Big-Bang Nucleosynthesis on a bubble universe nucleated in Kerr-AdS$_5$ Black Hole
We present the Big-Bang Nucleosynthesis (BBN) simulation with a bubble universe scenario around a rotating black hole (BH) in Kerr-AdS$_5$ spacetime to explain recently updated observations of light elements such as the primordial helium abundance. In this scenario, the geometry of the 4D- early Uni...
Saved in:
Main Authors | , , |
---|---|
Format | Journal Article |
Language | English |
Published |
19.08.2024
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | We present the Big-Bang Nucleosynthesis (BBN) simulation with a bubble
universe scenario around a rotating black hole (BH) in Kerr-AdS$_5$ spacetime
to explain recently updated observations of light elements such as the
primordial helium abundance. In this scenario, the geometry of the 4D- early
Universe is described as a vacuum bubble that undergoes quasi-de Sitter
expansion in Kerr- AdS$_5$ spacetime. We find that the BH mass and spin
parameter, which show an anti-correlation against the total radiation, are
important to resolve the ^4$He anomaly. The present results provide clues to
finding a connection between the observed results of light-element
nucleosynthesis and the scenario of the 4D-bubble universe in AdS$_5$
spacetimes |
---|---|
Bibliography: | RIKEN-iTHEMS-Report24 |
DOI: | 10.48550/arxiv.2408.10315 |