76 research outputs found
Estrutura dos halos de matéria escura no modelo ΛCDM
No full textCaracterizamos estatisticamente a estrutura dos halos de matéria escura extraídos da Simulação do Millennium, uma das maiores simulações do modelo cosmológico CDM realizadas até hoje, com 10 bilhões de partículas num volume de 500h−1Mpc3. Nossos resultados confirmam que na época atual, z = 0, o parâmetro de concentração dos halos se correlaciona com a massa. Esta correlação é ajustada por uma lei de potência no intervalo de massas que corresponde a halos de galáxias (1012h−1M) até aglomerados de galáxias (1015h−1M), log10 c ∞ −α log10M, com α = 0.1. Comparamos a previsão de três modelos existentes na literatura para esta correlação. Medimos a distribuição de probilidade do parâmetro de concentração, que é ajustada com boa aproximação por uma função lognormal com dispersão σlog10 c = 0.1 em todo o intervalo de massas. Verificamos que o parâmetro de concentração é independente do spin do halo quando sistemas claramente fora de equilíbrio são removidos da análise. Comparamos modelos que relacionam o parÂmetro de concentração com histórico de formação extraído da simulação. Mostramos que quando definimos a época de formação levando em conta a distribuição de progenitores do halo e não apenas o progenitor mais massivo, obtemos uma correlação melhor entre densidade média do universo nessa época e a densidade característica do halo. Finalmente, testamos a validade de dois modelos que predizem o parâmetro de concentração a z = 0 com base no histórico de acreção de massa do progenitor mais massivo do halo.We use the Millennium Simulation (MS) to study the statistics of CDM halo concentrations at z = 0. Our results confirm that the average halo concentration declines monotonically with mass; the concentration-mass relation is well fit by a power-law over 3 decades in mass, up to the most massive objects that form in a CDM universe (~1015h−1M). We compare this relation with three models in the literature. The large volume surveyed, together with the unprecedented numerical resolution of the MS, allow us to estimate with confidence the distribution of concentrations and, consequently, the abundance of systems with unusual properties. We find that halo concentrations are independent of spin once haloes manifestly out of equilibrium have been removed from the sample. The concentrations of out-ofequilibrium haloes tend to be lower and have more scatter, while their spins tend to be higher. A number of previously noted trends within the halo population are induced primarily by these properties of unrelaxed systems. Finally, we compare the result of predicting halo concentrations using the mass assembly history of the main progenitor with predictions based on simple arguments regarding the assembly time of all progenitors. The latter are typically as good or better than the former, suggesting that halo concentration depends not only on the evolutionary path of a halo’s main progenitor, but on how and when all of its constituents collapsed to form non-linear objects
Dinâmica de satélites da Via-Láctea
No full textNesta dissertação apresentamos o trabalho desenvolvido com a finalidade de estudar alguns aspectos da dinâmica de satélites da Via-Láctea. Discutimos a montagem do computador paralelo CPADA onde realizamos as simulações além da implementação do código GADGET e dos programas auxiliares desenvolvidos para viabilizar nossos estudos sobre interações gravitacionais de N-corpos. Do ponto de vista astrofísico estudamos 3 problemas diferentes: a. Modelamos a órbita do aglomerado globular M92 comparando as estruturas de maré observadas a distâncias de até 3 raios de maré do centro do aglomerado. Concluímos que as velocidades espaciais conhecidas e o modelo usado para o halo da Via Láctea permitem, através das simulacões reproduzir bastante bem estas estruturas e predizer a localização das caudas de maré que se extenderiam a grandes distâncias à frente e atrás do aglomerado. b. A possibilidade de que o par de aglomerados abertos NGC1907 e NGC1912, espacialmente próximos formem um par físico. Demonstramos que as velocidades espaciais observadas não são compatíveis com a possibilidade de eles estarem gravitacionalmente ligados e que a sua aproximação espacial é um fato casual. c. A possibilidade de captura de aglomerados globulares da Via Láctea pela Grande Nuvem de Magalhães. Demonstramos que sob as condições iniciais do nosso modelo o número de capturas é menor que 15, o número de aglomerados velhos existentes na LMC. O que nos permite concluir que a presença desses aglomerados é devida ao processo de formação estelar nessa galáxia.In this work we present the tasks developed in order to study some aspects about the dynamics of Milky Way satellites. We discuss the assembly of the cluster CPADA and the implementation of the GADGET code, as well as the auxiliary softwares developed in order to carry out our studies in the gravitational N-body field. From the astrophysical point oí view we studied three problems: a. We modeled the orbit oí the globular cluster M92 in order to compare the tidally produced structures, observed up to 3 tidal radii of the cluster center. We concluded that the known spatial velocities and our model of the Milky Way allows to fiducially reproduce this structures and predict the orientation of the tidal tails, which extend themselves backwards and frontwards along the cluster orbit, for large distances from the cluster center. b. The possible physical association oí the pair of open clusters NGC1907 and NGC1912, which presently are spatially close to each other. We demonstrated that their observed spatial velocities are not compatible with the hypothesis of the cluster being gravitationally bounded, and that their present spatial approximation is an accidental facto c. The possibility oí Milky Way globular clusters capture by the Large Magellanic Cloud. We demonstrated that under the initial constrains oí our model the captures number is smaller than 15, the number of old clusters belonging to the LMC. We conclude that the presence of these clusters in the LMC is due to the stellar formation process in this galaxy
The Observable Field for Antennas in Reception
No full textIn this paper, the portion of the incident field that can be received by an antenna is investigated: the observable field. This field can be estimated relying only on the volume allocated to the antenna and thus independently of the specific antenna geometry. The observable field is composed by a single spherical wave that first converges into the origin and then diverges to infinity. The power associated with the converging wave is the power available to an antenna located within the defined volume. Previously, an estimation of this observable spherical wave was obtained by truncating the spectral spherical modal series representation of the incident field. Here, instead, we provide more applicable approximation of the observable field, by truncating a spatial integral representation of the incident field that is based on the use of equivalent ideal currents. Eventually, for the vast majority of antennas, the estimation of the available power that can be obtained by approximating the observable field via the ideal currents is more accurate than the estimation that would be obtained via the spectral modal expansion. Moreover, analytical expressions for the observable field are provided here. The ideas are set here considering the case of single plane wave incidence, but the extension to multiple plane waves is straightforward.Accepted Author ManuscriptTera-Hertz Sensin
Fourier Optics for the Analysis of Distributed Absorbers Under THz Focusing Systems
No full textAn analytical spectral model able to accurately and efficiently characterize absorbers distributed in the focal plane of focusing THz systems is presented. The model is obtained by using a Fourier optics representation of the electromagnetic field in the focal plane in conjunction with a recently developed equivalent network representation for the interaction of plane waves with distributed absorbers. The model is validated by comparisons with numerical full-wave simulations. Finally, the model is used to design a few architectures based on lens-coupled Kinetic Inductance Detectors (KIDs), which show high absorption efficiency over alarge bandwidth.Accepted Author ManuscriptTera-Hertz Sensin
Time-Domain Modelling of Pulsed Photoconducting Sources - Part I: The Norton Equivalent Circuit
No full textIn the circuit theory, the Norton and Thevenin equivalent generators are tools that simplify the solutions of networks involving passive or active components. They have been extensively used in the frequency domain to describe time-harmonic sources. A time-stepped evolution is instead typically used to include transient sources. As a particular case of the latter, the Norton equivalent circuit is extended here to investigate pulsed photoconducting sources, where a dc bias voltage and a pulsed optical laser are combined to generate terahertz (THz) bursts. The proposed derivation relies on the application of the electromagnetic (EM) equivalence theorem. The main conclusion of this derivation is the understanding that, from the three different spectral regions (dc, THz, and optics), only the THz radiation is to be explicitly included in the equivalent circuit. The theory is validated by a campaign of measurements reported in a connected paper. </p
Coherent Fourier Optics Model for the Synthesis of Large Format Lens Based Focal Plane Arrays
No full textFuture sub millimeter imagers are being developed with large focal plane arrays (FPAs) of lenses to increase the field of view (FoV) and the imaging speed. A full-wave electromagnetic analysis of such arrays is numerically cumbersome and time-consuming. This article presents a spectral technique based on Fourier optics combined with geometrical optics for analyzing, in reception, lens-based FPAs with wide FoVs. The technique provides a numerically efficient methodology to derive the plane wave spectrum (PWS) of a secondary quasi-optical component. This PWS is used to calculate the power received by an antenna or absorber placed at the focal region of a lens. The method is applied to maximize the scanning performance of imagers with monolithically integrated lens feeds without employing an optimization algorithm. The derived PWS can be directly used to define the lens and feed properties. The synthesized FPA achieved scan losses much lower than the ones predicted by standard formulas for horn-based FPAs. In particular, an FPA with scan loss below 1 dB while scanning up to ±17.5° (±44 beam-widths) is presented with directivity of 52 dBi complying with the needs for future sub millimeter imagers. The technique is validated via a physical optics code with excellent agreement.Accepted Author ManuscriptTera-Hertz Sensin
Reception Power Pattern of Distributed Absorbers in Focal Plane Arrays: A Fourier Optics Analysis
No full textPassive imaging cameras at millimeter and submillimeter wavelengths are currently entering a new era with the development of large format arrays of direct detectors. Several of these arrays are being developed with bare absorbing meshes without any antenna coupling (lens or horn) structures. The design of such arrays is typically done resorting to geometrical considerations or basic broadside plane wave incidence analysis. This paper presents a spectral technique for the analysis of such focal plane arrays in reception using Fourier Optics, which is valid also for moderately skewed incident angles. The analysis constitutes a step improvement with respect to previously used methods by providing an accurate and efficient way to estimate the point-source angular response and the throughput from a distributed incoherent source of an absorbing mesh in the focal plane of a quasi-optical component (e.g. a parabolic reflector or lens). The proposed technique is validated with full-wave simulations. After presenting the analysis, the paper compares the performance of arrays of bare absorber in the focal plane of a quasi-optical component to those of corresponding antenna based arrays. It is found that absorbers lead to a comparable trade-off, in terms of spill-over and focusing efficiency, only for very tight samplings. For larger samplings, the focusing efficiency of absorbers is significantly lower than the one for antennas.Accepted Author ManuscriptTera-Hertz Sensin
A Benchmark for the Number of Independent Line of Sight Links on a Given Volume Platform
No full textThe number of independent links that can be hosted by an antenna platform for Line-of-Sight (LoS) communications is limited by its physical size and the interference between the beams associated with different users. For large-size platforms, the interference can be reduced by compromising the aperture efficiency, and this trade-off is the metric to quantify the effective use of the platform. This metric fails for antenna platforms that are not electrically large, for which the aperture efficiency is no longer a useful parameter. Here we resort to the concept of the Observable Field, related to the maximum theoretical directivity, to estimate the potential number of independent links supported by moderate-size platforms. This allows the introduction of coupling coefficients between the beams associated with the observable portion of the incident field and the beams associated with the receiving antennas. These coefficients are bounded to unity for any platform dimension, unlike the aperture efficiency, and they are maximized when the antenna pattern is equal to the pattern predicted by the Observable Field. Accordingly, selecting beams dictated by the Observable Field constitutes a benchmark for the effective use of the volume. Any antenna design can be compared to this benchmark to assess its merits.Green Open Access added to TU Delft Institutional Repository 'You share, we take care!' - Taverne project https://www.openaccess.nl/en/you-share-we-take-care Otherwise as indicated in the copyright section: the publisher is the copyright holder of this work and the author uses the Dutch legislation to make this work public.Tera-Hertz Sensin
- …
