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Bachelor thesis

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cc-by-nc-nd (c) Colom, 2018
Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/124897

Implementation of the radio/jet mode AGN feedback in the AMIGA model

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Abstract

In 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.

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Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2018, Tutor: Eduard Salvador Solé

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COLOM BERNADICH, Miquel. Implementation of the radio/jet mode AGN feedback in the AMIGA model. [consulted: 6 of June of 2026]. Available at: https://hdl.handle.net/2445/124897

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