Northwestern University researchers have identified stellar cocoons as a potential new source of gravitational waves. Simulations show that these turbulent, energetic structures form around collapsing stars and create ripples in space-time. Unlike supernovae or gamma-ray bursts, cocoons generate asymmetrical waves detectable by LIGO, opening a new frontier in gravitational wave astronomy.
So far, gravitational waves have been only detected by astrophysicists from binary systems – the fusion of either two black holes, two neutron stars, or one of each. In theory, it should be possible to detect gravitational waves emanating from a solitary, non-binary source, but such elusive signals have yet to be discovered.
Researchers from Northwestern University now propose that these elusive signals could be sought in a novel, unexpected, and entirely unexplored area: The turbulent, energetic cocoons of debris that surround dying massive stars.
For the first time ever, the researchers have used state-of-the-art simulations to show that these cocoons can emit gravitational waves. And, unlike gamma-ray burst jets, cocoons’ gravitational waves should be within the frequency band that the Laser Interferometer Gravitational-Wave Observatory (LIGO) can detect.
“As of today, LIGO has only detected gravitational waves from binary systems, but one day it will detect the first non-binary source of gravitational waves,” said Northwestern’s Ore Gottlieb, who led the study. “Cocoons are one of the first places we should look to for this type of source.”
Gottlieb recently presented the research during a virtual press briefing at the 242nd meeting of the American Astronomical Society.
The New Source Was ‘Impossible To Ignore’
To conduct the study, Gottlieb and his collaborators used new state-of-the-art simulations to model the collapse of a massive star. When massive stars collapse into black holes, they may create powerful outflows (or jets) of particles traveling close to the speed of light. Gottlieb’s simulations modeled this process — from the time the star collapses into a black hole until the jet escapes.
Initially, he wanted to see whether or not the accretion disk that forms around a black hole could emit detectable gravitational waves. But something unexpected kept emerging from his data.
The jet-cocoon evolution from birth by the black hole to breakout from the star (colormap is the logarithm of the off-axis strain amplitude and the sound reflects the GW frequency). Credit: Ore Gottlieb/CIERA/Northwestern University
“When I calculated the gravitational waves from the vicinity of the black hole, I found another source disrupting my calculations — the cocoon,” Gottlieb said. “I tried to ignore it. But I found it was impossible to ignore. Then I realized the cocoon was an interesting gravitational wave source.”
As jets collide into collapsing layers of the dying star, a bubble, or a “cocoon,” forms around the jet. Cocoons are turbulent places, where hot gases and debris mix randomly and expand in all directions from the jet. As the energetic bubble accelerates from the jet, it perturbs space-time to create a ripple of gravitational waves, Gottlieb explained.
“A jet starts deep inside of a star and then drills its way out to escape,” Gottlieb said. “It’s like when you drill a hole into a wall. The spinning drill bit hits the wall and debris spills out of the wall. The drill bit gives that material energy. Similarly, the jet punches through the star, causing the star’s material to heat up and spill out. This debris forms the hot layers of a cocoon.”
Call to Action To Look at Cocoons
If cocoons do generate gravitational waves, then LIGO should be able to detect them in its upcoming runs, Gottlieb said. Researchers have typically searched for single-source gravitational waves from gamma-ray bursts or supernovae, but astrophysicists doubt that LIGO could detect those.
“Both jets and supernovae are very energetic explosions,” Gottlieb said. “But we can only detect gravitational waves from a higher frequency, asymmetrical explosions. Supernovae are rather spherical and symmetrical, so spherical explosions do not change the balanced mass distribution in the star to emit gravitational waves. Gamma-ray bursts last dozens of seconds, so the frequency is very small — lower than the frequency band that LIGO is sensitive to.”
360-degree view of the dying star’s cocoon (colormap is the logarithmic strain amplitude). Credit: Ore Gottlieb/CIERA/Northwestern University
Instead, Gottlieb asks astrophysicists to redirect their attention to cocoons, which are both asymmetrical and highly energetic.
“Our study is a call to action to the community to look at cocoons as a source of gravitational waves,” he said. “We also know cocoons emit electromagnetic radiation, so they could be multi-messenger events. By studying them, we could learn more about what happens in the innermost part of stars, the properties of jets, and their prevalence in stellar explosions.”
Reference: “Jetted and Turbulent Stellar Deaths: New LVK-detectable Gravitational-wave Sources” by Ore Gottlieb, Hiroki Nagakura, Alexander Tchekhovskoy, Priyamvada Natarajan, Enrico Ramirez-Ruiz, Sharan Banagiri, Jonatan Jacquemin-Ide, Nick Kaaz and Vicky Kalogera, 10 July 2023, The Astrophysical Journal Letters.
DOI: 10.3847/2041-8213/ace03a
Gottlieb is a CIERA Fellow at Northwestern’s Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA). Northwestern co-authors of the study include professors Vicky Kalogera and Alexander Tchekovskoy, postdoctoral associates Sharan Banagiri and Jonatan Jacquemin-Ide and graduate student Nick Kaaz.
The study was supported by the National Science Foundation, NASA, and the Fermi Cycle 14 Guest Investigator program. These advanced simulations were made possible by the Department of Energy’s Oak Ridge National Laboratory supercomputer Summit and National Energy Research Scientific Computing Center’s supercomputer Perlmutter through the ASCR Leadership Computing Challenge computational time award.
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