Estrutura espacial urbana e mobilidade: o caso da Região Metropolitana de São Paulo

A metrópole de São Paulo é a maior e mais importante aglomeração urbana do Brasil e está entre as dez maiores áreas urbanas do mundo. No entanto, a forma como acessibilidade espacial ocorre gera um fardo para a população e para a atividade econômica. Este trabalho pretende contribuir para a discussão de como melhorar a acessibilidade na Região Metropolitana de São Paulo estudando as características e impactos de estruturas espaciais urbana, analisando criticamente a estrutura espacial da metrópole e proporcionando sugestões de melhorias a fim de proporcionar uma mobilidade mais sustentável. Os procedimentos metodológicos incluem uma revisão bibliográfica sobre o tema e uma caracterização da estrutura espacial da Região Metropolitana de São Paulo, considerando a alocação de população, alocação de empregos e os padrões de deslocamento para os modais individual, coletivo e não motorizado. Apresentamos um relato da evolução recente, com dados das pesquisas de origem e destino realizadas pelo Metrô em 1997 e 2007 e da pesquisa de mobilidade de 2012. Também realizamos uma caracterização mais aprofundada com os dados da pesquisa de 2007. As cidades se desenvolvem com base no trade-off entre proximidade e mobilidade: a fim de maximizar as possibilidades de interação, as pessoas e as empresas tendem a se localizar onde o deslocamento necessário para executar essas interações requer menos custos financeiros, perda de tempo e desconforto. Esse processo molda a alocação espacial de atividades, que define parcialmente os hábitos de transporte. A estrutura espacial urbana pode ser caracterizada por sua escala (padrões compacto ou disperso), arranjo de densidades (padrão disperso ou clusterizado) e arranjo de atividade (padrão monocêntrico ou policêntrico). Estruturas espaciais com padrão mais compacto apresentam menores distâncias de viagem, reduzindo o impacto ambiental das viagens e viabilizando o transporte não motorizado e coletivo, e levam a um uso mais eficiente da terra, menor custo de infraestrutura e maior equidade no acesso ao transporte. Já estruturas clusterizadas policêntricas são associadas com maior facilidade de acesso à terra. Existe um debate sobre a capacidade de estruturas policêntricas resultarem em uma aproximação generalizada de empregos e residências. A Região Metropolitana de São Paulo apresenta um padrão monocêntrico na escala metropolitana, com fortes movimentos pendulares da periferia para o centro expandido da iii capital. Durante o período de análise, foi observada uma realocação da população para áreas mais centrais da cidade e uma centralização dos empregos ainda mais forte, resultando no agravamento dos movimentos pendulares. Existe uma clara divisão modal por renda: as classes mais altas utilizam majoritariamente automóveis, enquanto as classes mais baixas utilizam majoritariamente transporte coletivo e não motorizado. Para o futuro, o novo plano diretor tem o mérito de caminhar na direção do desenvolvimento urbano orientado pelo transporte sustentável, porém os níveis de densidade máxima permitidos ainda são parecidos com o do plano anterior e a largura dos eixos de adensamento é restrita. Acreditamos ser vantajoso um aumento do adensamento em áreas próximas dos empregos; geração de polos de adensamento em áreas mais afastadas dos empregos, mas próximas das infraestruturas de transporte coletivo de alta velocidade, e desencorajamento do adensamento em áreas com baixa acessibilidade. Também é necessária uma gestão integrada dos transportes, provendo infraestrutura para viagens não motorizadas e viagens intermodais, e uma gestão dos impactos negativos do adensamento.

Caught in the act: gas and stellar velocity dispersions in a fast Quenching compact star-forming galaxy at z ~ 1.7

We present Keck I MOSFIRE spectroscopy in the Y and H bands of GDN-8231, a massive, compact, star-forming galaxy at a redshift of z ~ 1.7. Its spectrum reveals both Hα and [Nii] emission lines and strong Balmer absorption lines. The Hα and Spitzer MIPS 24 μm fluxes are both weak, thus indicating a low star-formation rate of SFR≲5-10 M_⨀ yr−1. This, added to a relatively young age of ~700 Myr measured from the absorption lines, provides the first direct evidence for a distant galaxy being caught in the act of rapidly shutting down its star formation. Such quenching allows GDN-8231 to become a compact, quiescent galaxy, similar to three other galaxies in our sample, by z ~ 1.5. Moreover, the color profile of GDN-8231 shows a bluer center, consistent with the predictions of recent simulations for an early phase of inside-out quenching. Its line-of-sight velocity dispersion for the gas, σ_LOG^gas = 127 ± 32 km s^−1, is nearly 40% smaller than that of its stars, σ_LOG^* = 215 ± 35 km s^−1. High-resolution hydro-simulations of galaxies explain such apparently colder gas kinematics of up to a factor of ~1.5 with rotating disks being viewed at different inclinations and/or centrally concentrated star-forming regions. A clear prediction is that their compact, quiescent descendants preserve some remnant rotation from their star-forming progenitors.

CANDELS: The progenitors of compact quiescent galaxies at z ~ 2

We combine high-resolution Hubble Space Telescope/WFC3 images with multi-wavelength photometry to track the evolution of structure and activity of massive (M_*> 10^10 M_☉) galaxies at redshifts z = 1.4-3 in two fields of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey. We detect compact, star-forming galaxies (cSFGs) whose number densities, masses, sizes, and star formation rates (SFRs) qualify them as likely progenitors of compact, quiescent, massive galaxies (cQGs) at z = 1.5-3. At z≲2, cSFGs present SFR = 100-200 M_☉ yr^–1, yet their specific star formation rates (sSFR ~ 10^–9 yr^–1) are typically half that of other massive SFGs at the same epoch, and host X-ray luminous active galactic nuclei (AGNs) 30 times (~30%) more frequently. These properties suggest that cSFGs are formed by gas-rich processes (mergers or disk-instabilities) that induce a compact starburst and feed an AGN, which, in turn, quench the star formation on dynamical timescales (few 10^8 yr). The cSFGs are continuously being formed at z = 2-3 and fade to cQGs down to z ~ 1.5. After this epoch, cSFGs are rare, thereby truncating the formation of new cQGs. Meanwhile, down to z = 1, existing cQGs continue to enlarge to match local QGs in size, while less-gas-rich mergers and other secular mechanisms shepherd (larger) SFGs as later arrivals to the red sequence. In summary, we propose two evolutionary tracks of QG formation: an early (z≲2), formation path of rapidly quenched cSFGs fading into cQGs that later enlarge within the quiescent phase, and a late-arrival (z≳2) path in which larger SFGs form extended QGs without passing through a compact state.

Central compact objects and the hidden magnetic field scenario

Central compact objects (CCOs) are X-ray sources lying close to the centre of supernova remnants, with inferred values of the surface magnetic fields significantly lower (≲1011 G) than those of standard pulsars. In this paper, we revise the hidden magnetic field scenario, presenting the first 2D simulations of the submergence and re-emergence of the magnetic field in the crust of a neutron star. A post-supernova accretion stage of about 10−4–10−3 M⊙ over a vast region of the surface is required to bury the magnetic field into the inner crust. When accretion stops, the field re-emerges on a typical time-scale of 1–100 kyr, depending on the submergence conditions. After this stage, the surface magnetic field is restored close to its birth values. A possible observable consequence of the hidden magnetic field is the anisotropy of the surface temperature distribution, in agreement with observations of several of these sources. We conclude that the hidden magnetic field model is viable as an alternative to the antimagnetar scenario, and it could provide the missing link between CCOs and the other classes of isolated neutron stars.

Lipschitz compact operators

We introduce the notion of Lipschitz compact (weakly compact, finite-rank, approximable) operators from a pointed metric space X into a Banach space E. We prove that every strongly Lipschitz p-nuclear operator is Lipschitz compact and every strongly Lipschitz p-integral operator is Lipschitz weakly compact. A theory of Lipschitz compact (weakly compact, finite-rank) operators which closely parallels the theory for linear operators is developed. In terms of the Lipschitz transpose map of a Lipschitz operator, we state Lipschitz versions of Schauder type theorems on the (weak) compactness of the adjoint of a (weakly) compact linear operator.

A compact difference scheme for numerical solutions of second order dual-phase-lagging models of microscale heat transfer

Dual-phase-lagging (DPL) models constitute a family of non-Fourier models of heat conduction that allow for the presence of time lags in the heat flux and the temperature gradient. These lags may need to be considered when modeling microscale heat transfer, and thus DPL models have found application in the last years in a wide range of theoretical and technical heat transfer problems. Consequently, analytical solutions and methods for computing numerical approximations have been proposed for particular DPL models in different settings. In this work, a compact difference scheme for second order DPL models is developed, providing higher order precision than a previously proposed method. The scheme is shown to be unconditionally stable and convergent, and its accuracy is illustrated with numerical examples.

The case of the disappearing Fiscal Compact. CEPS Commentary, 5 November 2014

Following the Commission’s autumn forecast showing that only five euro-area countries exhibit a fiscal balance better than the 0.5% of GDP deficit allowed by the Fiscal Compact, Daniel Gros and Cinzia Alcidi attempt to explain in this new Commentary why there is precious little policy debate over these flagrant treaty violations. They find that it is not possible to put fiscal policy in a legal straightjacket and that the tight rules enshrined in the new Treaty and in national constitutions are discarded as soon as they become politically inconvenient.

The fiscal compact - Europe's "hard core" based on German economic conditions. OSW Commentary No. 71, 2012-03-07

On 2 March, the leaders of 25 EU member states signed the Treaty on stability, coordination and governance in the economic and monetary union. It will introduce new fiscal constraints and officially vest new competences in the eurozone countries. Thus, their right to coordinate economic policy among them will be sanctioned. So far, the Lisbon Treaty has only provided for organisation of informal Eurogroup meetings, to be attended by representatives of the European Commission. The principles introduced by the compact, if the eurozone countries are really determined to observe its provisions, will create a new way of managing the single currency. Within the next few years, the most indebted countries will have to carry out radical reforms to boost their competitiveness and adjust it to German standards. During this period the Federal Republic of Germany will most probably decide to offer higher loan guarantees to relieve these countries’ budgets. The compact’s political consequences are also of great significance, especially considering how the treaty was finalised. The eurozone states have in fact accepted that the direction for changes will be devised by France and Germany, and the role of European institutions such as the Commission or the Parliament may weaken. From the perspective of eurozone candidate countries, the introduction of the fiscal compact means expanding the scope of conditions they must meet to become members of the single currency area. In the future, a country, in order to adopt the single currency, will have to meet the structural deficit criterion, and also most probably carry out economic reforms such as unifying its fiscal system. These goals will be achieved across the eurozone gradually, in the subsequent stages of the economic governance reform.