Possible dark matter hint detected in gravitational wave

Physicists have found a potential signature of dark matter in data from a black hole merger observed in 2019. The signal known as GW190728 showed patterns consistent with the invisible substance interacting with the colliding objects. A new model developed by researchers at MIT and partner institutions made the analysis possible.

The team examined 28 clear gravitational wave events from the first three observing runs of the LIGO-Virgo-KAGRA network. Twenty-seven signals matched expectations for mergers in empty space, but GW190728 stood out. The researchers suggest the black holes may have passed through a dense dark matter cloud before colliding, altering the resulting spacetime ripples.

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Researchers propose that ancient gravitational waves in the early universe produced particles that became dark matter. The study by scientists from Johannes Gutenberg University Mainz and Swansea University suggests a new mechanism involving stochastic gravitational waves converting into fermions. Published in Physical Review Letters, the work addresses a key mystery in cosmology.

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Astronomers have uncovered evidence that a black hole and neutron star merged while following an unusual oval-shaped orbit, challenging expectations of circular paths in such events. The discovery comes from a reanalysis of gravitational wave data from the event known as GW200105. This finding suggests the system formed in a dynamic stellar environment.

Astronomers have discovered that the Milky Way resides within a vast, flat sheet of matter dominated by dark matter, surrounded by enormous empty voids. This structure explains why most nearby galaxies are moving away from our Local Group rather than being drawn in by gravity. The finding, based on advanced simulations, resolves a longstanding puzzle in cosmology.

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Astronomers have identified a bright supernova from over 10 billion years ago, its light gravitationally lensed into multiple images by a foreground galaxy. This unique observation allows simultaneous views of different stages of the explosion. The time delays between images could reveal details about the universe's expansion rate and dark energy.

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