(Português) Resultado Final, após os recursos, do processo seletivo do PPGFSC/UFSC para ingresso em 2016/1

21/12/2015 12:33

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Segue abaixo o Resultado final do Processo Seletivo PPGFSC/UFSC, após análise dos recursos, para ingresso nos cursos de mestrado e doutorado no semestre 2016/1

 

 Resultado final Mestrado

 Resultado final Doutorado

 

 Os candidatos aprovados, assim como os candidatos contemplados com bolsa serão contactados pela coordenação do Programa a partir de 21 de dezembro de 2015.

Qualifying Examination for Doctoral Thesis of Guilherme Grams – 8/December/2015 – thursday-2:30 pm

05/12/2015 09:00

The Physics Graduate Program invites everyone to:

 

Qualifying Examination for Doctoral Thesis

 Guilherme Grams

Equação de estado com o modelo Quark-Meson-Coupling

 

Defense Committee:

 Profª. Drª. Débora Peres Menezes – (president) – UFSC/FSC

Prof. Dr. Manuel Maximo Bastos Malheiro de Oliveira – (external member) – ITA

Prof. Dr. Marcelo Dallagnol Alloy – (local member) – UFSC/Blumenau

Profª. Drª. Natalia Vale Asari – (local member) – UFSC/FSC

Prof. Dr. Paulo Juliano Liebgott – (supplementary member) – UFSC/FSC

Date: 8/December/2015 – thursday – Time: 2:30 pm – Place: Sala 212 – Auditorio do Departamento de Física

Seminar with prof. Prof. Dr. José Groh – 4/December/2015 – 10h15min

27/11/2015 14:25

THE PHYSICS GRADUATE PROGRAM invites everyone to the seminar: 

 

  The surprising look of core-collapse Supernova progenitors 

Prof. Dr. José Groh

Observatório de Genebra

 Abstract:

Stars more massive than about 8 Msun end their lives as a supernova (SN), an event of fundamental importance Universe-wide. The morphological appearance of massive stars before the SN event is very uncertain, both from a theoretical and observational perspective. In this talk, I will discuss the latest results of direct detection of SN progenitor stars by chance in images taken several years before the SN explosion. I will then present the latest stellar evolution and atmospheric models of stars at the pre-SN stage developed by our group. Using these models, we are able to predict the high-resolution spectrum and broadband photometry of SN progenitor stars, which can then be directly compared to the observations. I will discuss the surprising predictions of which kind of stars explode as SN, their look before death, and how detectable they are.

 

Date: 4/December/2015 – (friday) – Place: Sala 212 – Auditorio do Departamento de Física – Time: 10h15min

 

 

 

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