A Mistake in the Fourth Order express

Original: "Critical analysis of some weak-field Weyl conformal gravity solutions"
arXiv:2607.20381 · 2026-07-22 · CC BY 4.0 · 2 min
Fourth-order equations cannot be replaced by second-order ones, no matter how tempting.

Spring scales in a shop show weight simply: the load presses on a spring, it compresses, and the needle moves along the scale. The relation between force and compression is direct, like Hooke's law. Now imagine a scale with a tricky platform: the force is transmitted through levers, and the reading depends not only on the weight but also on how the platform itself bends. To calculate it, you need to account for the bending, not just the compression.

In general relativity, gravity is like an ordinary scale: in the weak field, everything reduces to a second-order equation. In conformal gravity, it's a tricky scale with bending: a fourth-order equation.

In several papers, for instance by [scientist:M. R. Tanhayi]Tanhayi[/scient], [scientist:M. Fathi]Fathi[/scient] and colleagues, the authors attempted to describe the weak field in conformal gravity. But instead of the correct fourth-order equation, they used a simpler one — second-order, as in ordinary gravity. This is like trying to describe the bending of the platform by looking only at the compression of a single spring. The result is erroneous solutions that do not describe reality. The authors of the new work checked the calculations and found this substitution.

The mistake is not the only one. In those same papers, it was claimed that the known vacuum solutions of conformal gravity describe the interior of massive bodies. But a vacuum is emptiness; there is no matter there.

Using an equation for emptiness to describe the inside of a star is like trying to measure the temperature in a room with an outdoor thermometer hidden in a closet.

Such inconsistencies call into question the conclusions of those papers. Correcting these errors is important because conformal gravity is one of the candidates for explaining dark matter and dark energy without invoking new particles. If we build a theory on incorrect solutions, we risk heading into a dead end.

In general relativity, gravitational waves are described by second-order equations, while in conformal gravity they would require fourth-order equations: this would greatly complicate their detection.

In Liu Cixin's novel "The Three-Body Problem," aliens use multidimensional folds of space where the familiar laws of physics break down — much like the fourth order of equations changes the rules of the game for gravity.

\nabla^4 \Phi = \kappa \rho
Fourth-order equation for the gravitational potential Φ in conformal gravity, where ∇⁴ is the biharmonic operator, κ is a constant, and ρ is the matter density.
Scientists
Albert EinsteinRobert H. DickeJohn Archibald WheelerJacob BekensteinRainer SachsJames Jeans
Concepts
fr gravity gravitational constant Maxwell's equations Einstein field equations newtonian limit gravitational instanton supergravity