Signals from the hot and whirly matter produced in heavy-ion collisions
Maelena Tejeda Yeomans - University of Colima
Valli, M. (2022). BBN circa 2022: New Physics hints from the Early Universe?. Perimeter Institute. https://pirsa.org/22100144
Valli, Mauro. BBN circa 2022: New Physics hints from the Early Universe?. Perimeter Institute, Oct. 28, 2022, https://pirsa.org/22100144
@misc{ pirsa_PIRSA:22100144,
doi = {10.48660/22100144},
url = {https://pirsa.org/22100144},
author = {Valli, Mauro},
keywords = {Particle Physics},
language = {en},
title = {BBN circa 2022: New Physics hints from the Early Universe?},
publisher = {Perimeter Institute},
year = {2022},
month = {oct},
note = {PIRSA:22100144 see, \url{https://pirsa.org}}
}
Bang Nucleosynthesis (BBN) is one of the greatest outcome of the Standard Model of Particle Physics when put next to ΛCDM cosmology. In this talk, I will first review the key aspects of standard BBN and illustrate a new code -- PRyMordial -- to make state-of-the-art predictions of primordial light-element abundances within and beyond the Standard Model. I will then highlight the latest measurements regarding the primordial abundance of helium-4 and deuterium, and present evidence at the 2 sigma level for a nonzero lepton asymmetry from BBN data jointly with the Cosmic Microwave Background. I will leave some final comments on how a large total lepton asymmetry can be consistently realized in the Early Universe.
Zoom Link: https://pitp.zoom.us/j/95011247645?pwd=S0EwZG9nSHQvTjV0QjBxeHNUWWtmUT09