Carneiro 2006: From de Sitter to de Sitter — a non-singular universe driven by vacuumResearch Paper
Motivation
The cosmological constant problem is the mismatch between the vacuum energy density predicted by quantum field theory in flat space–time and the small value of the cosmological term inferred from observations (Weinberg 1989). One line of work replaces the constant by a decaying vacuum: a time-dependent cosmological term that falls as the universe expands, while the energy it loses is transferred to matter so that total energy is conserved.
S. Carneiro's essay From de Sitter to de Sitter: a non-singular inflationary universe driven by vacuum (Int. J. Mod. Phys. D 15 (2006) 2241–2247, honorable mention in the 2006 Gravity Research Foundation essay competition) derives such a law from a semi-classical argument, , and studies the cosmologies it produces. In the early-time regime it finds a universe with no initial singularity: an eternal quasi-de Sitter phase at the Planck scale, followed by a fast transition to a radiation era. In the late-time regime it finds a dust era that tends again to a de Sitter universe. The calculations in the paper are explicit closed-form computations, which makes them a good target for a complete machine-checked development.
Setting
All quantities are in Planck units, and space is flat. The expansion is described by the Hubble parameter of a scale factor . The cosmic fluid has total energy density and total pressure , where are the matter density and pressure and is the vacuum term. The Friedmann equation is and the conservation equation is
Radiation has and dust has . The relative energy densities are and , and the deceleration parameter is .
The vacuum term comes from a massless scalar field obeying . For slowly varying this has the damped radial plane-wave solution , with and given by explicit square-root formulas (Eqs. (7)–(8)), and energy density . Shifting the cutoff of the thermally regularized vacuum integral by and subtracting the flat-space value gives the vacuum term . In the mission's Lean development these objects are waveNumber, dampingRate, planeWave, vacuumTerm, dustScaleFactor and decelerationParameter, all in the namespace CarneiroDeSitter.
Formalization targets
Goal: the non-singular early universe
With radiation and , the evolution equation is (Eq. (12)). The goal asserts that it has a solution defined for all times, given implicitly by Eq. (13):
Milestones (in the order of the paper)
- Eq. (2): .
- Eqs. (5)–(8): the damped plane wave solves for constant .
- Eqs. (9)–(10): its energy density is .
- Eq. (11): as and as .
- Eq. (12): the conservation equation with , , gives .
- Eq. (13): every solution on with satisfies .
- p. 2245: , , .
- Eq. (14): solves the dust era with .
- Limits of (14): as and as .
- Eq. (15): .
Significance
The goal is the paper's central claim: under the stated vacuum law the universe has existed for an infinite past, in a quasi-de Sitter phase with , and leaves it through a transition in which and fall towards zero, producing radiation. The milestones cover the steps the paper uses to reach it (the vacuum law, the evolution equation and its integration) and the late-time picture (the dust solution and its de Sitter limit, which the paper links to the Eddington–Dirac large-number relation ).
The results are proved by hand calculation in the paper. The same evolution equation and implicit solution reappear in Carneiro's later paper Cosmological Concordance Model with Particle Creation (2012), whose statements are also on the platform (namespace CarneiroParticleCreation); this mission formalizes the 2006 paper, its vacuum law and its late-time dust solution. Formalizing them produces a verified account of which statements are exact identities and which are approximations. Where the paper writes "", the milestones state the exact identity or asymptotic equivalence behind it.
Difficulty
The algebraic milestones (5, 7) are routine. The goal concerns a function known only implicitly: the solution is the inverse of on , and its existence on the whole line, its differentiability and its end behaviour all have to be established for an inverse function, not read off a formula. Milestone 6 is a uniqueness statement on all of , so it cannot be checked by substitution. Milestones 1 and 10 are improper integrals whose values involve and , and they need integrability arguments near and . Milestones 2, 3, 8 and 9 involve derivatives of complex exponentials, square roots and real powers, where Lean's conventions for and at non-positive arguments must be handled.
Formalization scope
- Real numbers throughout; the scalar field is complex-valued, and derivatives are one-variable derivatives in or .
- In milestones 2–3 the Hubble parameter is a constant and the Laplacian of the radial plane wave is , which is the paper's approximation.
- is Mathlib's
Real.artanh, the real power isReal.rpow, isAsymptotics.IsEquivalent, and is written as . - Every statement that divides by or assumes or . The goal requires the solution on the whole real line and states both limits, so a solution on a half-line or a constant function does not satisfy it.
- Approximate steps of the paper that are not exact statements (the identification , the radiation law quoted from earlier work, and the holographic entropy estimates) are not formalized.
Contributions are welcome on all milestones. The inverse-function and Bose-integral arguments can be reused outside this mission.
Selected references
- S. Carneiro, From de Sitter to de Sitter: a non-singular inflationary universe driven by vacuum, Int. J. Mod. Phys. D 15 (2006) 2241–2247. https://doi.org/10.1142/S0218271806009510
- S. Weinberg, The cosmological constant problem, Rev. Mod. Phys. 61 (1989) 1–23. https://doi.org/10.1103/RevModPhys.61.1