Pith. sign in

A Larger Estimate of the Entropy of the Universe

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it
abstract

Using recent measurements of the supermassive black hole (SMBH) mass function, we find that SMBHs are the largest contributor to the entropy of the observable universe, contributing at least an order of magnitude more entropy than previously estimated. The total entropy of the observable universe is correspondingly higher, and is S_obs = 3.1+3.0-1.7x10^104 k. We calculate the entropy of the current cosmic event horizon to be S_CEH = 2.6+-0.3x10^122 k, dwarfing the entropy of its interior, S_CEHint = 1.2+1.1-0.7x10^103 k. We make the first tentative estimate of the entropy of weakly interacting massive particle dark matter within the observable universe, S_dm = 10^87-10^89 k. We highlight several caveats pertaining to these estimates and make recommendations for future work.

citation-role summary

background 1

citation-polarity summary

fields

gr-qc 1

years

2025 1

verdicts

CONDITIONAL 1

roles

background 1

polarities

background 1

representative citing papers

citing papers explorer

Showing 1 of 1 citing paper.

  • Elementary considerations on possible entropy-driven cosmological evolutions gr-qc · 2025-01-25 · conditional · none · ref 8 · internal anchor

    In the entropy-modified Friedmann framework, sustained growth of the entropy source (ḟ/f > 0) makes the universe converge to an effective de Sitter state with density (ḟ/f)²/K², and current data bound the required source strength.