Constraining inflationary scalar field models with CMB spectral distortions
The Cosmic Microwave Background (CMB) demonstrates extreme uniformity, with only small temperature anisotropies of the order of 10^(-5). These anisotropies are believed to originate from primordial density perturbations, caused by quantum fluctuations of scalar fields during the cosmic inflation. In...
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| Muut tekijät: | , , , , , |
| Aineistotyyppi: | Lisensiaatintyö |
| Kieli: | eng |
| Julkaistu: |
2020
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| Aiheet: | |
| Linkit: | https://jyx.jyu.fi/handle/123456789/69925 |