Simple

Cosmic Engine: Why Vacuum is Not Empty

Original: "Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy"
· Joan Solà Peracaula
The vacuum energy density changes over time, explaining both inflation after the Big Bang and the current acceleration of the Universe.
Abstract

Picture the vacuum not as emptiness, but as an ocean with waves. A new approach suggests its energy rises and falls with the expansion of the Universe. This eliminates the need for a mysterious constant and one invisible particle, explaining both the current acceleration and the birth of the cosmos. Could the vacuum itself be steering cosmic evolution?

Links in the knowledge graph 1

The Universe is a cosmic engine. In the first moments of the Big Bang, its 'motor' roared to life, generating colossal vacuum energy through ultrafast expansion. Today, expansion has slowed, and the engine has settled into a quiet idle; the same energy has become a gentle dark background, pushing galaxies apart.

Vacuum energy is not constant; it changes with the expansion rate, like an engine's roar when you step on the gas.

It's long been known that the Universe is expanding (Edwin Hubble), and that it's driven by the energy of emptiness (Georges Lemaître). The key lies in quantum fluctuations: ghost particles forever pop in and out of curved spacetime, creating an energy 'noise'. This mechanism explains both the instantaneous inflation of the Universe and its homogeneity (the entropy problem), and its traces are preserved in the cosmic microwave background. Perhaps the same approach will clarify the nature of dark matter. Astonishingly, the density of vacuum energy is minuscule—across the volume of Earth, it would only be enough to flash a light bulb—yet it steers the cosmos.

The gravitational constant might also 'breathe'—an idea from Paul Dirac.

🎯 The vacuum energy in our Universe is incredibly small: if you collected it from the entire volume of Earth, it would only be enough to light a bulb for a fraction of a second. Yet on cosmic scales, that's enough to steer the fate of galaxies.

🎬 Echoes of this idea can be found in science fiction: in Greg Egan's novel 'Quarantine', the very structure of vacuum reacts to the presence of an observer.

\rho_{\rm vac}(H) \simeq \rho_{\rm vac}^0 + \frac{3\nu_{\rm eff}}{8\pi G_{\rm N}}(H^2 - H_0^2)
Soft dependence on the square of the Hubble parameter via a small coefficient ν_eff
\beta_{\rho_{\rm vac}} = M \frac{\partial \rho_{\rm vac}}{\partial M} \simeq -\frac{3m^2 H^2}{8\pi^2}\left(\xi - \frac{1}{6}\right)
Rate of change of vacuum energy density with renormalization scale; suppressed by factor m^2 H^2
Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
dark energy Quantum Field expansion of the universe spacetime curvature entropy dark matter cosmic microwave background big bang
Laws
Friedmann equationsHubble's lawsecond law of thermodynamicsgravitational lensingNoether's theoremBekenstein-Hawking entropy
Original: arXiv:2606.05352v2 · CC BY · bridge42worlds