Cosmic Friction: How Disorder Fixes the Universe ✎ express

Original: "Entropic backreaction from cosmic structure formation: a thermodynamic approach to the late-time cosmological tensions"
· Biswajit Pandey
arXiv:2605.28797 · 2026-05-27 · arXiv non-exclusive · independent analysis · 3 min
Gravity pulls matter into galaxies, but in doing so it creates a force that pushes space apart and calms its tremors.

A blacksmith forges a sword. With each hammer blow, the red-hot metal flattens, but the hammer, the anvil, and the surrounding air all warm up slightly. Part of the impact energy is irreversibly lost as heat — a trade-off familiar to anyone who has ever driven a nail, and it turns out to be the key to the biggest mysteries of the cosmos.

The universe is expanding faster than it should, and galaxies are clumping together more slowly than predicted.

The two main measurements in modern cosmology — the rate at which distant galaxies recede (the Hubble constant) and the degree of matter clumpiness in the late universe (the parameter S₈)—persistently disagree with calculations. The first number comes out noticeably larger, the second noticeably smaller. It is as if someone added energy to the void while simultaneously damping gravitational collapse. The authors of a new study show that the culprit may hide in the very process of cosmic structure formation, and it is not a new particle or unknown field, but good old-fashioned disorder.

When diffuse gas is pulled together by dark matter's gravity into dense clumps, future stars and galaxies, its particles speed up and collide. Some of the kinetic energy is converted into heat and dissipates into space. In physics terms, this means the system's order decreases and its entropy (a measure of disorder) increases. But entropy growth is not a mere formality. In a closed system, it creates pressure that tends to push boundaries outward. On cosmic scales, this pressure manifests as extra energy that nudges expansion, like warm air inflating a balloon from within.

The same heating that accelerates expansion simultaneously calms the jitter of matter.

At the same time, this heat acts like microscopic friction. Imagine a crowd trying to form a circle. If everyone moves smoothly, the circle quickly tightens. But if people start bustling, bumping into each other, and losing energy to random motion, the gathering slows down. The same goes for galaxies: dissipating energy as heat damps the coherent motion of matter toward clump centers, making the universe's final 'clumpiness' lower than pure gravitational calculations suggest. The same process, turning the mechanical energy of gravitational collapse into heat, simultaneously boosts expansion and softens structure.

This idea has a major virtue: it does not break familiar physics. Einstein's equations, Newton's law of universal gravitation, and the very concept of gravity all remain in place. No new fields, particles, or extra dimensions. Just thermodynamics, the science of heat and order, built into the description of how matter assembles into galaxies. If the calculations hold up, the two biggest cosmological puzzles get a common, surprisingly down-to-earth explanation: the universe simply heats up as it contracts, and this heating changes its fate. So the blacksmith, cooling his sword, sees the heat escape into the air, but on a cosmic scale, that heat does not vanish without a trace; it becomes a force that pushes worlds apart and stills their tremors.

If all the energy dissipated as heat during the formation of all galaxies were gathered in one place, it would be enough to boil an ocean the size of the Milky Way.

In Asimov's 'The Last Question,' entropy becomes the ultimate enemy of intelligence — here, it turns out to be the hidden conductor of cosmic evolution.

Scientists
Ludwig BoltzmannRudolf ClausiusAlan GuthAlexander FriedmannAndrei LindeGeorges Lemaître
Concepts
ecdm model cosmic structure formation structure growth entropic gravity interaction model cosmic expansion quantum cosmological inhomogeneities cosmological constant lambda cdm expanding universe inflationary cosmology backreaction dark energy alternatives entropic shadow early dark energy entropy driven self assembly black hole feedback hubble tension second law of thermodynamics cosmology