Please use this identifier to cite or link to this item:
Title: Methods to detect primordial black holes in astrophysics
Author: Circunsi Duxans, Martí
Director/Tutor: Miralda Escudé, Jordi
Keywords: Forats negres (Astronomia)
Halo de matèria fosca
Treballs de fi de grau
Black holes (Astronomy
Dark matter halo
Bachelor's thesis
Issue Date: Jun-2020
Abstract: Primordial black holes may account for at least part of the dark matter present in the Universe. We study how primordial black holes might be observed through their impact on observable properties of a star formed at redshift z = 20 in a low-mass dark matter halo. An analytical expression is presented for the reshaping of primordial black holes' orbits assuming the star formation process as adiabatic. An enhanced density profile is obtained due to dark matter halo contraction in the innermost halo region. It is also discussed how this system might produce a LIGO event (10-100Hz). A long periodical signal is expected for MPBH 10 7 M if this system is inside the Milky Way.
Note: Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Jordi Miralda Escudé
Appears in Collections:Treballs Finals de Grau (TFG) - Física

Files in This Item:
File Description SizeFormat 
CIRCUNS DUXANS MARTÍ_1338714_assignsubmission_file_TFG_CIRCUNS_DUXANS_MARTI.pdf275.88 kBAdobe PDFView/Open

This item is licensed under a Creative Commons License Creative Commons