Caracterização de espelhos para telescópios Cherenkov

Caracterização de espelhos para telescópios Cherenkov

Raios γ são bilhões de vezes mais energéticos do que fótons visíveis. Através da observação do céu deste tipo de radiação, é possível estudar fenômenos como a emissão de pulsares, explosões de super-novas e buracos negros, assim como os gamma ray bursts, um dos maiores mistérios da ast...

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Bibliographic Details
Main Author:	Jessica Dipold
Other Authors:	Luiz Vitor de Souza Filho
Language:	Portuguese
Published:	Universidade de São Paulo 2015
Subjects:	Cherenkov Telescope Array Espelhos Raios Gama Gamma-rays Mirrors
Online Access:	http://www.teses.usp.br/teses/disponiveis/76/76131/tde-22042015-141655/

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