Sort by
Refine Your Search
-
Listed
-
Category
-
Country
-
Program
-
Field
-
, the Piemonte Region, the University of Turin, the Fondazione per l'Arte of the Compagnia di San Paolo, and the Fondazione Cassa di Risparmio di Torino. Over time, additional institutions have joined the original
-
student will be supervised by a teacher-researcher (Dr. A. Chemtob) and a research engineer (Dr. C. Le). The PhD student will work on the synthesis of polymer monomers and colloids. The main applications
-
Additional Information Eligibility criteria -Excellent mastering of synthesis techniques and handling of compounds under inert atmosphere (Schlenk techniques, gloveboxes), including the preparation of highly
-
these entropy carriers has led to a number of original phenomena such as the phonon and phonon-electron hydrodynamic regimes in graphite and antimony. In terms of applications, thermal properties of solids
-
Research Framework Programme? Not funded by a EU programme Is the Job related to staff position within a Research Infrastructure? No Offer Description The main mission is to develop the high frequency (Radio
-
astronomy, and leverage the latest observational results of MeerKAT and other radio telescopes to investigate signals of various particle dark matter candidates. Qualifications: Applicants must have: a Master
-
topic: This position falls within the field of bioenergetics and protein biochemistry. The project aims to study the role of an original extra-membrane structural module involved in the mechanism
-
elements - A letter of motivation. - Two letters of recommendation, at least one from your master project supervisor. - Proof of academic record from official grades or transcripts. Where to apply Website
-
relevant from an interstellar perspective (ANR INTERSTELLAR project) produced by two types of original reactors (low-pressure premixed or diffusion flames). The analyses will be performed using laser
-
specifically designed to address this challenge. Their primary function is to suppress the overwhelming starlight, thereby allowing the detection of the much fainter exoplanet signal. The next generation of