http://arxiv.org/abs/1708.04476
These lecture notes are based on the short course presented in the XVI Brazilian School of Cosmology and Gravitation held at the Brazilian Center for Physical Research (CBPF) in July 2017. The objective of this course was to introduce the students to the notion and analysis of black hole quasinormal modes, starting from the linear perturbation theory, including a brief discussion of numerical methods and astrophysical implications in the gravitational wave signals recently detected by LIGO.
C. Chirenti
Wed, 16 Aug 17
14/46
Comments: 8 pages, short course presented in the XVI Brazilian School of Cosmology and Gravitation held at the Brazilian Center for Physical Research (CBPF), Rio de Janeiro, July 10-21 2017