Observation of high-energy neutrinos using Cerenkov detectors embedded deep in Antarctic Ice

Neutrinos are elementary particles that carry no electric charge and have little mass. As they interact only weakly with other particles, they can penetrate enormous amounts of matter, and therefore have the potential to directly convey astrophysical information from the edge of the Universe and from deep inside the most cataclysmic high-energy regions. The neutrino's great penetrating power, however, also makes this particle difficult to detect. Underground detectors have observed low-energy neutrinos from the Sun and a nearby supernova2, as well as neutrinos generated in the Earth's atmosphere. But the very low fluxes of high-energy neutrinos from cosmic sources can be observed only by much larger, expandable detectors in, for example, deep water3,4 or ice5. Here we report the detection of upwardly propagating atmospheric neutrinos by the ice-based Antarctic muon and neutrino detector array (AMANDA). These results establish a technology with which to build a kilometre-scale neutrino observatory necessary for astrophysical observations1.0SCOPUS: ar.jinfo:eu-repo/semantics/publishe

Sixty Years of Drug Discovery for Type 2 Diabetes: Where Are We Now?

The control of blood glucose is a dynamic interplay involving several complex systems. In diabetes these systems are perturbed, resulting in a disease continuum of progressive decline over many years. Today, excluding insulin, there are eight classes of anti-diabetic agent which have taken over 60 years to add to the pharmacy chest. In this review I have examined each of these classes with some bias towards drug discovery thinking. Based on history, future science here will be strong, progressive and innovative; the huge test for industry is their response to enormous challenges besetting drug discovery and successfully turn the drug discovery praxis into affordable, effective and safe medicines