Salvador Solé, EduardColom Bernadich, Miquel2018-09-272018-09-272018-06https://hdl.handle.net/2445/124897Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2018, Tutor: Eduard Salvador SoléIn this Treball de Fi de Grau the radio/jet mode Active Galactic Nunclei reheating feedback has been implemented in the AMIGA model, a semi-analytic hierarchical model of galaxy formation that works in the [Delta]CDM cosmology, in order to observe its possible repercussions onthe galaxy and black hole mass functions at redshifts z = 6:3 and z = 3:9 for the cases of radio/jet mode effciency equal to 0:1 and 1.5 p.application/pdfengcc-by-nc-nd (c) Colom, 2018http://creativecommons.org/licenses/by-nc-nd/3.0/es/Formació de les galàxiesNucli galàctic actiuTreballs de fi de grauGalaxy formationActive galactic nucleiBachelor's thesesinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/openAccess