Supermassive black hole binary mergers are among the most dramatic phenomena in the universe, Campanelli said.
“There are so many of them that they produce a huge gravitational-wave background hum that can now be observed and used to better understand the formation and evolution of the universe.”
“The NanoGrav’s breakthrough discovery provides strong support for what astronomers have been waiting to hear for many years-that the universe, since its earliest days, hosts a very large number of these supermassive binary mergers,” said RIT astrophysicist Manuela Campanelli, who was not part of this study but has been working for over a decade to model the electromagnetic signatures from these powerful mergers. International collaborations using telescopes in Europe, India, Australia, and China have independently reported similar results. The gravitational-wave signal was observed in 15 years of data acquired by the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) Physics Frontiers Center (PFC), a collaboration of more than 190 scientists from the United States and Canada who use pulsars to search for gravitational waves. Astrophysicists using large radio telescopes to observe a collection of cosmic clocks in our galaxy have found evidence for gravitational waves that oscillate with periods of years to decades, according to a set of papers published Thursday in The Astrophysical Journal Letters.
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