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Dark Energy Twice Went Unstable ⚡ экспресс

Original: "Interacting Dark Sector field theory with phantom crossing"
arXiv:2605.20060 · 2026-05-19 · CC BY · ⏱ 1 min · Cosmology
New data show that dark energy twice briefly became unstable, but a model with dark matter explains it all.
Abstract

A field model is presented to interpret DESI data on dynamic dark energy with a double crossing of the phantom divide (w = –1). Fermionic dark matter is coupled via a Yukawa interaction to a tachyon scalar field governed by Born–Infeld dynamics. The effective equation of state exhibits a phantom transition, while the fundamental field remains stable. A joint analysis of BAO (DESI DR2), CMB (Planck 2018), and Type Ia supernova data yields robust parameter constraints and reconstructs a recent double crossover. Under natural assumptions, the mass of the fermionic dark matter is estimated as ~1.9×10⁻³ eV, pointing to new light particles and motivating future tests using cosmological perturbations.

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When a car on cruise control hits a bump, the speed jumps for a moment, but the engine runs smoothly. Something similar was recently noticed with dark energy — the force that makes the Universe expand faster and faster. Scientists describe it with the parameter w: if it drops below -1, the Universe would accelerate toward the 'Big Rip.' DESI project data showed that w twice briefly dipped into this dangerous zone, but without disaster. Usually, such behavior requires weird physics, but a new model gives a simple explanation.

In it, dark matter particles interact with dark energy like a bump in the road: their coupling gently nudges the system, and the parameter w temporarily falls below -1, while dark energy itself remains stable. The model was checked against three sources: distances to galaxies (DESI), properties of the cosmic microwave background (Planck), and the brightness of distant supernovae. Everything matched.

The most unexpected conclusion: dark matter particles must be incredibly light — around 0.002 electronvolts. The electron's mass is almost half a million times larger. Such 'fluffs' might be part of an unknown family of particles yet to be discovered.

🎯 Dark energy behaves like water that momentarily boils without forming bubbles — pressure spikes, but the system quickly settles down.

🎬 The idea of unstable dark energy spawned many stories about the 'Big Rip,' such as in Paul McAuley's novel 'The War with the Remotes'.

w = -1
w — a number that describes dark energy; if w < -1, the Universe expands with ever-increasing force, potentially leading to a rip.
Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
dark energy dark matter expansion of the universe supernova
Laws
Friedmann equationsHubble's lawgravitational lensingvirial theoremChandrasekhar limitFermi acceleration
Original: arXiv:2605.20060 · CC BY · bridge42worlds