Processing optimized for symmetry in the problem of evasive maneuvers

The increasing number of space debris in operating regions around the earth constitutes a real threat to space missions. The goal of the research is to establish appropriate scientific-technological conditions to prevent the destruction and/or impracticability of spacecraft in imminent collision in these regions. A definitive solution to this problem has not yet been reached with the degree of precision that the dynamics of spatial objects (vehicle and debris) requires mainly due to the fact that collisions occur in chains and fragmentation of these objects in the space environment. This fact threatens the space missions on time and with no prospects for a solution in the near future. We present an optimization process in finding the initial conditions (CIC) to collisions, considering the symmetry of the distributions of maximum relative positions between spatial objects with respect to the spherical angles. For this, we used the equations of the dynamics on the Clohessy-Witshire, representing a limit of validation that is highly computationally costly. We simulate different maximum relative positions values of the corresponding initial conditions given in terms of spherical angles. Our results showed that there are symmetries that significantly reduce operating costs, such that the search of the CIC is advantageously carried out up to 4 times the initial processing routine. Knowledge of CIC allows the propulsion system operating vehicle implement evasive maneuvers before impending collisions with space debris.

Plasma Steroid Dynamics in Late- and Near-term Naturally and Artificially Conceived Bovine Pregnancies as Elucidated by Multihormone High-resolution LC-MS/MS

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Evolutionary optimization applied for fine-tuning parameter estimation in optical flow-based environments

Optical flow methods are accurate algorithms for estimating the displacement and velocity fields of objects in a wide variety of applications, being their performance dependent on the configuration of a set of parameters. Since there is a lack of research that aims to automatically tune such parameters, in this work we have proposed an evolutionary-based framework for such task, thus introducing three techniques for such purpose: Particle Swarm Optimization, Harmony Search and Social-Spider Optimization. The proposed framework has been compared against with the well-known Large Displacement Optical Flow approach, obtaining the best results in three out eight image sequences provided by a public dataset. Additionally, the proposed framework can be used with any other optimization technique.

Polychlorinated biphenyls and organochlorine pesticides in plastics ingested by seabirds

The occurrence of plastic objects in the digestive tract was assessed in eight species of Procellariiformes collected in southern Brazil and the occurrence of polychlorinated biphenyls (PCBs) and organochlorine pesticides (OCPs) in the ingested plastics pellets and plastic fragments was evaluated. PCBs were detected in plastic pellets (491 ng g(-1)) and plastic fragments (243-418 ng g(-1)). Among the OCPs, p,p`-DDE had the highest concentrations, ranging from 68.0 to 99.0 ng g(-1). The occurrence of organic pollutants in post-consumer plastics supports the fact that plastics are an important source carrying persistent organic pollutants in the marine environment. Although transfer through the food chain may be the main source of exposure to POPs to seabirds, plastics could be an additional source for the organisms which ingest them, like Procellariiformes which are the seabirds most affected by plastic pollution. (c) 2010 Elsevier Ltd. All rights reserved.

Ontogeny of manipulative behavior and nut-cracking in young tufted capuchin monkeys (Cebus apella): a Perception-action perspective

How do capuchin monkeys learn to use stones to crack open nuts? Perception-action theory posits that individuals explore producing varying spatial and force relations among objects and surfaces, thereby learning about affordances of such relations and how to produce them. Such learning supports the discovery of tool use. We present longitudinal developmental data from semifree-ranging tufted capuchin monkeys (Cebus apella) to evaluate predictions arising from Perception-action theory linking manipulative development and the onset of tool-using. Percussive actions bringing an object into contact with a surface appeared within the first year of life. Most infants readily struck nuts and other objects against stones or other surfaces from 6 months of age, but percussive actions alone were not sufficient to produce nut-cracking sequences. Placing the nut on the anvil surface and then releasing it, so that it could be struck with a stone, was the last element necessary for nut-cracking to appear in capuchins. Young chimpanzees may face a different challenge in learning to crack nuts: they readily place objects on surfaces and release them, but rarely vigorously strike objects against surfaces or other objects. Thus the challenges facing the two species in developing the same behavior (nut-cracking using a stone hammer and an anvil) may be quite different. Capuchins must inhibit a strong bias to hold nuts so that they can release them; chimpanzees must generate a percussive action rather than a gentle placing action. Generating the right actions may be as challenging as achieving the right sequence of actions in both species. Our analysis suggests a new direction for studies of social influence on young primates learning sequences of actions involving manipulation of objects in relation to surfaces.

The peculiar isolated neutron star in the Carina Nebula Deep XMM-Newton and ESO-VLT observations of 2XMM J104608.7-594306

While fewer in number than the dominant rotation-powered radio pulsar population, peculiar classes of isolated neutron stars (INSs) which include magnetars, the ROSAT-discovered "Magnificent Seven" (M7), rotating radio transients (RRATs), and central compact objects in supernova remnants (CCOs) - represent a key element in understanding the neutron star phenomenology. We report the results of an observational campaign to study the properties of the source 2XMM J104608.7-594306, a newly discovered thermally emitting INS. The evolutionary state of the neutron star is investigated by means of deep dedicated observations obtained with the XMM-Newton Observatory, the ESO Very Large Telescope, as well as publicly available gamma-ray data from the Fermi Space Telescope and the AGILE Mission. The observations confirm previous expectations and reveal a unique type of object. The source, which is likely within the Carina Nebula (N-H = 2.6x10(21) cm(-2)), has a spectrum that is both thermal and soft, with kT(infinity) = 135 eV. Non-thermal (magnetospheric) emission is not detected down to 1% (3 sigma, 0.1-12 keV) of the source luminosity. Significant deviations (absorption features) from a simple blackbody model are identified in the spectrum of the source around energies 0.6 keV and 1.35 keV. While the former deviation is likely related to a local oxygen overabundance in the Carina Nebula, the latter can only be accounted for by an additional spectral component, which is modelled as a Gaussian line in absorption with EW = 91 eV and sigma = 0.14 keV (1 sigma). Furthermore, the optical counterpart is fainter than m(V) = 27 (2 sigma) and no gamma-ray emission is significantly detected by either the Fermi or AGILE missions. Very interestingly, while these characteristics are remarkably similar to those of the M7 or the only RRAT so far detected in X-rays, which all have spin periods of a few seconds, we found intriguing evidence of very rapid rotation, P = 18.6ms, at the 4 sigma confidence level. We interpret these new results in the light of the observed properties of the currently known neutron star population, in particular those of standard rotation-powered pulsars, recycled objects, and CCOs. We find that none of these scenarios can satisfactorily explain the collective properties of 2XMM J104608.7-594306, although it may be related to the still poorly known class of Galactic anti-magnetars. Future XMM-Newton data, granted for the next cycle of observations (AO11), will help us to improve our current observational interpretation of the source, enabling us to significantly constrain the rate of pulsar spin down.

Star formation in H I tails: HCG 92, HCG 100 and six interacting systems

We present new Gemini spectra of 14 new objects found within the H?i tails of Hickson Compact Groups (HCGs) 92 and 100. Nine of them are Galaxy Evolution Explorer (GALEX) far-ultraviolet (FUV) and near-ultraviolet (NUV) sources. The spectra confirm that these objects are members of the compact groups and have metallicities close to solar, with an average value of 12+log(O/H) similar to 8.5. They have average FUV luminosities 7 x 10(40)?erg?s-1 and very young ages (<100?Myr), and two of them resemble tidal dwarf galaxy (TDG) candidates. We suggest that they were created within gas clouds that were ejected during galaxygalaxy interactions into the intergalactic medium, which would explain the high metallicities of the objects, inherited from the parent galaxies from which the gas originated. We conduct a search for similar objects in six interacting systems with extended H?i tails: NGC 2623, NGC 3079, NGC 3359, NGC 3627, NGC 3718 and NGC 4656. We found 35 ultraviolet (UV) sources with ages < 100?Myr; however, most of them are on average less luminous/massive than the UV sources found around HCG 92 and HCG 100. We speculate that this might be an environmental effect and that compact groups of galaxies are more favourable to TDG formation than other interacting systems.

The nature of extremely red galaxies in the local universe

We investigate the nature of extremely red galaxies (ERGs), objects whose colours are redder than those found in the red sequence present in colour–magnitude diagrams of galaxies. We selected from the Sloan Digital Sky Survey Data Release 7 a volume-limited sample of such galaxies in the redshift interval 0.010 < z < 0.030, brighter than Mr = −17.8 (magnitudes dereddened, corrected for the Milky Way extinction) and with (g − r) colours larger than those of galaxies in the red sequence. This sample contains 416 ERGs, which were classified visually. Our classification was cross-checked with other classifications available in the literature. We found from our visual classification that the majority of objects in our sample are edge-on spirals (73 per cent). Other spirals correspond to 13 per cent, whereas elliptical galaxies comprise only 11 per cent of the objects. After comparing the morphological mix and the distributions of Hα/Hβ and axial ratios of ERGs and objects in the red sequence, we suggest that dust, more than stellar population effects, is the driver of the red colours found in these extremely red galaxies.

Stellar Models in General Relativity

Neutron stars are some of the most fascinating objects in Nature. Essentially all aspects of physics seems to be represented inside them. Their cores are likely to contain deconfined quarks, hyperons and other exotic phases of matter in which the strong interaction is the dominant force. The inner region of their solid crust is penetrated by superfluid neutrons and their magnetic fields may reach well over 1012 Gauss. Moreover, their extreme mean densities, well above the densities of nuclei, and their rapid rotation rates makes them truly relativistic both in the special as well as in the general sense. This thesis deals with a small subset of these phenomena. In particular the exciting possibility of trapping of gravita-tional waves is examined from a theoretical point of view. It is shown that the standard condition R < 3M is not essential to the trapping mechanism. This point is illustrated using the elegant tool provided by the optical geometry. It is also shown that a realistic equation of state proposed in the literature allows stable neutron star models with closed circular null orbits, something which is closely related to trapped gravitational waves. Furthermore, the general relativistic theory of elasticity is reviewed and applied to stellar models. Both static equilibrium as well as radially oscillating configurations with elasticsources are examined. Finally, Killing tensors are considered and their applicability to modeling of stars is discussed

Mica fish in mylonites

Mögliche Verformungsmechanismen, die zu den verschiedenen Glimmer- und Mineralfischen führen, sind: intrakristalline Verformung, Kristallrotation, Biegung und Faltung, Drucklösung in Kombination mit Ausfällung und dynamische Rekristallisation oder Mechanismen, die ein großes Mineral in mehrere kleine, fischförmige Kristalle aufspalten.Experimente mit ein neues Verformungsgerät und Objekten in zwei verschiedenen Matrixmaterialien werden beschrieben. Das eine ist PDMS, (Newtonianisch viskoses Polymer), und das andere Tapioca Perlen (Mohr-Couloumb Verhalten). Die Rotation von fischförmigen Objekten in PDMS stimmt mit der theoretischen Rotationsrate für ellipsenförmige Objekte in einem Newtonianischen Material überein. In einer Matrix von Tapioca Perlen nehmen die Objekte eine stabile Lage ein. Diese Orientierung ist vergleichbar mit der von Glimmerfischen. Die Verformung in der Matrix von Tapioca Perlen ist konzentriert auf dünne Scherzonen. Diese Ergebnisse implizieren, daß die Verformung in natürlichen Gesteinen auch in dünnen Scherzonen konzentriert ist.Computersimulationen werden beschrieben, mit denen der Einfluß der Eigenschaften einer Matrix auf die Rotation von Objekten und Verteilung von Deformation untersucht wird.Mit diesen Experimenten wird gezeigt, daß die Orientierung von Glimmerfischen nicht mit Verformung in einem nicht-linearen viskosen Material erklärt werden kann. Eine solche nicht-lineare Rheologie wird im Allgemeinen für die Erdkurste angenommen. Die stabile Orientierung eines Objektes kann mit weicheren Lagen in der Matrix erklärt werden.

Servizi di posizionamento e potenzialità degli atti di aggiornamento cartografico in coordinate assolute ETRF2000

Il contesto nazionale è cambiato recentemente per l’introduzione del nuovo Sistema Geodetico coincidente con quello Europeo (ETRS89, frame ETRF00) e realizzato dalle stazioni della Rete Dinamica Nazionale. Sistema geodetico, associato al cartografico UTM_ETRF00, divenuto per decreto obbligatorio nelle Pubbliche Amministrazioni. Questo cambiamento ha consentito di ottenere rilevamenti dei dati cartografici in coordinate assolute ETRF00 molto più accurate. Quando i dati così rilevati vengono utilizzati per aggiornamenti cartografici perdono le coordinate originarie e vengono adattati a particolari cartografici circostanti. Per progettare una modernizzazione delle mappe catastali e delle carte tecniche finalizzata a consentire l’introduzione degli aggiornamenti senza modificarne le coordinate assolute originarie, lo studio è iniziato valutando come utilizzare sviluppi di strutturazione dei dati topografici presenti nel Database Geotopografico, modellizzazioni 3D di fabbricati nelle esperienze catastali INSPIRE, integrazioni in ambito MUDE tra progetti edilizi e loro realizzazioni. Lo studio è proseguito valutando i servizi di posizionamento in tempo reale NRTK presenti in Italia. Inoltre sono state effettuate sperimentazioni per verificare anche in sede locale la precisione e l’affidabilità dei servizi di posizionamento presenti. La criticità della cartografia catastale deriva sostanzialmente dal due fatti: che originariamente fu inquadrata in 850 Sistemi e successivamente fu trasformata in Roma40 con una esigua densità di punti rimisurati; che fino al 1988 fu aggiornata con modalità non rigorose di bassa qualità. Per risolvere tali criticità si è quindi ipotizzato di sfruttare le modalità di rilevamento NRTK per aumentare localmente la densità dei punti rimisurati e reinquadrare le mappe catastali. Il test, realizzato a Bologna, ha comportato un’analisi preliminare per individuare quali Punti Fiduciali considerare coerenti con le specifiche cartografiche per poi utilizzarli e aumentare localmente la densità dei punti rimisurati. La sperimentazione ha consentito la realizzazione del progetto e di inserire quindi i prossimi aggiornamenti senza modificarne le coordinate ETRF00 ottenute dal servizio di posizionamento.

Plasticity in body and peripersonal space representations

A successful interaction with objects in the environment requires integrating information concerning object-location with the shape, dimension and position of body parts in space. The former information is coded in a multisensory representation of the space around the body, i.e. peripersonal space (PPS), whereas the latter is enabled by an online, constantly updated, action-orientated multisensory representation of the body (BR) that is critical for action. One of the critical features of these representations is that both PPS and BR are not fixed, but they dynamically change depending on different types of experience. In a series of experiment, I studied plastic properties of PPS and BR in humans. I have developed a series of methods to measure the boundaries of PPS representation (Chapter 4), to study its neural correlates (Chapter 3) and to assess BRs. These tasks have been used to study changes in PPS and BR following tool-use (Chapter 5), multisensory stimulation (Chapter 6), amputation and prosthesis implantation (Chapter 7) or social interaction (Chapter 8). I found that changes in the function (tool-use) and the structure (amputation and prosthesis implantation) of the physical body elongate or shrink both PPS and BR. Social context and social interaction also shape PPS representation. Such high degree of plasticity suggests that our sense of body in space is not given at once, but it is constantly constructed and adapted through experience.

I manufatti egizi ed egittizzanti in Sicilia

Il progetto di ricerca si è posto l'obiettivo di analizzare una serie di manufatti egizî e di tradizione egizia della Sicilia preromana e di evidenziare le eventuali sopravvivenze della cultura egittizzante sull’isola fino all'età tardoantica. La realizzazione di un corpus, aggiornato sulla scorta di nuovi rinvenimenti, di recenti riletture e di studi su materiali inediti custoditi nei musei siciliani, ha contribuito a tracciare una mappa distributiva delle aree di rinvenimento e di attestazione, con particolare riferimento alle diverse etnie che recepiscono tali prodotti e alla possibilità di ricostruire l’ambientazione storica della domanda diretta o indiretta. Si è scelto di privilegiare lo studio tipologico, iconografico e iconologico di alcune “categorie” di materiali maggiormente documentati sull’isola, quali amuleti, scarabei e scaraboidi, cretule, ushabti, gioielli, bronzi figurati, gemme, con l’individuazione di riscontri in ambito mediterraneo. La documentazione delle testimonianze antiquarie contenenti notizie su reperti oggi non più reperibili ha permesso, infine, non solo l’acquisizione d’informazioni spesso ritenute perse, ma anche una comprensione storicizzata delle dinamiche del collezionismo siciliano e del suo ruolo nel più vasto ambito europeo dal XVII al XIX secolo. È stato importante, infatti, chiarire anche alcuni aspetti della cultura egittologica del periodo, legata in genere alla circolazione di stereotipi e alla mancanza di una conoscenza diretta della realtà faraonica.

Attualità del divieto assoluto di procreazione medicalmente assistita eterologa in Italia e prospettive di superamento

La presente ricerca si fonda su un’attenta ed approfondita analisi della normativa vigente in Italia in materia di procreazione medicalmente assistita (P.M.A.), con particolare riferimento al divieto assoluto di P.M.A. eterologa, di cui all’art. 4, comma 3, L. 19 febbraio 2004, n. 40, consentita invece – sia pure con la previsione di limitazioni differenti – nella quasi totalità dei paesi europei. Dopo aver esaminato la “questione etica” del ricorso alle tecniche di fecondazione assistita e le normative vigenti in Europa in materia di P.M.A. eterologa, il presente lavoro analizza i profili civilistici della L. n. 40/2004 ed i conseguenti dubbi interpretativi che la normativa italiana pone in materia di fecondazione eterologa, con specifico riguardo al consenso prestato dai coniugi o conviventi, al divieto di disconoscimento di paternità e di anonimato della madre ed, infine, al diritto del nato da fecondazione eterologa di conoscere le proprie origini biologiche. Ne consegue che, in una materia che coinvolge la sfera più intima e personale della vita privata e familiare, quale quella della P.M.A., il legislatore avrebbe dovuto intervenire con misura, individuando soluzioni ragionevoli ed equilibrate nel rispetto della pluralità di etiche contrapposte ed interessi in conflitto. Attraverso una capillare analisi della recente giurisprudenza nazionale ed europea, la presente ricerca mira, dunque, a valutare possibili prospettive di superamento del divieto assoluto di P.M.A. eterologa previsto dalla L. n. 40/2004. I risultati a cui la presente indagine ha consentito di pervenire dimostrano quanto sia opportuna l’adozione in Italia di un “modello liberale”, in cui sia lecita anche la fecondazione eterologa (con la previsione di limiti e condizioni volti a tutelare primariamente il superiore interesse del nascituro), onde consentire l’adeguamento al nuovo concetto di “genitorialità” ormai prevalente e l’arresto del cd. “turismo procreativo”.

Properties of cosmic voids in dark energy simulations

The last decade has witnessed the establishment of a Standard Cosmological Model, which is based on two fundamental assumptions: the first one is the existence of a new non relativistic kind of particles, i. e. the Dark Matter (DM) that provides the potential wells in which structures create, while the second one is presence of the Dark Energy (DE), the simplest form of which is represented by the Cosmological Constant Λ, that sources the acceleration in the expansion of our Universe. These two features are summarized by the acronym ΛCDM, which is an abbreviation used to refer to the present Standard Cosmological Model. Although the Standard Cosmological Model shows a remarkably successful agreement with most of the available observations, it presents some longstanding unsolved problems. A possible way to solve these problems is represented by the introduction of a dynamical Dark Energy, in the form of the scalar field ϕ. In the coupled DE models, the scalar field ϕ features a direct interaction with matter in different regimes. Cosmic voids are large under-dense regions in the Universe devoided of matter. Being nearby empty of matter their dynamics is supposed to be dominated by DE, to the nature of which the properties of cosmic voids should be very sensitive. This thesis work is devoted to the statistical and geometrical analysis of cosmic voids in large N-body simulations of structure formation in the context of alternative competing cosmological models. In particular we used the ZOBOV code (see ref. Neyrinck 2008), a publicly available void finder algorithm, to identify voids in the Halos catalogues extraxted from CoDECS simulations (see ref. Baldi 2012 ). The CoDECS are the largest N-body simulations to date of interacting Dark Energy (DE) models. We identify suitable criteria to produce voids catalogues with the aim of comparing the properties of these objects in interacting DE scenarios to the standard ΛCDM model, at different redshifts. This thesis work is organized as follows: in chapter 1, the Standard Cosmological Model as well as the main properties of cosmic voids are intro- duced. In chapter 2, we will present the scalar field scenario. In chapter 3 the tools, the methods and the criteria by which a voids catalogue is created are described while in chapter 4 we discuss the statistical properties of cosmic voids included in our catalogues. In chapter 5 the geometrical properties of the catalogued cosmic voids are presented by means of their stacked profiles. In chapter 6 we summarized our results and we propose further developments of this work.