Simple

Is Dark Energy Changing? A Fresh Look ⚡ экспресс

Original: "$$w_0$$-probe: A new diagnostic of dark energy based on $$Om$$"
arXiv:2605.27230 · 2026-05-26 · CC BY 4.0 · ⏱ 1 min · Cosmology General Relativity
A direct measurement method has shown that dark energy is probably not constant and may be weakening.
Abstract

Dark energy makes the universe expand faster and faster. To figure out if its strength changes, scientists have come up with a new tool—something like a pressure gauge for the cosmos—that directly measures today's 'push' of dark energy, without complicated calculations. Applying it to the data, they found that dark energy is weaker than expected and seems to be gradually fading. Could the universe's expansion be slowing down?

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The Universe is expanding faster and faster thanks to mysterious dark energy, discovered in the late 1990s by Adam Riess, Saul Perlmutter, and Brian Schmidt using supernovae. For a long time, scientists thought this force was constant, like a gas pedal floored forever. But a new approach — a direct look at that pedal — says otherwise. Without complex calculations, just by linking the expansion rates of different eras, the method reveals: dark energy is now weaker than expected. Its parameter w₀ (think of it as the pedal pressure) is –0.62, not the –1 predicted by the standard model. This rejects conventional cosmology with 95% confidence. If dark energy continues to fade, the Universe's expansion could not only slow down but reverse into a contraction — meaning the cosmos might be headed not for a cold, lonely death, but a fiery rebirth in a new cosmic cycle.

🎯 Although dark energy fills 70% of the cosmos, its nature remains a total mystery: invisible and intangible.

🎬 The idea of changing dark energy echoes the science fiction concept of 'quintessence' — a field that can weaken or strengthen, shaping the destiny of the Universe.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
dark energy expansion of the universe Standard Model supernova
Laws
Friedmann equationsHubble's lawNoether's theoremspin–statistics theoremFermi's golden ruleChandrasekhar limit
Original: arXiv:2605.27230 · CC BY 4.0 · bridge42worlds