ATTENTION/WARNING - NE PAS DÉPOSER ICI/DO NOT SUBMIT HERE

Ceci est la version de TEST de DIAL.mem. Veuillez ne pas soumettre votre mémoire sur ce site mais bien à l'URL suivante: 'https://thesis.dial.uclouvain.be'.
This is the TEST version of DIAL.mem. Please use the following URL to submit your master thesis: 'https://thesis.dial.uclouvain.be'.
 

Search for coincident neutrino and gravitational wave emissions from active galactic nuclei

Gorski, Romain
(2023)

Files

Gorski_78101800_2023_AEGWN_Bestfitpy.txt
  • Closed access
  • Text
  • 3.57 KB
Gorski_78101800_2023_AEGWN_PEpy.txt
  • Closed access
  • Text
  • 4.22 KB
Gorski_78101800_2023_Toolboxpy.txt
  • Closed access
  • Text
  • 12.92 KB
Gorski_78101800_2023.pdf
  • Closed access
  • Adobe PDF
  • 39.45 MB

Details

Supervisors
Bruno, Giacomo ; de Wasseige, Gwenhaël
Faculty
Faculté des sciences
Degree label
Master [120] en sciences physiques, à finalité approfondie
Abstract
While binary black hole mergers are not expected to efficiently accelerate cosmic particles, one suspects the surrounding environment to play a crucial role for the observations of joint emissions of cosmic messengers from these systems. In this work, we consider the case of binary black hole mergers occurring in the inner region of active galaxies. In such cases, the orbital evolution of the system might lead to the acceleration of the surrounding gas and produce particles via different processes such as particle collisions. Envisioning their low interaction rate, neutrinos constitute perfect candidates for the hunt of such events because they can make their way through the thickness of the accretion disk of the AGN. We try to find gravitational wave and astrophysical neutrino events coinciding in both space and time, and with the position of AGN.