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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

Fresh DESI observations hint that dark energy may be dynamic, recently dipping below the phantom divide (w < –1). Researchers have proposed a model in which fermionic dark matter and a tachyon field (with Born–Infeld dynamics) engage in a Yukawa interaction. This triggers a double phantom transition in the effective equation of state, while the field itself stays stable and obeys physical laws. A joint analysis of DESI, Planck, and supernova data supports this scenario and, under natural assumptions, points to ultralight dark matter with a mass of around 0.002 eV — a tantalizing prospect for future tests.

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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