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Radio signal discovered at the center of our galaxy could put Einstein's relativity to the test
Scientists hope to probe the nature of general relativity through a possible pulsar found in the center of the Milky Way, ...
Researchers from Columbia University and Breakthrough Listen, a scientific research program aimed at finding evidence of ...
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Unique pulsar may be orbiting our galaxy's supermassive black hole, posing an incredible test for Einstein’s relativity
Pulsars are a special class of neutron stars that spin very quickly on their axes, releasing pulses of radio waves. These ...
General relativity helps explain the lack of planets around tight binary stars by driving orbital resonances that eject or destroy close-in worlds. This process naturally creates a “desert” of ...
For those who watch gravitational waves roll in from the universe, GW250114 is a big one. It's the clearest gravitational ...
Ripples in space-time from a pair of merging black holes have been recorded in unprecedented detail, enabling physicists to test predictions of general relativity ...
One such mystery, described in a recent paper in The Astrophysical Journal Letters, concerns circumbinary exoplanets—or rather, the shortage thereof—in the now 6,000+ exoplanets confirmed to date.
The sharpest black hole collision ever detected just gave Einstein another win—and raised hopes that the next one might ...
Learn why only 14 out of over 6,000 exoplanets orbit two stars, and how Einstein’s general theory of relativity may be to blame.
Add Yahoo as a preferred source to see more of our stories on Google. A illustration shows a quantum experiment investigating gravity on a tiny scale. Scientists have determined a way to measure ...
A newly detected gravitational wave, GW250114, is giving scientists their clearest look yet at a black hole collision—and a powerful way to test Einstein’s theory of gravity. Its clarity allowed ...
LIGO's GW250114 signal tests Einstein's relativity, revealing black hole properties and confirming key theorems in ...
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