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Open Quantum Systems Decoherence
Quantum Simulation
Quantum Foundations
Universe as Klein-Gordon Eigenstates
arXiv
Authors: Marco Matone
Year
2021
Paper ID
61015
Status
Preprint
Abstract Read
~2 min
Abstract Words
175
Citations
N/A
Abstract
We formulate Friedmann's equations as second-order linear differential equations. This is done using techniques related to the Schwarzian derivative that selects the β-times t_β:=intt a-2β, where a is the scale factor. In particular, it turns out that Friedmann's equations are equivalent to the eigenvalue problems $O1/2 Ψ=fracΛ{12}Ψ\ , qquad O1 a =fracΛ{3} a \ ,which is suggestive of a measurement problem.O_β(ρ,p)are space-independent Klein-Gordon operators, depending only on energy density and pressure, and related to the Klein-Gordon Hamilton-Jacobi equations. TheO_β's are also independent of the spatial curvature, labeled byk, and absorbed inΨ=sqrt a e^{frac{i}{2}sqrt{k}η} \ .The above pair of equations is the unique possible linear form of Friedmann's equations unlessk=0, in which case there are infinitely many pairs of linear equations. Such a uniqueness just selects the conformal timeη\equiv t_{1/2}among thet_β$'s, which is the key to absorb the curvature term. An immediate consequence of the linear form is that it reveals a new symmetry of Friedmann's equations in flat space.
Why This Paper Matters
- This paper contributes to the Quantum Simulation research area in the Quantum Articles archive.
- It adds a 2021 reference point for readers tracking recent quantum research.
- We formulate Friedmann's equations as second-order linear differential equations.
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