El Programa de Posgrado en Física invita a todos para:
Examen de Cualificación al Doctorado
Rodrigo Pereira Rocha
Difusão e Localização em Sistemas Desordenados Descritas por uma Equação Mestra Estocástica
Jurados
Prof. Dr. Wagner Figueiredo – (Presidente) – FSC/UFSC
Prof. Dr. Mario Jose de Oliveira – (Miembro externo) – IF/USP
Prof. Dr. Nilton da Silva Branco – (Miembro titular) – FSC/UFSC
Prof. Dr. Jeferson de Lima Tomazelli – (Miembro titular) – FSC/UFSC
Fecha: 30 de agosto de 2013- sexta-feira – Horario: 10:00 am -Lugar: Sala de Reuniones del bloque G – Sala 11
EL PROGRAMA DE POSGRADO EN FÍSICA invita a todos para lo seminario:
J-PAS: The Javalambre-Physics of the Accelerated Universe Astrophysical Survey
Narciso Benitez Lozano
Instituto de Astrofísica de Andalucía (CSIC)
Resumen:
The Javalambre-Physics of the Accelerated Universe Astrophysical Survey (J-PAS) is a very wide field Cosmological Survey to be carried out from the Javalambre Observatory in Spain with a purpose-built, dedicated 2.5m telescope, using a set of 54 narrow band and 5 broad band filters over a 1.2Gpix, 4.7deg2 camera. Starting in 2015, J-PAS will image 8500deg2 of Northern Sky and obtain 0.003(1 + z) precision photometric redshifts for 9 × 107 galaxies, about 50 times more than the largest current spectroscopic survey, sampling an effective volume of ∼ 14 Gpc3. In addition J-PAS will also carry out a SNIe survey, a cosmic shear survey (thanks to the superb seeing at Javalambre) and a cluster survey, exploring the four main Dark Energy probes. In fact, and thanks to its innovative design, J-PAS will be the first experiment capable of reaching Stage IV according to the Dark Energy Task Force classification, several years before other projects like Euclid or LSST start their operations. The instrumental development of this project involves a small fraction of the cost and complexity of a high multiplexing spectrograph, yet it will produce data which enable a much wider range of Astrophysical applications: J-PAS effectively uses a 4.7deg2 “IFU” which will produce a low resolution 3D image of the Extragalactic Northern sky. Our survey will have a lasting legacy value, serving as a fundamental dataset for future cosmological projects.
Fecha: 30 de agosto de 2013 – (Viernes) – Lugar: Auditorio del bloque G – Sala 419 – Horário: 10:00
El programa de Posgrado en Física invita a todos para la:
Sustentación de Disertación
Graziâni Candiotto
Método potenciodinâmico aplicado ao estudo da difusão iônica limitada por camada porosa em substratos de ITO
Jurados
Profª. Drª. Maria Luisa Sartorelli – (Presidente) – FSC/UFSC
Prof. Dr. Lucas Fugikawa Santos – (Miembro externo) – Unesp – São José do Rio Preto
Prof. Dr. Osvaldo Frederico Schilling Neto – (Miembro titular) -FSC/UFSC
Profª. Drª. Marta Elisa Rosso Dotto – (Miembro titular) – FSC/UFSC
Fecha: 28 de agosto de 2013 – Miércoles – Horario: 10:00 am – Lugar: Auditorio del bloque G – Sala 419
