrato utilizado en la corriente túnel que atraviesa la barrera aislante. Por otro lado, se discuten los fenómenos relacionados a la optimización de las propiedades magnéticas de electrodos ferromagnéticos para la fabricación de junturas túnel Co_90Fe_10/MgO/Co_90Fe_10 y Co_90Fe_10/MgO /Fe_20Ni_80. En particular, se estudió el acople magnético entre capas ferromagnéticas y la inuencia del sustrato utilizado para el crecimiento de las tricapas. La optimización de los electrodos magnéticos involucró el análisis de la inuencia de la presencia de un aislante entre dos capas magnéticas en el acople de los electrodos. Se logró el desacople de films de 10 nm de Co_90Fe_10 y Fe_20Ni_80 separados por un espaciador de MgO de 2 nm. Finalmente se detallan los pasos para la fabricación de una red de junturas túnel magnéticas y su caracterización eléctrica a bajas temperaturas. El sistema estudiado fue la tricapa Co_90Fe_10 (10 nm)/M_gO (8 nm)/ Fe_20Ni_80 (10 nm) crecido sobre un sustrato de M_gO. La caracterización eléctrica confirmó la buena calidad de la junturas fabricadas. Las junturas obtenidas presentaron un comportamiento altamente resistivo (~ MΩ). Las mediciones de la corriente túnel en función de la temperatura permitieron descartar la presencia de pinholes en la barrera. El transporte de los portadores de carga es por efecto túnel a través de la barrera aislante. Las curvas de conductancia diferencial permitieron calcular el valor medio de la altura de la barrera de potencial (φ = 3.1 eV) a partir del modelo de Brinkman. Los resultados obtenidos en cada uno de los capítulos se complementan y son relevantes para la optimización de junturas túnel, debido a que brindan información crítica para su correcto funcionamiento. En la presente tesis se lograron obtener los primeros avances para la fabricación de arreglos de junturas túnel que permitan el desarrollo de dispositivos.

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In this thesis the low-temperature magnetism of the spin-ice systems Dy2Ti2O7 and Ho2Ti2O7 is investigated. In general, a clear experimental evidence for a sizable magnetic contribution kappa_{mag} to the low-temperature, zero-field heat transport of both spin-ice materials is observed. This kappa_{mag} can be attributed to the magnetic monopole excitations, which are highly mobile in zero field and are suppressed by a rather small external field resulting in a drop of kappa(H). Towards higher magnetic fields, significant field dependencies of the phononic heat conductivities kappa_{ph}(H) of Ho2Ti2O7 and Dy2Ti2O7 are found, which are, however, of opposite signs, as it is also found for the highly dilute reference materials (Ho0.5Y0.5)2Ti2O7 and (Dy0.5Y0.5)2Ti2O7. The dominant effect in the Ho-based materials is the scattering of phonons by spin flips which appears to be significantly stronger than in the Dy-based materials. Here, the thermal conductivity is suppressed due to enhanced lattice distortions observed in the magnetostriction. Furthermore, the thermal conductivity of Dy2Ti2O7 has been investigated concerning strong hysteresis effects and slow-relaxation processes towards equilibrium states in the low-temperature and low-field regime. The thermal conductivity in the hysteretic regions slowly relaxes towards larger values suggesting that there is an additional suppression of the heat transport by disorder in the non-equilibrium states. The equilibration can even be governed by the heat current for particular configurations. A special focus was put on the dilution series Dy2Ti2O7x. From specific heat measurements, it was found that the ultra-slow thermal equilibration in pure spin ice Dy2Ti2O7 is rapidly suppressed upon dilution with non-magnetic yttrium and vanishes completely for x>=0.2 down to the lowest accessible temperatures. In general, the low-temperature entropy of (Dy1-xYx)2Ti2O7, considerably decreases with increasing x, whereas its temperature-dependence drastically increases. Thus, it could be clarified that there is no experimental evidence for a finite zero-temperature entropy in (Dy1-xYx)2Ti2O7 above x>=0.2, in clear contrast to the finite residual entropy S_{P}(x) expected from a generalized Pauling approximation. A similar discrepancy is also present between S_{P}(x) and the low-temperature entropy obtained by Monte Carlo simulations, which reproduce the experimental data from 25 K down to 0.7 K, whereas the data at 0.4 K are overestimated. A straightforward description of the field-dependence kappa(H) of the dilution series with qualitative models justifies the extraction of kappa_{mag}. It was observed that kappa_{mag} systematically scales with the degree of dilution and its low-field decrease is related to the monopole excitation energy. The diffusion coefficient D_{mag} for the monopole excitations was calculated by means of c_{mag} and kappa_{mag}. It exhibits a broad maximum around 1.6 K and is suppressed for T<=0.5 K, indicating a non-degenerate ground state in the long-time limit, and in the high-temperature range for T>=4 K where spin-ice physics is eliminated. A mean-free path of 0.3 mum is obtained for Dy2Ti2O7 at about 1 K within the kinetic gas theory.

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In recent years, higher cadence, higher resolution observations have revealed the quiet-Sun photosphere to be complex and rapidly evolving. Since magnetic fields anchored in the photosphere extend up into the solar corona, it is expected that the small-scale coronal magnetic field exhibits similar complexity. For the first time, the quiet-Sun coronal magnetic field is continuously evolved through a series of non-potential, quasi-static equilibria, deduced from magnetograms observed by the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory, where the photospheric boundary condition which drives the coronal evolution exactly reproduces the observed magnetograms. The build-up, storage, and dissipation of magnetic energy within the simulations is studied. We find that the free magnetic energy built up and stored within the field is sufficient to explain small-scale, impulsive events such as nanoflares. On comparing with coronal images of the same region, the energy storage and dissipation visually reproduces many of the observed features. The results indicate that the complex small-scale magnetic evolution of a large number of magnetic features is a key element in explaining the nature of the solar corona.

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La presente tesis es un estudio dedicado a la optimización y desarrollo de sistemas del tipo juntura túnel. La metodología utilizada para la realización de la tesis consistió, en primer lugar, en la optimización de las componentes independientes de la juntura túnel: electrodo y barrera aislante. Posteriormente se optimizaron los procesos de fabricación para el desarrollo y caracterización de dispositivos del tipo juntura túnel en su forma final. En la primera parte de la tesis se analizan detalladamente los resultados obtenidos de la caracterización eléctrica y topografica de barreras aislantes en sistemas electrodo - barrera. Los sistemas bicapas estudiados, GdBa_2Cu_3_7/SrTiO_3, Nb/Ba_0,05Sr_0,95TiO_3 y YBa_2Cu_3O_7/SrTiO_3, fueron caracterizados utilizando un microscopio de fuerza atómica en modo conductor. Se propuso un modelo fenomenológico basado en los resultados experimentales, que permitió la obtención de parámetros críticos para el desarrollo de dispositivos del tipo juntura túnel con nuevas funcionalidades. La información obtenida de la caracterización de los sistemas bicapas (homogeneidad de crecimiento, baja densidad de defectos y de pinholes) indican un muy buen control de los parámetros de crecimiento de las barreras. Por otro lado, se obtuvo un buen comportamiento aislante para espesores mayores a 2 nm sin la presencia de pinholes en la barrera. La similitud en la estequiometría de las barreras (SrTiO_3) permitió comparar los distintos sistemas estudiados en términos de conductividad eléctrica. Se verificó que el modelo fenomenológico permite comparar la conductividad eléctrica de los sistemas mediante uno de los parámetros definidos en el modelo fenomenológico (obtenido de los ajustes lineales de las curvas I(V)). De los 3 sistemas estudiados, las bicapas GdBa_2Cu_3O_7/SrTiO_3 presentaron un mayor valor de longitud de atenuación de los portadores de carga a través de la barrera y una muy baja densidad de defectos superficiales. Las bicapas YBa_2Cu_3O_7/SrTiO_3 y Nb/Ba_0,05Sr_0,95TiO_3 permitieron validar el modelo fenomenológico propuesto para el análisis de la respuesta corriente - voltaje obtenida con el microscopio de fuerza atómica en modo conductor. La segunda parte de la tesis abarca conceptos de magnetismo y microfabricación para el desarrollo de junturas túnel magnéticas. Durante la caracterización de las películas ferromagnéticas individuales de Co_90Fe_10 (CoFe) se logró aumentar valor del campo coercitivo de films de 10 nm de espesor al incrementar la temperatura de depósito. Esto se debe a un aumento del tamaño de grano de los films. El aumento de la temperatura del sustrato durante el crecimiento influye en la morfología y las propiedades magnéticas de los films de CoFe favoreciendo la formación de granos y la pérdida del eje preferencial de magnetización. Estos resultados permitieron la fabricación de sistemas Co_90Fe_10/M_gO/Co_90Fe_10 con distintas orientaciones relativas accesibles con campo magnético para el estudio del acople magnético entre los films de CoFe. La caracterización eléctrica de estos sistemas, particularmente la respuesta corriente - voltaje obtenida con el microscopio de fuerza atómica en modo conductor, indicó que las propiedades de transporte eléctrico de las junturas presentan un alto grado de reproducibilidad. Se analizó además la inuencia del sustrato utilizado en la corriente túnel que atraviesa la barrera aislante. Por otro lado, se discuten los fenómenos relacionados a la optimización de las propiedades magnéticas de electrodos ferromagnéticos para la fabricación de junturas túnel Co_90Fe_10/MgO/Co_90Fe_10 y Co_90Fe_10/MgO /Fe_20Ni_80. En particular, se estudió el acople magnético entre capas ferromagnéticas y la inuencia del sustrato utilizado para el crecimiento de las tricapas. La optimización de los electrodos magnéticos involucró el análisis de la inuencia de la presencia de un aislante entre dos capas magnéticas en el acople de los electrodos. Se logró el desacople de films de 10 nm de Co_90Fe_10 y Fe_20Ni_80 separados por un espaciador de MgO de 2 nm. Finalmente se detallan los pasos para la fabricación de una red de junturas túnel magnéticas y su caracterización eléctrica a bajas temperaturas. El sistema estudiado fue la tricapa Co_90Fe_10 (10 nm)/M_gO (8 nm)/ Fe_20Ni_80 (10 nm) crecido sobre un sustrato de M_gO. La caracterización eléctrica confirmó la buena calidad de la junturas fabricadas. Las junturas obtenidas presentaron un comportamiento altamente resistivo (~ MΩ). Las mediciones de la corriente túnel en función de la temperatura permitieron descartar la presencia de pinholes en la barrera. El transporte de los portadores de carga es por efecto túnel a través de la barrera aislante. Las curvas de conductancia diferencial permitieron calcular el valor medio de la altura de la barrera de potencial (φ = 3.1 eV) a partir del modelo de Brinkman. Los resultados obtenidos en cada uno de los capítulos se complementan y son relevantes para la optimización de junturas túnel, debido a que brindan información crítica para su correcto funcionamiento. En la presente tesis se lograron obtener los primeros avances para la fabricación de arreglos de junturas túnel que permitan el desarrollo de dispositivos.