The renewed role of sweep functions in noisy shortcuts to adiabaticity

We study the robustness of different sweep protocols for accelerated adiabaticity following in the presence of static errors and of dissipative and dephasing phenomena. While in the noise-free case, counterdiabatic driving is, by definition, insensitive to the form of the original sweep function, this property may be lost when the quantum system is open. We indeed observe that, according to the decay and dephasing channels investigated here, the performance of the system becomes highly dependent on the sweep function. Our findings are relevant for the experimental implementation of robust shortcuts-to-adiabaticity techniques for the control of quantum systems

Scenari: Corte costituzionale

Commento breve al alcune pronunce della Corte costituzional

The impact of diabetes in implant oral rehabilitations: A bibliometric study and literature review

Introduction: Diabetes represents a potential risk factor for bone healing and dental implant treatment predictability. The aim of the present investigation was to perform a bibliometric evaluation of articles on the topic of the impact of diabetes on implant oral rehabilitations. Material and methods: A Boolean keywords search was performed on Scopus database and recorded the list of articles, authors and affiliations. The journal impact factor was calculated by the Journal Citation Report Clarivate electronic database. The total papers, number of citations and journal impact factors were calculated. Results: a total of 476 papers and 162 authors were assessed. The mean authors total citations were 2880.11± 4070.24 and the mean impact factor value was 1.942±1.15 Conclusions: uncontrolled diabetes impacts on dental implant rehabilitation with an increased risk of implant failure and periimplant disease in long-term rehabilitation

Atomic interactions for qubit-error compensation

Experimental imperfections induce phase and population errors in quantum systems. We present a method to compensate unitary errors affecting also the population of the qubit states. This is achieved through the interaction of the target qubit with an additional control qubit. We show that our approach works well for single-photon and two-photon excitation schemes. In the first case, we study two reduced models: (i) a two-level system in which the interaction corresponds to an effective level shift and (ii) a three-level one describing two qubits in the Bell triplet subspace. In the second case, a double Stimulated Raman Adiabatic Passage process is presented with comparable compensation efficiency with respect to the single-photon case

B cells in the formation of Tertiary Lymphoid Organs in autoimmunity, transplantation and tumorigenesis.

TLS develop in target organs of autoimmune diseases, transplantation and cancer. • TLS can function as germinal centres supporting B-cell selection/differentiation. • TLS can be destructive or have beneficial effects at the site of inflammation/disease. • Therapeutic targeting of TLS results in beneficial effects in patients, though inhibition may lead to immune suppression while stimulation may lead to autoimmunity. Tertiary lymphoid organs named also tertiary lymphoid structures (TLS) often occur at sites of autoimmune inflammation, organ transplantation and cancer. Although the mechanisms for their formation/function are not entirely understood, it is known that TLS can display features of active germinal centres supporting the proliferation and differentiation of (auto)-reactive B cells. In this Review, we discuss current knowledge on TLS-associated B cells with particular reference on how within diseased tissues these structures are linked to either deleterious or protective outcomes in patients and the potential for therapeutic targeting of TLS through novel drugs

SPRITZ is sparkling: Simulated CO and [C II] luminosities

Aims. We present a new prediction for the luminosity functions (LFs) of the [C II] line at 158 mu M, of the CO lines from J = 0 to J = 24, and of the molecular gas mass density up to z = 10, using the Spectro-Photometric Realisations of Infrared-selected Targets at all-z (SPRITz) simulation.Methods. We update the state-of-the-art phenomenological simulation SPRITZ to include both the CO (J <= 24) and the [C II] line luminosities. This has been performed using different empirical and theoretical relations to convert the total infrared luminosity (or star formation rate, SFR) to the [C II] or CO luminosity. The resulting line LFs were compared for validation with a large set of observations available in the literature. We then used the derived CO and [C II] line luminosities to estimate the molecular gas mass density and compare it with available observations.Results. The CO and [C II] LFs presented here are in good agreement with all the available observations. In particular, the best results for [C II] are obtained deriving the [C II] luminosity directly from the SFR, but considering a dependence of this relation on the gas metallicity. For all the CO LFs, the estimates favoured by the data are derived considering different relations, depending on the ionisation mechanism dominating each galaxy, namely star formation or active galactic nuclei, and, moreover, by deriving the J >= 4 CO lines directly from the [C II] luminosity. However, further data are necessary to fully distinguish between models. Finally, the best agreements with observations of the molecular gas mass density are derived by converting the [C II] luminosity to H-2 mass, using a [C II]-to-H-2 conversion similar to 130 M-circle dot/L-circle dot. All the line LFs, useful for planning and interpreting future observations, are made publicly available

Star-forming galaxies versus low- and high-excitation radio AGN in the VLA-COSMOS 3GHz Large Project

We study the composition of the faint radio population selected from the VLA-COSMOS 3GHz Large Project, a radio continuum survey performed at 10 cm wavelength. The survey covers the full 2 square degree COSMOS field with mean $rms\sim2.3$ $\mu$Jy/beam, cataloging 10,899 source components above $5\times rms$. By combining these radio data with UltraVISTA, optical, near-infrared, and Spitzer/IRAC mid-infrared data, as well as X-ray data from the Chandra Legacy, and Chandra COSMOS surveys, we gain insight into the emission mechanisms within our radio sources out to redshifts of $z\sim5$. From these emission characteristics we classify our souces as star forming galaxies or AGN. Using their multi-wavelength properties we further separate the AGN into sub-samples dominated by radiatively efficient and inefficient AGN, often referred to as high- and low-excitation emission line AGN. We compare our method with other results based on fitting of the sources' spectral energy distributions using both galaxy and AGN spectral models, and those based on the infrared-radio correlation. We study the fractional contributions of these sub-populations down to radio flux levels of $\sim$10 $\mu$Jy. We find that at 3 GHz flux densities above $\sim$400 $\mu$Jy quiescent, red galaxies, consistent with the low-excitation radio AGN class constitute the dominant fraction. Below densities of $\sim$200 $\mu$Jy star-forming galaxies begin to constitute the largest fraction, followed by the low-excitation, and X-ray- and IR-identified high-excitation radio AGN.Comment: 7 pages, 3 figures, The many facets of extragalactic radio surveys: towards new scientific challenges, Bologna 20-23 October 201

Body Mass Index in Children and Their Parents: A Cross-Sectional Study in a Study Population of Children from Southern Italy

The prevalence of overweight and obesity has increased over the last decades. Parental obesity plays an important role in determining childhood obesity. We aimed to evaluate the relationship between parental and offspring’ weight status in a population of children from South of Italy, as no data have ever been published from this area. We recruited 636 children (5.7 ± 1.5 years old) and their parents. Seventy-three (11.5%) and sixteen (2.5%) children were overweight and obese, respectively. Offspring weight status was significantly associated with parents’ weight status. The linear regression analysis showed that offspring BMI was more affected by paternal than by maternal BMI. Our data confirmed that parents’ weight status plays an important role on children’s BMI. Interestingly, in our study, parents’ height and weight were measured and not reported as in most of the previous papers, strengthening our conclusions. We suggest that intensive nutritional education and preventive programs should be performed in children with overweight / obese parents rather than in children with normal weight parent. Furthermore, nutritional education should be performed also for overweight parents to modify preventable risk factor for pediatric obesity