The dark matter map is derived from Hubble Space Telescope Frontier Fields data of a trio of galaxy clusters that act as cosmic magnifying glasses to peer into older, more distant parts of the universe, a phenomenon known as gravitational lensing.
"With the data of these three lensing clusters we have successfully mapped the granularity of dark matter within the clusters in exquisite detail," said Priyamvada Natarajan, astrophysicist at the Yale University in the US.
Scientists believe dark matter - theorised, unseen particles that neither reflect nor absorb light, but are able to exert gravity - may comprise 80 per cent of the matter in the universe.
Dark matter may explain the very nature of how galaxies form and how the universe is structured.
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Experiments at Yale and elsewhere are attempting to identify the dark matter particle; the leading candidates include axions and neutralinos.
Dark matter particles are thought to provide the unseen mass that is responsible for gravitational lensing, by bending light from distant galaxies.
This light bending produces systematic distortions in the shapes of galaxies viewed through the lens. Natarajan's group decoded the distortions to create the new dark matter map.
Significantly, the map closely matches computer simulations of dark matter theoretically predicted by the cold dark matter model; cold dark matter moves slowly compared to the speed of light, while hot dark matter moves faster.
The high-resolution simulations used in the study, known as the Illustris suite, mimic structure formation in the universe in the context of current accepted theory.
The findings appear in the journal Monthly Notices of the Royal Astronomical Society.
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