Den svenska nedskärningsmodellen

Målet med detta examensarbete är att skapa en modell för svenska förhållanden,vilken kan användas för att minimera de negativa konsekvenserna avnedskärningar men även lyfta fram de positiva effekterna som en nedskärningmedför.Utifrån modellen Realistic Downsizing Preview (RDP) (Appelbaum & Donia,2001) har vi arbetat fram en egen modell över hur en nedskärningsprocess börutföras för att få ett så lyckat resultat som möjligt. Vi vill med vår modell främjade positiva effekterna utav nedskärningar och hur organisationen skall arbeta föratt uppnå dessa, på detta sätt bör de samtidigt kunna förebygga de negativaeffekterna.Vår studie är en kvalitativ litteraturundersökning där stort fokus har lagts påinsamlandet av artiklar och arbeten som behandlar ämnet Survivor Syndrome ochhur organisation bör arbeta med nedskärningar. Det insamlade materialet har sedananalyserats källkritiskt för att sedermera kunna bli en bidragen faktor vidskapandet av vår modell ”Den Svenska Nedskärningsmodellen”(SNM). Vi utfördetvå intervjuer, den ena var på SSAB och den andra var på NCC Construction.Detta gjordes efter modellen var klar för att kunna prova den praktiskt samt för attfå synpunkter. I vår modell kommer störst fokus att läggas på tre nyckelfaktorer,dessa är arbetet med utförarna, överlevarna och offren.Arbetet riktar sig till ledningen på större svenska organisationer som står inför ennedskärning.

Estrutura organizacional versus desempenho profissional. Estudo de caso de uma autarquia federal

During the 1980¿s and the 1990¿s, the Brazilian federal government started to set up a new public administration policy called ¿managerial¿ conceived of new patterns of efficiency and effectiveness and extremelly concerned about optimizing state administration to grant best results for people. This decision has been taken due to three main reasons; (i) the worst fiscal crisis considering the last decades; (ii) exhaustion on interfering with Brazilian economy due to its opening to globalization, and (iii) extremelly deep-rooted burocratic methods. The Brazilian state reform presented as a diagnosis of the human resource government area: (i) gradual raising costs in payroll, allied to (ii) huge raising inefficiency in public services, and (iii) civil servants are unprepared to improve better responses to currents citizen demands and to adopt new methods of management based on the best professional performance and the best quality of public services. We have concluded that the federal government often tries to make civil servants redundant instead of adopting a real policy of management that would give them better conditions to improve their performance. This paper presents a concrete proposal to improve quality in civil servants performance by taking advantage of information technology and of our assumed country¿s democratization. We suggest that the Brazilian state reform must be and should be a new path of social growth and development not only in economic basis.

Sistema de controle: evidências da contribuição do sistema para a minimização de fraudes nas organizações

As organizações estão se conscientizando que a mudança decorrente da transição de estruturas tradicionais para funcionais, da implementação de estruturas, assim como da união de culturas organizacionais, está repleta de riscos. Esta mudança vem em decorrência de downsizing, fusões, incorporações, cisões, joint ventures, entre outras alternativas administrativas, societárias e comerciais praticadas. Com a necessidade de adaptar rapidamente o negócio às exigências externas, os riscos, muitas vezes, não são analisados ou o são superficial ou parcialmente, resultando na elevação dos mesmos e expondo os processos de negócios a potenciais fraudes. O ambiente de controle do negócio tem se mostrado uma área de preocupação, principalmente nos momentos de transição estrutural e organizacional, pelo desconhecimento conceitual do risco e da importância do controle, como também pela forma de implementação das mudanças. Verifica-se também que há empresas, normalmente as grandes, que possuem um sistema estruturado de controles implementado e outras, normalmente as médias e pequenas, que não o possuem, onde, de acordo com pesquisas realizadas, encontra-se um maior número de fraudes, que, proporcionalmente ao seu patrimônio, representa uma perda substancial aos seus negócios. Este estudo objetiva abordar a evidência de contribuição de um sistema estruturado de controle para a minimização de ocorrência de fraudes nas organizações.

From public to private : the performance of former public workers in the Brazilian labor market

This paper analyzes the placement in the private sector of a subset of Brazilian public-sector employees. This group left public employment in the mid-1990’s through a voluntary severance program. This paper contrasts their earnings before and after quitting the public sector, and compares both sets of wages to public and private sector earnings for similar workers. We find that participants in this voluntary severance program suffered a significant reduction in average earnings wage and an increase in earnings dispersion. We test whether the reduction in average earnings and the increase in earnings dispersion is the expected outcome once one controls for observed characteristics, by means of counterfactual simulations. Several methods of controlling for observed characteristics (parametric and non-parametrically) are used for robustness. The results indicate that this group of workers was paid at levels below what would be expected given their embodied observable characteristics.

Foreign investment in Mexico after economic reform

Includes bibliography

Employment, growth and reforms in Jamaica

Includes bibliography

Modelo de gerenciamento integrado de resíduos sólidos urbanos: uma contribuição ao planejamento urbano

Pós-graduação em Geociências e Meio Ambiente - IGCE

Perfil do adoecimento dos trabalhadores de câmpus universitário do interior paulista: análise dos dados de absenteísmo por motivo de doença

Pós-graduação em Saúde Coletiva - FMB

O recurso e o razoável

Pós-graduação em Direito - FCHS

Dimensionamento de pessoal de enfermagem na atenção básica em uma região de saúde

Pós-graduação em Enfermagem - FMB

CC98-410 Money 2000+ News (Introductory Issue)

Money 2000+ is a program designed to increase the financial well being of Nebraskans through increased savings and reduced household debt. This Campaign Circular, Money 2000+ News is an introductory publication to this program which talks about setting goals for saving money, downsizing your debt with ways to save with credit cards, passing up things that waste money, record keeping, looking for ways to save money, avoiding late fees, and saving and credit tips.

The VIMOS-VLT Deep Survey: the evolution of type-1 AGN

Quasars and AGN play an important role in many aspects of the modern cosmology. Of particular interest is the issue of the interplay between AGN activity and formation and evolution of galaxies and structures. Studies on nearby galaxies revealed that most (and possibly all) galaxy nuclei contain a super-massive black hole (SMBH) and that between a third and half of them are showing some evidence of activity (Kormendy and Richstone, 1995). The discovery of a tight relation between black holes mass and velocity dispersion of their host galaxy suggests that the evolution of the growth of SMBH and their host galaxy are linked together. In this context, studying the evolution of AGN, through the luminosity function (LF), is fundamental to constrain the theories of galaxy and SMBH formation and evolution. Recently, many theories have been developed to describe physical processes possibly responsible of a common formation scenario for galaxies and their central black hole (Volonteri et al., 2003; Springel et al., 2005a; Vittorini et al., 2005; Hopkins et al., 2006a) and an increasing number of observations in different bands are focused on collecting larger and larger quasar samples. Many issues remain however not yet fully understood. In the context of the VVDS (VIMOS-VLT Deep Survey), we collected and studied an unbiased sample of spectroscopically selected faint type-1 AGN with a unique and straightforward selection function. Indeed, the VVDS is a large, purely magnitude limited spectroscopic survey of faint objects, free of any morphological and/or color preselection. We studied the statistical properties of this sample and its evolution up to redshift z 4. Because of the contamination of the AGN light by their host galaxies at the faint magnitudes explored by our sample, we observed that a significant fraction of AGN in our sample would be missed by the UV excess and morphological criteria usually adopted for the pre-selection of optical QSO candidates. If not properly taken into account, this failure in selecting particular sub-classes of AGN could, in principle, affect some of the conclusions drawn from samples of AGN based on these selection criteria. The absence of any pre-selection in the VVDS leads us to have a very complete sample of AGN, including also objects with unusual colors and continuum shape. The VVDS AGN sample shows in fact redder colors than those expected by comparing it, for example, with the color track derived from the SDSS composite spectrum. In particular, the faintest objects have on average redder colors than the brightest ones. This can be attributed to both a large fraction of dust-reddened objects and a significant contamination from the host galaxy. We have tested these possibilities by examining the global spectral energy distribution of each object using, in addition to the U, B, V, R and I-band magnitudes, also the UV-Galex and the IR-Spitzer bands, and fitting it with a combination of AGN and galaxy emission, allowing also for the possibility of extinction of the AGN flux. We found that for 44% of our objects the contamination from the host galaxy is not negligible and this fraction decreases to 21% if we restrict the analysis to a bright subsample (M1450 <-22.15). Our estimated integral surface density at IAB < 24.0 is 500 AGN per square degree, which represents the highest surface density of a spectroscopically confirmed sample of optically selected AGN. We derived the luminosity function in B-band for 1.0 < z < 3.6 using the 1/Vmax estimator. Our data, more than one magnitude fainter than previous optical surveys, allow us to constrain the faint part of the luminosity function up to high redshift. A comparison of our data with the 2dF sample at low redshift (1 < z < 2.1) shows that the VDDS data can not be well fitted with the pure luminosity evolution (PLE) models derived by previous optically selected samples. Qualitatively, this appears to be due to the fact that our data suggest the presence of an excess of faint objects at low redshift (1.0 < z < 1.5) with respect to these models. By combining our faint VVDS sample with the large sample of bright AGN extracted from the SDSS DR3 (Richards et al., 2006b) and testing a number of different evolutionary models, we find that the model which better represents the combined luminosity functions, over a wide range of redshift and luminosity, is a luminosity dependent density evolution (LDDE) model, similar to those derived from the major Xsurveys. Such a parameterization allows the redshift of the AGN density peak to change as a function of luminosity, thus fitting the excess of faint AGN that we find at 1.0 < z < 1.5. On the basis of this model we find, for the first time from the analysis of optically selected samples, that the peak of the AGN space density shifts significantly towards lower redshift going to lower luminosity objects. The position of this peak moves from z 2.0 for MB <-26.0 to z 0.65 for -22< MB <-20. This result, already found in a number of X-ray selected samples of AGN, is consistent with a scenario of “AGN cosmic downsizing”, in which the density of more luminous AGN, possibly associated to more massive black holes, peaks earlier in the history of the Universe (i.e. at higher redshift), than that of low luminosity ones, which reaches its maximum later (i.e. at lower redshift). This behavior has since long been claimed to be present in elliptical galaxies and it is not easy to reproduce it in the hierarchical cosmogonic scenario, where more massive Dark Matter Halos (DMH) form on average later by merging of less massive halos.

Study of silicon-on-insulator multiple-gate MOS structures including band-gap engineering and self heating effects

The progresses of electron devices integration have proceeded for more than 40 years following the well–known Moore’s law, which states that the transistors density on chip doubles every 24 months. This trend has been possible due to the downsizing of the MOSFET dimensions (scaling); however, new issues and new challenges are arising, and the conventional ”bulk” architecture is becoming inadequate in order to face them. In order to overcome the limitations related to conventional structures, the researchers community is preparing different solutions, that need to be assessed. Possible solutions currently under scrutiny are represented by: • devices incorporating materials with properties different from those of silicon, for the channel and the source/drain regions; • new architectures as Silicon–On–Insulator (SOI) transistors: the body thickness of Ultra-Thin-Body SOI devices is a new design parameter, and it permits to keep under control Short–Channel–Effects without adopting high doping level in the channel. Among the solutions proposed in order to overcome the difficulties related to scaling, we can highlight heterojunctions at the channel edge, obtained by adopting for the source/drain regions materials with band–gap different from that of the channel material. This solution allows to increase the injection velocity of the particles travelling from the source into the channel, and therefore increase the performance of the transistor in terms of provided drain current. The first part of this thesis work addresses the use of heterojunctions in SOI transistors: chapter 3 outlines the basics of the heterojunctions theory and the adoption of such approach in older technologies as the heterojunction–bipolar–transistors; moreover the modifications introduced in the Monte Carlo code in order to simulate conduction band discontinuities are described, and the simulations performed on unidimensional simplified structures in order to validate them as well. Chapter 4 presents the results obtained from the Monte Carlo simulations performed on double–gate SOI transistors featuring conduction band offsets between the source and drain regions and the channel. In particular, attention has been focused on the drain current and to internal quantities as inversion charge, potential energy and carrier velocities. Both graded and abrupt discontinuities have been considered. The scaling of devices dimensions and the adoption of innovative architectures have consequences on the power dissipation as well. In SOI technologies the channel is thermally insulated from the underlying substrate by a SiO2 buried–oxide layer; this SiO2 layer features a thermal conductivity that is two orders of magnitude lower than the silicon one, and it impedes the dissipation of the heat generated in the active region. Moreover, the thermal conductivity of thin semiconductor films is much lower than that of silicon bulk, due to phonon confinement and boundary scattering. All these aspects cause severe self–heating effects, that detrimentally impact the carrier mobility and therefore the saturation drive current for high–performance transistors; as a consequence, thermal device design is becoming a fundamental part of integrated circuit engineering. The second part of this thesis discusses the problem of self–heating in SOI transistors. Chapter 5 describes the causes of heat generation and dissipation in SOI devices, and it provides a brief overview on the methods that have been proposed in order to model these phenomena. In order to understand how this problem impacts the performance of different SOI architectures, three–dimensional electro–thermal simulations have been applied to the analysis of SHE in planar single and double–gate SOI transistors as well as FinFET, featuring the same isothermal electrical characteristics. In chapter 6 the same simulation approach is extensively employed to study the impact of SHE on the performance of a FinFET representative of the high–performance transistor of the 45 nm technology node. Its effects on the ON–current, the maximum temperatures reached inside the device and the thermal resistance associated to the device itself, as well as the dependence of SHE on the main geometrical parameters have been analyzed. Furthermore, the consequences on self–heating of technological solutions such as raised S/D extensions regions or reduction of fin height are explored as well. Finally, conclusions are drawn in chapter 7.

Development of a new galaxy classification technique and its application to the zCOSMOS survey

The purpose of this Thesis is to develop a robust and powerful method to classify galaxies from large surveys, in order to establish and confirm the connections between the principal observational parameters of the galaxies (spectral features, colours, morphological indices), and help unveil the evolution of these parameters from $z \sim 1$ to the local Universe. Within the framework of zCOSMOS-bright survey, and making use of its large database of objects ($\sim 10\,000$ galaxies in the redshift range $0 < z \lesssim 1.2$) and its great reliability in redshift and spectral properties determinations, first we adopt and extend the \emph{classification cube method}, as developed by Mignoli et al. (2009), to exploit the bimodal properties of galaxies (spectral, photometric and morphologic) separately, and then combining together these three subclassifications. We use this classification method as a test for a newly devised statistical classification, based on Principal Component Analysis and Unsupervised Fuzzy Partition clustering method (PCA+UFP), which is able to define the galaxy population exploiting their natural global bimodality, considering simultaneously up to 8 different properties. The PCA+UFP analysis is a very powerful and robust tool to probe the nature and the evolution of galaxies in a survey. It allows to define with less uncertainties the classification of galaxies, adding the flexibility to be adapted to different parameters: being a fuzzy classification it avoids the problems due to a hard classification, such as the classification cube presented in the first part of the article. The PCA+UFP method can be easily applied to different datasets: it does not rely on the nature of the data and for this reason it can be successfully employed with others observables (magnitudes, colours) or derived properties (masses, luminosities, SFRs, etc.). The agreement between the two classification cluster definitions is very high. ``Early'' and ``late'' type galaxies are well defined by the spectral, photometric and morphological properties, both considering them in a separate way and then combining the classifications (classification cube) and treating them as a whole (PCA+UFP cluster analysis). Differences arise in the definition of outliers: the classification cube is much more sensitive to single measurement errors or misclassifications in one property than the PCA+UFP cluster analysis, in which errors are ``averaged out'' during the process. This method allowed us to behold the \emph{downsizing} effect taking place in the PC spaces: the migration between the blue cloud towards the red clump happens at higher redshifts for galaxies of larger mass. The determination of $M_{\mathrm{cross}}$ the transition mass is in significant agreement with others values in literature.

Sviluppo e validazione sperimentale di strategie di previsione e controllo del fenomeno della preaccensione (Mega-Knock)

L’algoritmo per la previsione del Mega-Knock si inserisce all’interno di uno dei temi cardine dell’attuale ricerca nel campo motoristico: la minimizzazione del consumo di combustibile nei motori ad alto grado di sovralimentazione, sviluppati nell’ottica del downsizing. La possibilità di prevedere l’innescarsi del Mega-Knock consente di ottimizzare la definizione dell’obiettivo di titolo, evitando arricchimenti non necessari in un range di funzionamento del motore che frequentemente viene esplorato nella normale guida su strada. Si tratterà la possibilità di utilizzare una relazione empirica per cercare di arrivare alla previsione dell’insorgere della preaccensione, per poi ricorrere ad opportune strategie motore per evitare il verificarsi del fenomeno; il tutto tramite lo sviluppo di un algoritmo in ambiente MatLab-Simulink