Manifestazioni Cranio-facciali delle Neurofibromatosi

The term neurofibromatosis (NF) subsumes at least seven different genetic disorders associated by the presence of neurofibromas located in the skin, oral cavity, visceral and skeletal level. As NF1 (Von Recklinghausen disease), one of the most common genetic diseases, can have oral manifestations, dentists have to be aware about pathognomonic features. The thesis’ target is the literature’s review on the NF1 manifestations either systemic or cefalic area and these features’ research in a specimen of 30 patients NF1 affected. NF1 is manifested in the cefalic area locating either in the jaws (isolated neurofibromas, ipoplasia or bone structures absence) or soft tissues (fibromas and neurofibromas located in: cheeck, lips, oral mucosa, tongue, mouth’s floor, gingiva and palate). Frequently, NF1 patients are affected by dental anomalies of position, number and eruption, that determinates the possibility of orthopaedic-orthodontic problems. An increased prevalence of the caries risk and a possible pulpar involvement of neurofibromas is reported. Clinical and radiographical typical signs of the disease and specific indications for the differential diagnosis with other oral pathologies are described (cysts and odontogenic tumors, periapical lesions of endodontic origin and severe parodontitis). The importance of screening programs and periodical follow-ups (biannual dental visits from the age of four years, annual X-ray checks from the age of six) is supported by the high frequency of manifestations at hard and soft tissues level of the cefalic area and by the documented risk of malignant transformation.

Background minimization issues for next generation hard X-ray focusing telescopes

The hard X-ray band (10 - 100 keV) has been only observed so far by collimated and coded aperture mask instruments, with a sensitivity and an angular resolution lower than two orders of magnitude as respects the current X-ray focusing telescopes operating below 10 - 15 keV. The technological advance in X-ray mirrors and detection systems is now able to extend the X-ray focusing technique to the hard X-ray domain, filling the gap in terms of observational performances and providing a totally new deep view on some of the most energetic phenomena of the Universe. In order to reach a sensitivity of 1 muCrab in the 10 - 40 keV energy range, a great care in the background minimization is required, a common issue for all the hard X-ray focusing telescopes. In the present PhD thesis, a comprehensive analysis of the space radiation environment, the payload design and the resulting prompt X-ray background level is presented, with the aim of driving the feasibility study of the shielding system and assessing the scientific requirements of the future hard X-ray missions. A Geant4 based multi-mission background simulator, BoGEMMS, is developed to be applied to any high energy mission for which the shielding and instruments performances are required. It allows to interactively create a virtual model of the telescope and expose it to the space radiation environment, tracking the particles along their path and filtering the simulated background counts as a real observation in space. Its flexibility is exploited to evaluate the background spectra of the Simbol-X and NHXM mission, as well as the soft proton scattering by the X-ray optics and the selection of the best shielding configuration. Altough the Simbol-X and NHXM missions are the case studies of the background analysis, the obtained results can be generalized to any future hard X-ray telescope. For this reason, a simplified, ideal payload model is also used to select the major sources of background in LEO. All the results are original contributions to the assessment studies of the cited missions, as part of the background groups activities.