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"Gravitational Waves May Have Been Deflected, Explaining 'Impossible' Black Hole Merger"

**SUMMARY:** A new study suggests that the merger of two massive black holes detected by LIGO may not have been as extraordinary as previously thought. Researchers propose that the gravitational wave...

SUMMARY:

A new study suggests that the merger of two massive black holes detected by LIGO may not have been as extraordinary as previously thought. Researchers propose that the gravitational wave signal was distorted by a massive object, making the black holes appear larger than they actually were.

CONTENT:

🚀 The Impossible Merger

On November 23, 2023, LIGO detected a gravitational wave signal, designated GW231123, which seemed to be the result of a black hole with 140 times the mass of the sun colliding with another holding 100 solar masses. This raised eyebrows among researchers, as usual models of stellar evolution struggle to account for such massive black holes.

🌐 Gravitational Lensing: The Key to Unlocking the Mystery

The team behind this new research suggests that the masses of these black holes were an illusion. They propose that the signal was deflected and distorted by a massive object, which warped the fabric of spacetime, making the black holes appear larger than they actually were. This phenomenon, known as gravitational lensing, was first predicted by Albert Einstein's theory of general relativity.

💡 The Science Behind Gravitational Lensing

Gravitational lensing occurs when light from a background object passes a massive foreground object. The foreground object can warp the fabric of spacetime, causing the light's path to be curved. This means light from the same background source can reach Earth at different times, depending on how much that light was diverted. The team believes that this effect also applies to gravitational waves, suggesting that the signal GW231123 is an example of gravitationally lensed ripples in spacetime.

🔍 The Research

To investigate this possibility, the team developed a mathematical model of gravitational lensing and created software powerful and fast enough to analyze it. They found that if they assume the signal was deflected and distorted by a compact object of about 190 to 850 solar masses, or by an extended structure such as a globular cluster, they can understand the observed high masses. Moreover, the lensing interpretation does not require unusually high spins.

📊 The Implications

The team's research points to the utility of gravitational wave astronomy to study some of the universe's most violent events. The discovery of gravitationally lensed gravitational wave signals could provide new insights into the formation and evolution of massive black holes. However, the team acknowledges that the nature of the lens remains a major mystery and future work will be needed to establish whether such lenses can form or whether an ensemble of lighter objects, including stars, can explain this event.

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