English

Universe's Primordial Quantum Memories

High Energy Physics - Theory 2019-08-01 v1 Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology Quantum Physics

Abstract

We provide a very general argument showing that the Universe must have kept its quantum memories from an epoch much earlier than 6060 e-foldings before the end of inflation. The point is that a generic system of enhanced memory storage capacity exhibits a phenomenon of memory burden. Due to its universal nature this effect must be applicable to de Sitter since the latter has a maximal memory storage capacity thanks to its Gibbons-Hawking entropy. The primordial information pattern encoded in de Sitter memory initially costs very little energy. However, because of Gibbons-Hawking evaporation, the memory burden of the pattern grows in time and increasingly back reacts on the evaporation process. After a finite time the memory burden becomes unbearable and de Sitter quantum breaks. If inflation ended not long before its quantum break-time, the imprints of the primordial memory pattern can be observable. This provides a qualitatively new type of window in the Universe's beginning, a sort of cosmic quantum hair.

Cite

@article{arxiv.1812.08749,
  title  = {Universe's Primordial Quantum Memories},
  author = {Gia Dvali and Lukas Eisemann and Marco Michel and Sebastian Zell},
  journal= {arXiv preprint arXiv:1812.08749},
  year   = {2019}
}

Comments

9 pages, 2 figures

R2 v1 2026-06-23T06:51:44.609Z