Right after the Big Bang, the Universe likely went through a stage of inflation that smoothed out irregularities. However, the fine details of this process are encoded in the cosmic microwave background — the microwave glow that, according to Edwin Hubble's law, has stretched along with spacetime. Searching for deviations from a power-law primordial perturbation spectrum has become one of the main ways to peek beyond the inflationary horizon. The ideas of Alan Guth and Andrei Linde about accelerated expansion predict a nearly scale-invariant spectrum, but if inflation wasn't simple, rhythmic features should show up — like ripples on water from a tossed stone.
To catch these ripples, researchers applied symbolic regression — an algorithm that independently searches for analytic formulas that best describe the data. Instead of fitting pre-made templates, it iterates through combinations of operators (sine, cosine, powers) and finds optimal expressions. Using the CLASS code that solves the Friedmann equations, cosmic microwave background spectra were computed for each variant, and the quality was judged by chi-squared. Radio astronomical data from the Planck satellite and ground-based ACT and SPT-3G, combined into the SPA dataset, were used. Precise numerical processing and spectroscopy on angular scales allowed fine oscillations to be resolved.
Both samples — Planck and SPA — independently chose the inverse k-oscillation as the leading feature: f(k) ∝ cos(B/k) with B ≈ 4 Mpc⁻¹. Remarkably, this result emerged on its own, without human imposition. These oscillations may point to a phase of accelerated expansion with an exotic equation of state. Bayesian comparison with traditional linear (sin(ω k)) and logarithmic (sin(ω ln k)) templates showed that the inverse template gives noticeably better agreement — Δχ² ≈ −12.6 versus −7.7 and −5.8 respectively. Moreover, the amplitude of the inverse oscillations turned out to be at the edge of significance: A = 0.016 ± 0.01, whereas for the standard templates only upper limits were obtained.
If the inverse k-periodicity is real, it could mean that in the early Universe there was a special phase where the scale factor grew as a(t) ∼ $t^p$ with p = -1 — that is, expansion with negative acceleration and an exotic equation of state w < -1, reminiscent of phantom energy. Such scenarios are usually associated with a violation of the null energy condition and require fields that don't fit into the standard model of particle physics. Thus, these oscillations could serve as a test of quantum-gravity effects. Meanwhile, symbolic regression has shown itself capable of uncovering non-obvious correlations while avoiding researcher bias.
Future sky surveys — of the cosmic microwave background by the Simons Observatory and CMB-S4 — with their high sensitivity and resolution will either confirm the inverse oscillations or place tighter constraints on their parameters. At the same time, the symbolic regression method will be refined, paving the way for automated searches for unforeseen patterns in cosmological data without pre-set templates.
The results directly impact inflationary cosmology, early-Universe astrophysics, and data analysis methodology in the era of large surveys, shifting the focus from testing specific models to unbiased physics extraction.
First and foremost, detailed physical modeling is needed to explain the inverse frequency dependence within specific inflationary potentials or alternative theories of gravity.
The search for primordial features is directly tied to the problem of choosing an inflationary scenario among countless theoretical possibilities and to attempts to detect observational signatures of quantum gravity.
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What the work does
In the study, using symbolic regression on Planck and SPA data, inverse oscillations in the primordial power spectrum were discovered: f(k) ∝ cos(B/k) with B ≈ 4 Mpc⁻¹. These oscillations arise spontaneously without imposing templates and provide a better fit (Δχ² ≈ −12.6) compared to linear and logarithmic oscillations. The authors interpret the result as a possible indication of a phase with scale factor a(t) ∼ t^p, p = -1, corresponding to phantom energy with w < -1.
Where its strength is
The strength of the work lies in the application of symbolic regression, which allows for an unbiased search for non-standard deviations from the power-law spectrum, and in obtaining a statistically significant preference for inverse oscillations over traditional templates.
Where it could go next
Worth trying
Why this may matter
If inverse oscillations are confirmed, it would be a strong indication of exotic physics in the early Universe, possibly related to quantum gravity, and would provide a new observational test for inflationary models.
Nearby works in our archive
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Once, symbolic regression, while analyzing pendulum motion, independently derived the law of conservation of energy, surprising even its creators. Now it has set its sights on the mysteries of the Big Bang.