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Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/171205
Understanding the Cosmic Microwave Background and its relevance in Cosmology
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The Cosmic Microwave Background (hereafter CMB) allows the accurate determination of cosmological parameters upon a careful study of its temperature anisotropies. In this work, physical phenomena that give rise to such anisotropies are discussed, along with an exhaustive analysis on the impact of baryon and dark matter density over the power spectrum's shape by using an online simulator. Finally, a sky map, illustrating the spatial distribution of temperature anisotropies, is generated.
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Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Alberto Manrique
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FERNÁNDEZ BONET, David. Understanding the Cosmic Microwave Background and its relevance in Cosmology. [consulted: 11 of June of 2026]. Available at: https://hdl.handle.net/2445/171205