Primordial Black Hole Formation in Modified Gravity
Analysis
This paper explores the formation of primordial black holes (PBHs) within a specific theoretical framework (Higgs hybrid metric-Palatini model). It investigates how large density perturbations, originating from inflation, could have led to PBH formation. The study focuses on the curvature power spectrum, mass variance, and mass fraction of PBHs, comparing the results with observational constraints and assessing the potential of PBHs as dark matter candidates. The significance lies in exploring a specific model's predictions for PBH formation and its implications for dark matter.
Key Takeaways
- •Investigates PBH formation within the Higgs hybrid metric-Palatini model.
- •Analyzes the curvature power spectrum, mass variance, and mass fraction of PBHs.
- •Compares results with observational constraints.
- •Assesses the potential of PBHs as dark matter.
- •Finds that PBHs can account for all or a fraction of dark matter depending on model parameters.
“The paper finds that PBHs can account for all or a fraction of dark matter, depending on the coupling constant and e-folds number.”