Role of Massive Radiation Pressure in the Early Universe

TL;DR

This paper proposes that radiation pressure from massive stellar explosions significantly influenced the early universe's matter distribution and expansion, potentially explaining observed acceleration.

Contribution

It introduces a novel perspective that early stellar explosion radiation pressure played a key role in shaping the universe's structure and expansion.

Findings

Radiation pressure affected matter distribution

Explains apparent acceleration without dark energy

Highlights importance of early stellar explosions

Abstract

The characteristic distribution of the matter in the universe and its observable expansion with apparent acceleration is the result of historical event - massive stellar explosions' radiation pressure on drifting particles of hydrogen environment in the early stage of universe evolution.