Dust fluid component from Lie symmetries in Scalar field Cosmology
Andronikos Paliathanasis
TL;DR
This paper demonstrates that in scalar-field cosmology, dust fluid components can emerge as quantum corrections derived from solutions of the Wheeler-DeWitt equation influenced by Lie symmetries, linking energy density to wavefunction frequency.
Contribution
It introduces a novel connection between Lie symmetries, quantum corrections, and dust fluid components in scalar-field cosmology.
Findings
Dust fluid arises as quantum correction from Wheeler-DeWitt solutions.
Energy density of dust fluid correlates with wavefunction frequency.
Lie symmetries generate solutions that include dust fluid components.
Abstract
We show that in scalar-field cosmology, a dust fluid follows as quantum corrections from solutions of the Wheeler-DeWitt equation generated by Lie symmetries. The energy density of the dust fluid is related with the frequency of the wavefunction.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.