10-01-2017 “Physico-mathematical methods for complex data”: this is the title of the symposium that will be held at SISSA on 13 January 2017. Riccardo Zecchina of the Politecnico di Torino will open the meeting with a talk on neural networks architectures. Antonietta Mira of the Università della Svizzera Italiana will discuss a methodology for statistical inference in complex models. The symposium will be closed by Yonatan Loewenstein of the Hebrew University of Jerusalem, with a talk on the computational modeling of operant learning.
SISSA is hosting the first of a series of meetings to discuss potential scenarios. To talk about the advancements and perspectives of this area, some of the top scientists in the field will be meeting on 10 and 11 January 2017
03-01-2017 You can now register through the website www.startcupfvg.it to Start Cup FVG, the business plan competition open to innovative business project and to start-ups. The deadline is February 28, 2017.
La SISSA di Trieste tra le eccellenze della ricerca italiana. È questo il verdetto dell’Anvur, l’Agenzia di valutazione del sistema universitario e della ricerca, che ha reso nota ieri la classifica dei migliori atenei d’Italia nella Valutazione della Qualità della Ricerca (VQR).
Luca Venturi, che ha conseguito una laurea specialistica in matematica UNITS-SISSA (laurea triennale in matematica presso università degli studi di Pavia), il 21 dicembre 2016 riceverà, presso la sede di Confindustria Pavia, il premio di Laurea per la sua tesi di laurea magistrale discussa all’Università di Trieste il 14 luglio 2016 dal titolo “Weighted reduced order methods for parametrized PDEs in Uncertainty Quantification problems”.
Although our genes normally come in pairs (one on each homologous chromosome), sometimes one of them is missing and the “surviving” one is unable to do all the work (it is referred as "haploinsufficient"): this situation can give rise to very serious diseases. So what can be done to fight these, often neurological, diseases? One possible strategy has been successfully adopted by a SISSA research team, in vitro and in vivo: using leading-edge techniques to stimulate the surviving gene to also do the work of the missing gene.
Statistical analysis of mini-spiral galaxies shows an unexpected interaction between dark matter and ordinary matter.
Psychologists and neuroscientists have thoroughly investigated olfactory behaviours in newborns and adults, but relatively little is known about the characteristics of the sense of smell during infancy and adolescence. In a study carried out by SISSA in collaboration with the Please Touch Museum of Philadelphia (an interactive science museum for children), over 150 children aged 3 to 11 years old took part in a simple experiment allowing investigators to trace the curve of visuo-olfactory integration.
The more massive, or full of stars, a galaxy is, the faster the stars in it are formed. This seems to be the general rule, which is contradicted, however, by some abnormal cases, for example thin (not massive) galaxies that are hyperactive in their star formation. Until now the phenomenon had been explained by catastrophic external events like galaxies colliding and merging, but a new theory offers an alternative explanation, related to an in situ (internal) process of galaxy evolution.