Inflation via Black Holes with Quantized Area Spectrum
Tongu\c{c} Rador

TL;DR
This paper proposes a toy model for cosmic inflation driven by a universe initially composed of black holes with quantized area spectra, leading to exponential growth.
Contribution
It introduces a novel inflationary model based on quantized black holes, connecting quantum properties of black holes to early universe expansion.
Findings
Universe undergoes exponential growth in the model
Black holes with quantized area spectra can drive inflation
Initial state of the universe as a collection of such black holes
Abstract
I present a very simplistic toy model for the inflationary paradigm where the size of the universe undergoes a period of exponential growth. The basic assumption I make use of is that black holes might have a quantized area (mass) spectrum with a stable ground state and that the universe has started with a tightly packed collection of these objects alone.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
