Lun Mar Mié Jue Vie Sáb Dom
Speaker Tipo de Evento
Feb 22 2016 - 15:00 Using dark energy to suppress power at small scales Savvas Nesseris The latest Planck results reconfirm the existence of a slight but chronic tension between the best-fit Cosmic Microwave Background (CMB) and low-redshift observables: power seems to be consistently Seminar
Feb 23 2016 - 11:30 Are cosmic strings back? ERC-SPLE organizes a bi-weekly journal club, the SPLE-club, in which IFT members and visitors interested in string model building and related topics gather to discuss recent papers, new resul SPLE-Club
Feb 23 2016 - 15:00 Determining the physical impact of operators in effective field theories Luca Merlo I will discuss a counting rule that allows to order effective operators in terms of their physical impact. It applies to weakly and strongly coupled theories. Webinars
Feb 25 2016 - 15:00 Aspects of dynamical EWSB with a Higgs: from the EFT to concrete models Oscar Cata Dynamical EWSB, although initially conceived for Higgsless models, can easily accommodate a naturally light scalar via different dynamical mechanisms. Seminar
Feb 26 2016 - 15:00 Coffee with a teaspoon of phenomenology (UNUSUAL TIME) Pheno-Coffee
Feb 29 2016 - 15:00 Charged hadrons in a finite box Agostino Patella In order to calculate QED corrections to hadronic physical quantities by means of lattice simulations, a coherent description of electrically-charged states in finite volume is needed. Seminar
Mar 4 2016 - 15:00 March Pheno-Coffee (UNUSUAL TIME) Pheno-Coffee
Mar 7 2016 - 15:00 Theory status of (g-2)_mu and experimental prospects Fred Jegerlehner he anomalous magnetic moment of the muon provides stringent tests for the electroweak Standard Model (SM) and is an excellent monitor for new physics. Seminar
Mar 8 2016 - 11:30 A jump into topological insulators Alberto Cortijo This is the first of a small series of holoclubs dedicated to the topic of topological insulators. HoloClub
Mar 10 2016 - 15:00 Relaxion and natural inflation with multiple axions Kiwoon Choi Both natural inflation scenario and the relaxion solution to the weak scalehierarchy problem involve an axion-like field which is required to have Seminar