Masses dynamics during black hole evaporation in spatially flat FLRW universes

Key Points

• Evaporating black holes experience mass dissipation into dust, altering their dynamics and evolution.
• The analysis reveals how black hole and dust masses evolve over time under specific models, providing insights into cosmic behavior.
• Analytical and graphical methods are employed to study these mass dynamics, revealing complex interactions in the spacetime framework.
• Findings may influence theoretical understanding of black hole formation and evaporation in wider cosmological contexts.