0000000000202799

AUTHOR

Roberta Giuffrida

0000-0002-5492-3033

showing 2 related works from this author

A Brief Synopsis on Scalp Melanoma

2020

Melanoma constitutes one of the most sinister and troublesome malignancies encountered by humanity. Generally, the diagnosis of advanced melanoma connotes a grave prognosis, prompting a sense of looming threat of death, however, the early-stage detected disease responds well to robust treatment resulting in reasonable survivorship. Scalp melanomas are even more troublesome, because they typically exhibit more aggressive biologic behavior and are often diagnosed at a late stage. This review tries to comprehensively highlight the various diagnostic, therapeutic, and outcome aspects of scalp melanomas. The literature research includes peer-reviewed articles (clinical trials or scientific revie…

Melanomasmedicine.medical_specialtySkin NeoplasmsMEDLINEDermatologyEnglish languageDiseaseBreslow thickness; head and neck melanomas; melanomas; scalp melanomas; skin malignancies; Humans; Prognosis; Scalp; Head and Neck Neoplasms; Melanoma; Skin NeoplasmsBreslow thickne030207 dermatology & venereal diseases03 medical and health sciences0302 clinical medicinemedicineHumansMelanomaScalp melanomaAdvanced melanomaScalpHead and neck melanomabusiness.industryMelanomaLate stageHead and neck melanomasGeneral MedicinePrognosismedicine.diseaseDermatologyBreslow thickness; Head and neck melanomas; Melanomas; Scalp melanomas; Skin malignanciesClinical trialmedicine.anatomical_structureScalp melanomasHead and Neck NeoplasmsSkin malignancies030220 oncology & carcinogenesisScalpbusinessBreslow thickness
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The supernova remnant SN 1006 as a Galactic particle accelerator

2022

The origin of cosmic rays is a pivotal open issue of high-energy astrophysics. Supernova remnants are strong candidates to be the Galactic factory of cosmic rays, their blast waves being powerful particle accelerators. However, supernova remnants can power the observed flux of cosmic rays only if they transfer a significant fraction of their kinetic energy to the accelerated particles, but conclusive evidence for such efficient acceleration is still lacking. In this scenario, the shock energy channeled to cosmic rays should induce a higher post-shock density than that predicted by standard shock conditions. Here we show this effect, and probe its dependence on the orientation of the ambient…

High Energy Astrophysical Phenomena (astro-ph.HE)Astrophysical plasmasSHARPHorizon 2020MultidisciplinaryFOS: Physical sciencesGeneral Physics and Astronomyshock wavesGeneral ChemistryGeneral Biochemistry Genetics and Molecular BiologyHigh-energy astrophysicsSettore FIS/05 - Astronomia E AstrofisicaEuropean Union (EU)Particle astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomenacosmic rayNature Communications
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