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Although astrophysicists theoretically should be able to detect gravitational waves from a single, non-binary source, they have yet to uncover these elusive signals. Now researchers suggest looking at a new, unexpected and entirely unexplored place: The turbulent, energetic cocoons of debris that surround dying massive stars.

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United States ,American ,Sharan Banagiri ,Vicky Kalogera ,Nick Kaaz ,Jonatan Jacquemin Ide ,Alexander Tchekovskoy ,American Astronomical Society ,Northwestern Center ,Department Of Energy Oak Ridge National Laboratory ,National Energy Research Scientific Computing Center ,Research In Astrophysics ,National Science Foundation ,Northwestern University ,Now Northwestern University ,Ore Gottlieb ,American Astronomical ,Distant Galaxies ,Interdisciplinary Exploration ,Fermi Cycle ,Oak Ridge National Laboratory ,Computing Challenge ,

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