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X-ray Thunder After Gamma-ray Lightning ⚡ экспресс

Original: "Minutes-long soft X-ray prompt emission from a compact object merger"
arXiv:2601.14137 · 2026-01-20 · CC BY · ⏱ 1 min · High Energy
The Einstein Probe telescope captured for the first time a long X-ray 'echo' after an instant gamma-ray burst — like thunder after lightning.
Abstract

Like thunder follows lightning, a short gamma-ray burst (a powerful cosmic explosion) was trailed by a long, nearly ten-minute X-ray flare. This hints that long-lasting X-ray glow might be business as usual when neutron stars collide. Such flares will help us snag gravitational waves – the ripples in space-time. Does that mean every short gamma-ray burst has a stealthy 'tail' we’ve been missing?

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The Einstein Probe space telescope detected a celestial storm: after a short (0.4-second) gamma-ray burst — a cosmic lightning bolt — came a long roll of X-ray thunder. It lasted nearly 10 minutes. This is the first direct proof that such explosions leave a lingering X-ray afterglow. These events are caused by collisions of neutron stars or black holes. The impact produces an instantaneous gamma-ray flash, and then the crash site continues to emit soft X-rays for a long time. This tail not only tells us about the merger details — it helps locate the source, even after the gravitational waves, the tremors of space, have subsided. But the biggest surprise is the power. In those same 10 minutes, this X-ray echo releases as much energy as hundreds of billions of Suns shining at once.

🎯 In 10 minutes, this X-ray signal releases energy equivalent to the luminosity of hundreds of billions of Suns.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
gravitational waves neutron star black hole
Laws
Hawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsFermi–Dirac statisticsChandrasekhar limit
Original: arXiv:2601.14137 · CC BY · bridge42worlds