Weigh Them All!

1. Front Matter

   Pages i-xxxi

   PDF

2. Introduction

   • Sunny Vagnozzi

   Pages 1-4

3. Standard Models and What Lies Beyond

   • Sunny Vagnozzi

   Pages 5-36

4. Overview of Physical Cosmology

   • Sunny Vagnozzi

   Pages 37-63

5. Massive Neutrinos and How to Search for Them with Cosmological Observations

   • Sunny Vagnozzi

   Pages 65-121

6. A Brief Interlude: Statistical Methods in Cosmology

   • Sunny Vagnozzi

   Pages 123-136

7. Early 2017 Limits on Neutrino Masses and Mass Ordering

   • Sunny Vagnozzi

   Pages 137-150

8. Scale-Dependent Galaxy Bias and CMB Lensing-Galaxy Cross-Correlations

   • Sunny Vagnozzi

   Pages 151-157

9. Scale-Dependent Galaxy Bias Induced by Massive Neutrinos

   • Sunny Vagnozzi

   Pages 159-165

10. Massive Neutrinos Meet (Non-Phantom) Dark Energy

    • Sunny Vagnozzi

    Pages 167-177

11. Massive Neutrinos Meet Inflation

    • Sunny Vagnozzi

    Pages 179-188

12. Summary and Outlook

    • Sunny Vagnozzi

    Pages 189-195

The three neutrinos are ghostly elementary particles that exist all across the Universe. Though every second billions of them fly through us, they are extremely hard to detect. We used to think they had no mass, but recently discovered that in fact they have a tiny mass. The quest for the neutrino mass scale and mass ordering (specifying how the three masses are distributed) is an extremely exciting one, and will open the door towards new physics operating at energy scales we can only ever dream of reaching on Earth. This thesis explores the use of measurements of the Cosmic Microwave Background (the oldest light reaching us, a snapshot of the infant Universe) and maps of millions of galaxies to go after the neutrino mass scale and mass ordering. Neutrinos might teach us something about the mysterious dark energy powering the accelerated expansion of the Universe, or about cosmic inflation, which seeded the initial conditions for the Universe. Though extremely baffling, neutrinos are also an exceptionally exciting area of research, and cosmological observations promise to reveal a great deal about these elusive particles in the coming years.

• Determination of Neutrino Masses
• Neutrino Cosmology
• Neutrino Mass Ordering
• Cosmic Microwave Background
• Large-Scale Structure of the Universe
• Galaxy Surveys
• Neutrinos and Dark Energy
• Cosmic Inflation
• Data Analysis in Cosmology
• Bayesian Statistics

• Kavli Institute for Cosmology, University of Cambridge, Cambridge, UK

  Sunny Vagnozzi

Originally from Italy, Sunny Vagnozzi studied Physics at the University of Trento (BSc, 2012), at the University of Melbourne (MSc, 2014), and finally at Stockholm University, where he obtained his PhD in Theoretical Physics in 2019. He is currently a researcher at the University of Cambridge, where he holds a Newton-Kavli Fellowship. His research is at the interface of cosmology, astrophysics, and particle physics, and aims to address fundamental questions about the origin, composition, and fate of the Universe.

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