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The unprecedented flare from the supermassive black hole Sagittarius A* in May 2025 challenges standard astrophysical models. My new paper, "The 2025 Flare of Sagittarius A* as a Retrocausal Information Echo in HLV Theory," proposes a novel solution from the Helix-Light-Vortex (HLV) framework.

I hypothesize that the flare was not caused by infalling matter, but was a retrocausal information echo from a significant future event, transmitted backwards in time via the theory's concept of spiral time. This mechanism naturally explains the flare's anomalous properties—its extreme intensity, short duration, and 'clean' signature—without requiring any new particles.

Crucially, this model offers a testable prediction: such flares may not be random but could be preceded by smaller "pre-echoes," a signature that can be searched for in astronomical data. I invite you to read the paper and discuss this new perspective on black hole dynamics and the nature of time.