Simple

Warm Emptiness Instead of Dark Energy ⚡ экспресс

Original: "Thermal Vacuum Cosmology Explains Hubble Tension"
· Robert Alicki
arXiv:2602.08522 · 2026-02-09 · CC BY · ⏱ 1 min · General Relativity Cosmology
The expansion of the Universe may be driven by heat, not a mysterious constant.
Abstract

To explain the puzzling discrepancy in the Universe's expansion rate, astrophysicists proposed tweaking the standard model: instead of constant dark energy, use the heat of the expanding vacuum. This heat, tied to the temperature of the cosmic horizon, is like the glow of a warm body. This approach resolves the famous 'Hubble tension'. Could it be that the void isn't so empty after all, but filled with a thermal breath?

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In the standard cosmological model ΛCDM, galaxies recede under the pressure of dark energy — an invisible spring. However, different methods of measuring the expansion rate give different numbers, as if the ruler's scale is off. This discrepancy was noticed by Edwin Hubble almost a century ago.

A new study proposes an alternative: replace the spring with heat. Emptiness is not empty — according to calculations by Stephen Hawking and Gary Gibbons, the boundary of the visible world, the cosmic horizon, has a tiny temperature. This heat presses from within, and the wider the horizon, the higher the temperature. Expansion becomes a thermal breath: an exhalation of heat expands space.

Unexpected twist: the Universe is not cooling but heating up. The horizon's thermal energy grows, spurring the outward rush. Thus, there's no need for a mysterious constant — the heat of its own boundaries is enough. Big Bang turns out not to be a push from the past, but the kindling heat of the present.

🎯 The temperature of the cosmic horizon is about 10⁻²⁹ Kelvin — billions of times colder than the coldest point ever created by humans.

🎬 Science fiction writers sometimes talk about a 'warm Universe' with an inner fire — here it gets a scientific basis.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
dark energy expansion of the universe Standard Model big bang
Laws
Friedmann equationsHubble's lawNoether's theoremEinstein field equationsPlanck's lawspin–statistics theorem
Original: arXiv:2602.08522 · CC BY · bridge42worlds