924 resultados para Relativistic many-body perturbation theory
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Compared to μ→eγ and μ→eee, the process μ→e conversion in nuclei receives enhanced contributions from Higgs-induced lepton flavor violation. Upcoming μ→e conversion experiments with drastically increased sensitivity will be able to put extremely stringent bounds on Higgs-mediated μ→e transitions. We point out that the theoretical uncertainties associated with these Higgs effects, encoded in the couplings of quark scalar operators to the nucleon, can be accurately assessed using our recently developed approach based on SU(2) chiral perturbation theory that cleanly separates two- and three-flavor observables. We emphasize that with input from lattice QCD for the coupling to strangeness fNs, hadronic uncertainties are appreciably reduced compared to the traditional approach where fNs is determined from the pion-nucleon σ term by means of an SU(3) relation. We illustrate this point by considering Higgs-mediated lepton flavor violation in the standard model supplemented with higher-dimensional operators, the two-Higgs-doublet model with generic Yukawa couplings, and the minimal supersymmetric standard model. Furthermore, we compare bounds from present and future μ→e conversion and μ→eγ experiments.
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We show how to avoid unnecessary and uncontrolled assumptions usually made in the literature about soft SU(3) flavor symmetry breaking in determining the two-flavor nucleon matrix elements relevant for direct detection of weakly interacting massive particles (WIMPs). Based on SU(2) chiral perturbation theory, we provide expressions for the proton and neutron scalar couplings fp,nu and fp,nd with the pion-nucleon σ term as the only free parameter, which should be used in the analysis of direct detection experiments. This approach for the first time allows for an accurate assessment of hadronic uncertainties in spin-independent WIMP-nucleon scattering and for a reliable calculation of isospin-violating effects. We find that the traditional determinations of Vfpu−fnu and fpd−fnd are off by a factor of 2.
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Once seen as anomalous, facilitative interactions among plants and their importance for community structure and functioning are now widely recognized. The growing body of modelling, descriptive and experimental studies on facilitation covers a wide variety of terrestrial and aquatic systems throughout the globe. However, the lack of a general body of theory linking facilitation among different types of organisms and biomes and their responses to environmental changes prevents further advances in our knowledge regarding the evolutionary and ecological implications of facilitation in plant communities. Moreover, insights gathered from alternative lines of inquiry may substantially improve our understanding of facilitation, but these have been largely neglected thus far. Despite over 15 years of research and debate on this topic, there is no consensus on the degree to which plant–plant interactions change predictably along environmental gradients (i.e. the stress-gradient hypothesis), and this hinders our ability to predict how plant–plant interactions may affect the response of plant communities to ongoing global environmental change. The existing controversies regarding the response of plant–plant interactions across environmental gradients can be reconciled when clearly considering and determining the species-specificity of the response, the functional or individual stress type, and the scale of interest (pairwise interactions or community-level response). Here, we introduce a theoretical framework to do this, supported by multiple lines of empirical evidence. We also discuss current gaps in our knowledge regarding how plant–plant interactions change along environmental gradients. These include the existence of thresholds in the amount of species-specific stress that a benefactor can alleviate, the linearity or non-linearity of the response of pairwise interactions across distance from the ecological optimum of the beneficiary, and the need to explore further how frequent interactions among multiple species are and how they change across different environments. We review the latest advances in these topics and provide new approaches to fill current gaps in our knowledge. We also apply our theoretical framework to advance our knowledge on the evolutionary aspects of plant facilitation, and the relative importance of facilitation, in comparison with other ecological processes, for maintaining ecosystem structure, functioning and dynamics. We build links between these topics and related fields, such as ecological restoration, woody encroachment, invasion ecology, ecological modelling and biodiversity–ecosystem-functioning relationships. By identifying commonalities and insights from alternative lines of research, we further advance our understanding of facilitation and provide testable hypotheses regarding the role of (positive) biotic interactions in the maintenance of biodiversity and the response of ecological communities to ongoing environmental changes.
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Using explicitly-correlated coupled-cluster theory with single and double excitations, the intermolecular distances and interaction energies of the T-shaped imidazole⋯⋯benzene and pyrrole⋯⋯benzene complexes have been computed in a large augmented correlation-consistent quadruple-zeta basis set, adding also corrections for connected triple excitations and remaining basis-set-superposition errors. The results of these computations are used to assess other methods such as Møller–Plesset perturbation theory (MP2), spin-component-scaled MP2 theory, dispersion-weighted MP2 theory, interference-corrected explicitly-correlated MP2 theory, dispersion-corrected double-hybrid density-functional theory (DFT), DFT-based symmetry-adapted perturbation theory, the random-phase approximation, explicitly-correlated ring-coupled-cluster-doubles theory, and double-hybrid DFT with a correlation energy computed in the random-phase approximation.
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Meindl et al. (Adv Space Res 51(7):1047–1064, 2013) showed that the geocenter z -component estimated from observations of global navigation satellite systems (GNSS) is strongly correlated to a particular parameter of the solar radiation pressure (SRP) model developed by Beutler et al. (Manuscr Geod 19:367–386, 1994). They analyzed the forces caused by SRP and the impact on the satellites’ orbits. The authors achieved their results using perturbation theory and celestial mechanics. Rebischung et al. (J Geod doi:10.1016/j.asr.2012.10.026, 2013) also deal with the geocenter determination with GNSS. The authors carried out a collinearity diagnosis of the associated parameter estimation problem. They conclude “without much exaggerating that current GNSS are insensitive to any component of geocenter motion”. They explain this inability by the high degree of collinearity of the geocenter coordinates mainly with satellite clock corrections. Based on these results and additional experiments, they state that the conclusions drawn by Meindl et al. (Adv Space Res 51(7):1047–1064, 2013) are questionable. We do not agree with these conclusions and present our arguments in this article. In the first part, we review and highlight the main characteristics of the studies performed by Meindl et al. (Adv Space Res 51(7):1047–1064, 2013) to show that the experiments are quite different from those performed by Rebischung et al. (J Geod doi:10.1016/j.asr.2012.10.026,2013) . In the second part, we show that normal equation (NEQ) systems are regular when estimating geocenter coordinates, implying that the covariance matrices associated with the NEQ systems may be used to assess the sensitivity to geocenter coordinates in a standard way. The sensitivity of GNSS to the components of the geocenter is discussed. Finally, we comment on the arguments raised by Rebischung et al. (J Geod doi:10.1016/j.asr.2012.10.026, 2013) against the results of Meindl et al. (Adv Space Res 51(7):1047–1064, 2013).
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We calculate the all-loop anomalous dimensions of current operators in λ-deformed σ-models. For the isotropic integrable deformation and for a semi-simple group G we compute the anomalous dimensions using two different methods. In the first we use the all-loop effective action and in the second we employ perturbation theory along with the Callan–Symanzik equation and in conjunction with a duality-type symmetry shared by these models. Furthermore, using CFT techniques we compute the all-loop anomalous dimension of bilinear currents for the isotropic deformation case and a general G . Finally we work out the anomalous dimension matrix for the cases of anisotropic SU(2) and the two couplings, corresponding to the symmetric coset G/H and a subgroup H, splitting of a group G.
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The difficulties of applying the Hartree-Fock method to many body problems is illustrated by treating Helium's electrons up to the point where tractability vanishes. Second, the problem of applying Hartree-Fock methods to the helium atom's electrons, when they are constrained to remain on a sphere, is revisited. The 6-dimensional total energy operator is reduced to a 2-dimensional one, and the application of that 2-dimensional operator in the Hartree-Fock mode is discussed.
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We study a model of nonequilibrium quantum transport of particles and energy in a many-body system connected to mesoscopic Fermi reservoirs (the so-called meso-reservoirs). We discuss the conservation laws of particles and energy within our setup as well as the transport properties of quasi-periodic and disordered chains.
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From a vibrationally corrected 3D potential energy surface determined with highly correlated ab initio calculations (CCSD(T)), the lowest vibrational energies of two dimethyl-ether isotopologues, 12CH3–16O–12CD3 (DME-d3) and 12CD3–16O–12CD3 (DME-d6), are computed variationally. The levels that can be populated at very low temperatures correspond to the COC-bending and the two methyl torsional modes. Molecular symmetry groups are used for the classification of levels and torsional splittings. DME-d6 belongs to the G36 group, as the most abundant isotopologue 12CH3–16O–12CH3 (DME-h6), while DME-d3 is a G18 species. Previous assignments of experimental Raman and far-infrared spectra are discussed from an effective Hamiltonian obtained after refining the ab initio parameters. Because a good agreement between calculated and experimental transition frequencies is reached, new assignments are proposed for various combination bands corresponding to the two deuterated isotopologues and for the 020 → 030 transition of DME-d6. Vibrationally corrected potential energy barriers, structural parameters, and anharmonic spectroscopic parameters are provided. For the 3N – 9 neglected vibrational modes, harmonic and anharmonic fundamental frequencies are obtained using second-order perturbation theory by means of CCSD and MP2 force fields. Fermi resonances between the COC-bending and the torsional modes modify DME-d3 intensities and the band positions of the torsional overtones.
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A linear method is developed for solving the nonlinear differential equations of a lumped-parameter thermal model of a spacecraft moving in a closed orbit. This method, based on perturbation theory, is compared with heuristic linearizations of the same equations. The essential feature of the linear approach is that it provides a decomposition in thermal modes, like the decomposition of mechanical vibrations in normal modes. The stationary periodic solution of the linear equations can be alternately expressed as an explicit integral or as a Fourier series. This method is applied to a minimal thermal model of a satellite with ten isothermal parts (nodes), and the method is compared with direct numerical integration of the nonlinear equations. The computational complexity of this method is briefly studied for general thermal models of orbiting spacecraft, and it is concluded that it is certainly useful for reduced models and conceptual design but it can also be more efficient than the direct integration of the equations for large models. The results of the Fourier series computations for the ten-node satellite model show that the periodic solution at the second perturbative order is sufficiently accurate.
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A new method to study large scale neural networks is presented in this paper. The basis is the use of Feynman- like diagrams. These diagrams allow the analysis of collective and cooperative phenomena with a similar methodology to the employed in the Many Body Problem. The proposed method is applied to a very simple structure composed by an string of neurons with interaction among them. It is shown that a new behavior appears at the end of the row. This behavior is different to the initial dynamics of a single cell. When a feedback is present, as in the case of the hippocampus, this situation becomes more complex with a whole set of new frequencies, different from the proper frequencies of the individual neurons. Application to an optical neural network is reported.
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Multigroup diffusion codes for three dimensional LWR core analysis use as input data pre-generated homogenized few group cross sections and discontinuity factors for certain combinations of state variables, such as temperatures or densities. The simplest way of compiling those data are tabulated libraries, where a grid covering the domain of state variables is defined and the homogenized cross sections are computed at the grid points. Then, during the core calculation, an interpolation algorithm is used to compute the cross sections from the table values. Since interpolation errors depend on the distance between the grid points, a determined refinement of the mesh is required to reach a target accuracy, which could lead to large data storage volume and a large number of lattice transport calculations. In this paper, a simple and effective procedure to optimize the distribution of grid points for tabulated libraries is presented. Optimality is considered in the sense of building a non-uniform point distribution with the minimum number of grid points for each state variable satisfying a given target accuracy in k-effective. The procedure consists of determining the sensitivity coefficients of k-effective to cross sections using perturbation theory; and estimating the interpolation errors committed with different mesh steps for each state variable. These results allow evaluating the influence of interpolation errors of each cross section on k-effective for any combination of state variables, and estimating the optimal distance between grid points.
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In this paper, an analytical solution of the main problem, a satellite only perturbed by the J2 harmonic, is derived with the aid of perturbation theory and by using DROMO variables. The solution, which is valid for circular and elliptic orbits with generic eccentricity and inclination, describes the instantaneous time variation of all orbital elements, that is, the actual values of the osculating elements
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El principal objetivo de la tesis es estudiar el acoplamiento entre los subsistemas de control de actitud y de control térmico de un pequeño satélite, con el fin de buscar la solución a los problemas relacionados con la determinación de los parámetros de diseño. Se considera la evolución de la actitud y de las temperaturas del satélite bajo la influencia de dos estrategias de orientación diferentes: 1) estabilización magnética pasiva de la orientación (PMAS, passive magnetic attitude stabilization), y 2) control de actitud magnético activo (AMAC, active magnetic attitude control). En primer lugar se presenta el modelo matemático del problema, que incluye la dinámica rotacional y el modelo térmico. En el problema térmico se considera un satélite cúbico modelizado por medio de siete nodos (seis externos y uno interno) aplicando la ecuación del balance térmico. Una vez establecido el modelo matemático del problema, se estudia la evolución que corresponde a las dos estrategias mencionadas. La estrategia PMAS se ha seleccionado por su simplicidad, fiabilidad, bajo coste, ahorrando consumo de potencia, masa coste y complejidad, comparado con otras estrategias. Se ha considerado otra estrategia de control que consigue que el satélite gire a una velocidad requerida alrededor de un eje deseado de giro, pudiendo controlar su dirección en un sistema inercial de referencia, ya que frecuentemente el subsistema térmico establece requisitos de giro alrededor de un eje del satélite orientado en una dirección perpendicular a la radiación solar incidente. En relación con el problema térmico, para estudiar la influencia de la velocidad de giro en la evolución de las temperaturas en diversos puntos del satélite, se ha empleado un modelo térmico linealizado, obtenido a partir de la formulación no lineal aplicando un método de perturbaciones. El resultado del estudio muestra que el tiempo de estabilización de la temperatura y la influencia de las cargas periódicas externas disminuye cuando aumenta la velocidad de giro. Los cambios de temperatura se reducen hasta ser muy pequeños para velocidades de rotación altas. En relación con la estrategia PMAC se ha observado que a pesar de su uso extendido entre los micro y nano satélites todavía presenta problemas que resolver. Estos problemas están relacionados con el dimensionamiento de los parámetros del sistema y la predicción del funcionamiento en órbita. Los problemas aparecen debido a la dificultad en la determinación de las características magnéticas de los cuerpos ferromagnéticos (varillas de histéresis) que se utilizan como amortiguadores de oscilaciones en los satélites. Para estudiar este problema se presenta un modelo analítico que permite estimar la eficiencia del amortiguamiento, y que se ha aplicado al estudio del comportamiento en vuelo de varios satélites, y que se ha empleado para comparar los resultados del modelo con los obtenidos en vuelo, observándose que el modelo permite explicar satisfactoriamente el comportamiento registrado. ABSTRACT The main objective of this thesis is to study the coupling between the attitude control and thermal control subsystems of a small satellite, and address the solution to some existing issues concerning the determination of their parameters. Through the thesis the attitude and temperature evolution of the satellite is studied under the influence of two independent attitude stabilization and control strategies: (1) passive magnetic attitude stabilization (PMAS), and (2) active magnetic attitude control (AMAC). In this regard the mathematical model of the problem is explained and presented. The mathematical model includes both the rotational dynamics and the thermal model. The thermal model is derived for a cubic satellite by solving the heat balance equation for 6 external and 1 internal nodes. Once established the mathematical model of the problem, the above mentioned attitude strategies were applied to the system and the temperature evolution of the 7 nodes of the satellite was studied. The PMAS technique has been selected to be studied due to its prevalent use, simplicity, reliability, and cost, as this strategy significantly saves the overall power, weight, cost, and reduces the complexity of the system compared to other attitude control strategies. In addition to that, another control law that provides the satellite with a desired spin rate along a desired axis of the satellite, whose direction can be controlled with respect to the inertial reference frame is considered, as the thermal subsystem of a satellite usually demands a spin requirement around an axis of the satellite which is positioned perpendicular to the direction of the coming solar radiation. Concerning the thermal problem, to study the influence of spin rate on temperature evolution of the satellite a linear approach of the thermal model is used, which is based on perturbation theory applied to the nonlinear differential equations of the thermal model of a spacecraft moving in a closed orbit. The results of this study showed that the temperature stabilization time and the periodic influence of the external thermal loads decreases by increasing the spin rate. However, the changes become insignificant for higher values of spin rate. Concerning the PMAS strategy, it was observed that in spite of its extended application to micro and nano satellites, still there are some issues to be solved regarding this strategy. These issues are related to the sizing of its system parameters and predicting the in-orbit performance. The problems were found to be rooted in the difficulties that exist in determining the magnetic characteristics of the ferromagnetic bodies (hysteresis rods) that are applied as damping devices on-board satellites. To address these issues an analytic model for estimating their damping efficiency is proposed and applied to several existing satellites in order to compare the results with their respective in-flight data. This model can explain the behavior showed by these satellites.
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Esta tesis doctoral busca estudiar el espacio desde la premisa de que el espacio es, fundamentalmente, lo intermedio. El entre, lo que hay entre las cosas mismas y que les da, precisamente, su definición como cosas en un constante proceso de delimitación. Este entre, lo que hay entre las cosas, no es sin embargo un resto que queda, sino bien al contrario el principio activo que hace que las cosas, desde lo que hay alrededor, se configuren en su ser sensible y puedan percibirse. El entre, lo intermedio, no es así una línea, un corte puro, sino un intervalo, un espacio en sí mismo, un ámbito en que se desarrolla un proceso. Es por tanto un espacio de formación, en el que las cosas aún no son y ya están siendo, un intervalo ambiguo pleno de virtualidades, unas desplegadas otras que permanecen en espera, siempre en movimiento. Es la hipótesis principal de esta tesis que en el llamado Movimiento Moderno en la arquitectura del siglo veinte esta condición ambigua del límite se pone de manifiesto como la raíz articuladora de los cambios espaciales y formales que definen su ser y su estética. Para desarrollar esta hipótesis, se parte de una doble premisa: por una parte, como un entre que es en sí misma, la arquitectura se encuentra delimitada por las disciplinas artísticas contemporáneas, especialmente pintura y escultura y a la vez las delimita. Por tanto, se explorarán una serie de momentos claves en las vanguardias de comienzos del siglo veinte en paralelo a una serie de arquitecturas contemporáneas para estudiar esta doble dialéctica entre límites. Por otra parte, y entendiendo que lo propio de la arquitectura es el espacio, se estudiarán en profundidad las concepciones espaciales que en la física y la estética del finales del siglo diecinueve y principios del veinte se desarrollan, para comprender cómo estas nuevas concepciones, centradas en las ideas de relatividad y de espacio-tiempo como magnitudes interlimitadas, determinan a su vez las concepciones espaciales que se desarrollan simultáneamente en las artes plásticas y en la arquitectura. La tríada espacio/tiempo/luz regirá este recorrido, en un doble camino: a través de la física y la teoría del arte, y a través de la arquitectura y las artes plásticas. Se trata por tanto de incardinar la arquitectura en su contexto artístico y científico, y comprobar cómo la comprensión del espacio como un entre, como un intervalo del límite y no como un absoluto trascendente, se generaliza en dichos ámbitos en una exploración paralela que condiciona los resultados en todos ellos y que define, por tanto, la arquitectura de la modernidad como una arquitectura del entre. El encuadre enmarca como motivo principal el Movimiento Moderno a través de la figura de Le Corbusier. Se muestra el modo en que los recursos y mecanismos empleados provocan el encuentro del espacio indecible a través de la polifonía de las artes. Desde el espaciamiento del límite, su borradura, su ambigüedad, producidos mediante el entrelazamiento de los recursos artísticos, la continuidad de lo lineal, el encabalgamiento, el maridaje, la ambivalencia, la relatividad del color y la luz, el intersticio. Ello se analiza a través de la obra de le Corbusier, destacando la dialéctica entre Le Cheminée y Nature morte aux nombreux objets; Ma maison y el pabellón del Zurichhorn; Unité y L’espace indicible. Aclaradas las premisas fundamentales y las consecuencias inmediatas para la arquitectura del Movimiento Moderno, la cuarta parte y final de la tesis, mucho más breve que las anteriores, expone una primera aproximación a las consecuencias que todo esto ha tenido en un momento liminal también: el comienzo de la postmodernidad. En realidad se trata de una apertura a lo que ha de venir, pues establecida la operatividad de la hipóteisi inicial, se trata aquí solamente de abrir el camino a una interpretación que en realidad escapa del alcance de esta tesis. Así se deja apuntado cómo, a través de la obra de tres arquitectos, teóricos y artistas trabajando en los años setenta y comienzos de los ochenta del pasado siglo, una comprensión más clara de la revolución moderna precipitada por esta nueva comprensión del espacio como límite-entre queda patente. Chamberworks de Daniel Libeskind, Wexner Center for the Visual Arts de Peter Eisenman y Manhattan Transcripts de Bernard Tschumi servirían de privilegiados ejemplo. Como queda patente que las consecuencias de todo ello aún las estamos sintiendo en nuestra contemporaneidad. ABSTRACT This thesis aims to study the space from the premise that space is mainly the in-between. The in-between, what is in-between the things themselves and gives them precisely its definition as things in a constant process of delimitation. This in-between, what is in between things, is not a remnant that remains, but on the contrary it is the active ingredient that produces things from what is around, that configures them in a sensitive to be perceived. The in-between, the intermediate, is not a line, a pure cut, but an interval, a space in itself, an area in which a process is developed. It is therefore a space in development, where things are still not and already been, delimiting an ambiguous range full of potentialities, some present and others that remain only as virtualities. It is the main hypothesis of this thesis that in the so-called Modern Movement in the architecture of the twentieth century this ambiguous boundary condition is revealed as the result of the articulatation of spatial and formal changes. To develop this hypothesis, I posit this double premise: On the one hand, as an in-between which is in itself, architecture is defined by contemporary artistic disciplines, especially painting and sculpture and simultaneously defines them. Therefore, a number of key moments in the avantgarde of the early twentieth century in parallel with a number of contemporary architecture to study this double dialectic between boundaries will be explored. On the other hand, and considering that the “essence” of the architecture is space, I will study in depth the spatial concepts in physics and aesthetics of late-nineteenth century and early twentieth century to understand how these new concepts centered on the ideas of relativity and space-time as interlimited magnitudes in turn determine the spatial conceptions that take place simultaneously in the visual arts and architecture. The space / time / light triad governs this journey in a double way: through physics and theory of art, and through architecture and the arts. The aim is to anchor architecture in its artistic and scientific context, and to see how the understanding of space as an in-between interval and not as an absolute transcendent determines the results in all of them, defining, therefore, the architecture of modernity as an architecture of the in-between. The frame of the study is centered in the modern movement through the figure of Le Corbusier and how rthe different resources and mechanisms employed provoke an unspeakable space of encounter through the polyphony of the arts. From the spacing of the limit, its erasure, its ambiguity, produced by the intertwining of artistic resources to continuity of the linear, the marriage, the ambivalence, the relativity of color and light, the gap. All this is analyzed through the work of Le Corbusier, highlighting the dialectic between Le Cheminée and Nature morte aux nombreux objets, Ma maison and Zürichhorn pavilion, Unité and L’espace indicible. Once the basic premises and immediate consequences for the architecture of the Modern Movement are set, the fourth and final part of the thesis aims to explore the impact that all this has had in another liminal time: the beginning of postmodernism. Of course, this part is shorter, in fact it is more a prospective survey and an opening of possibilities than a truly articulated body of theory, since the conceptual core of this thesis has been developed in the central part. Hence, through the work of three architects, theorists and artists working in the seventies and early eighties of last century, a clearer understanding of the modern revolution precipitated by this new understanding of space as a boundary- between is proposed. Chamberworks by Daniel Libeskind, Wexner Center for the Visual Arts by Peter Eisenman and Manhattan Transcripts by Bernard Tschumi will exemplify this approach. The consequences of all this are still haunting our contemporaneity.