New evidence suggests dark energy—the force driving cosmic expansion—may not be constant after all. Recent large-scale observations point to a possible weakening, challenging the foundations of modern cosmology.
If confirmed, this shift could radically alter the universe’s fate, reopening scenarios like the Big Crunch, where gravity reverses expansion, or the Big Rip, where space-time itself is torn apart.
This episode explores how a dynamic, evolving cosmos may replace our static models—and why the ultimate destiny of the universe is now more uncertain than ever.
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This episode includes AI-generated content.