Characterizing the physical parameters of the Black Hole Binary coalescence GW170104: Distances, Masses, and Spins.

Characterizing the physical parameters of the Black Hole Binary coalescence GW170104: Distances, Masses, and Spins.

Gravitational waves start a new era of observational astronomy, allowing us to investigate the astrophysics of binary black holes and test general relativity. The present thesis is aimed to explain what are gravitational waves, how they were predicted and could be studied. It is focused on the chara...

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Bibliografische gegevens
Hoofdauteur: Solórzano Aguilar, Carlo Magno (author)
Formaat: bachelorThesis
Taal:eng
Gepubliceerd in: 2019
Onderwerpen:
Gravitational-waves
PyCBC
LIGO
Bayesian Inference
Post-Newtonian Methods
Ondas Gravitacionales
Inferencia Bayesiana
Métodos Post-Newtonianos
Online toegang:http://repositorio.yachaytech.edu.ec/handle/123456789/50
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