Abstract
We propose that the spectrum of the surface area of the apparent horizon (AH) of de Sitter (dS) spacetime leads to corrected temperature and entropy of the dS spacetime, offering new insights into its thermodynamic properties. This is done by employing the spectrum of the AH radius, acquired from the Wheeler–DeWitt (WDW) equation, together with the Stefan–Boltzmann law, the time-energy uncertainty relation, and the unified first law of thermodynamics.
Original language | English |
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Article number | 165006 |
Number of pages | 15 |
Journal | Classical and Quantum Gravity |
Volume | 41 |
Issue number | 16 |
DOIs | |
Publication status | Published - 18 Jul 2024 |