To investigate, Adams and his team used a mathematical duality between Einstein's theory of general relativity — which describes
gravity near black holes — and fluid dynamics.
Not exact matches
As the
black holes drew
near in a deepening pit of spacetime, they also churned up that fabric, emitting gravitational radiation (or
gravity waves, as scientists often call them).
Flashes of X-ray light
near the center of the disk result in light echoes that allow astronomers to map the structure of the funnel - like flow, revealing for the first time strong
gravity effects around a normally quiescent
black hole.
But something special occurs when pairs of particles emerge
near the event horizon — the boundary between a
black hole, whose
gravity is so strong that it warps space - time, and the rest of the Universe.
This behavior aligns with Albert Einstein's predictions about extreme
gravity near rotating
black holes, published in his famous theory of general relativity.
This particular energy range offers astronomers a detailed look at what is happening
near the event horizon, the region around a
black hole from which light can no longer escape
gravity's grasp.
Related sites Abstract of paper, with link to full text A primer on strong
gravity, including light
near a
black hole
A century later, that insight underpins cutting - edge physics: searching for gravitational waves, probing the extreme
gravity near the supermassive
black hole at the center of our galaxy, tracing the origin of the universe.
By some estimates, the telescope could be used to image
near the
black hole's event horizon — the boundary around which nothing can escape the
black hole's
gravity.
The team led by three principal investigators, Heino Falcke, Radboud University Nijmegen, Michael Kramer, Max - Planck - Institut für Radioastronomie, and Luciano Rezzolla, Goethe University in Frankfurt and Max - Planck - Institut für Gravitationsphysik, Potsdam, hopes to measure the shadow cast by the event horizon of the
black hole in the center of the Milky Way, find new radiopulsars
near this
black hole, and combine these measurements with advanced computer simulations of the behaviour of light and matter around
black holes as predicted by theories of
gravity.