Did rapid spin delay 2017 collapse of merged neutron stars into black hole? Excess X-ray emissions from remnant four years after merger hint at bounce from delayed collapse — ScienceDaily


When two neutron stars spiral into each other and merge to kind a black gap — an occasion recorded in 2017 by gravitational wave detectors and telescopes worldwide — does it instantly turn out to be a black gap? Or does it take some time to spin down earlier than gravitationally collapsing previous the occasion horizon right into a black gap?

Ongoing observations of that 2017 merger by the Chandra X-ray Observatory, an orbiting telescope, suggests the latter: that the merged object caught round, doubtless for a mere second, earlier than present process final collapse.

The proof is within the type of an X-ray afterglow from the merger, dubbed GW170817, that may not be anticipated if the merged neutron stars collapsed instantly to a black gap. The afterglow might be defined as a rebound of fabric off the merged neutron stars, which plowed via and heated the fabric across the binary neutron stars. This scorching materials has now saved the remnant glowing steadily greater than 4 years after the merger threw materials outward in what’s known as a kilonova. X-ray emissions from a jet of fabric that was detected by Chandra shortly after the merger would in any other case be dimming by now.

Whereas the surplus X-ray emissions noticed by Chandra may come from particles in an accretion disk swirling round and ultimately falling into the black gap, astrophysicist Raffaella Margutti of the College of California, Berkeley, favors the delayed collapse speculation, which is predicted theoretically.

“If the merged neutron stars have been to break down on to a black gap with no intermediate stage, it could be very onerous to clarify this X-ray extra that we see proper now, as a result of there could be no onerous floor for stuff to bounce off and fly out at excessive velocities to create this afterglow,” stated Margutti, UC Berkeley affiliate professor of astronomy and of physics. “It will simply fall in. Performed. The true motive why I am excited scientifically is the likelihood that we’re seeing one thing greater than the jet. We would lastly get some details about the brand new compact object.”

Margutti and her colleagues, together with first writer Aprajita Hajela, who was Margutti’s graduate scholar when she was at Northwestern College earlier than shifting to UC Berkeley, report their evaluation of the X-ray afterglow in a paper lately accepted for publication in The Astrophysical Journal Letters.

The radioactive glow of a kilonova

Gravitational waves from the merger have been first detected on Aug. 17, 2017, by the Superior Laser Interferometer Gravitational-wave Observatory (LIGO) and the Virgo collaboration. Satellite tv for pc- and ground-based telescopes shortly adopted as much as file a burst of gamma rays and visual and infrared emissions that collectively confirmed the idea that many heavy components are produced within the aftermath of such mergers inside scorching ejecta that produces a brilliant kilonova. The kilonova glows due to gentle emitted in the course of the decay of radioactive components, like platinum and gold, which might be produced within the merger particles.

Chandra, too, pivoted to look at GW170817, however noticed no X-rays till 9 days later, suggesting that the merger additionally produced a slim jet of fabric that, upon colliding with the fabric across the neutron stars, emitted a cone of X-rays that originally missed Earth. Solely later did the top of the jet develop and start emitting X-rays in a broader jet seen from Earth.

The X-ray emissions from the jet elevated for 160 days after the merger, after which they steadily grew fainter because the jet slowed down and expanded. However Hajela and her group observed that from March 2020 — about 900 days after the merger — till the tip of 2020, the decline stopped, and the X-ray emissions remained roughly fixed in brightness.

“The truth that the X-rays stopped fading shortly was our greatest proof but that one thing along with a jet is being detected in X-rays on this supply,” Margutti stated. “A very completely different supply of X-rays seems to be wanted to clarify what we’re seeing.”

The researchers recommend that the surplus X-rays are produced by a shock wave distinct from the jets produced by the merger. This shock was a results of the delayed collapse of the merged neutron stars, doubtless as a result of its fast spin very briefly counteracted the gravitational collapse. By sticking round for an additional second, the fabric across the neutron stars received an additional bounce that produced a really quick tail of kilonova ejecta that created the shock.

“We predict the kilonova afterglow emission is produced by shocked materials within the circumbinary medium,” Margutti stated. “It’s materials that was within the surroundings of the 2 neutron stars that was shocked and heated up by the quickest fringe of the kilonova ejecta, which is driving the shock wave.”

The radiation is reaching us solely now as a result of it took time for the heavy kilonova ejecta to be decelerated within the low-density surroundings and for the kinetic vitality of the ejecta to be transformed into warmth by shocks, she stated. This is identical course of that produces radio and X-rays for the jet, however as a result of the jet is way, a lot lighter, it’s instantly decelerated by the surroundings and shines within the X-ray and radio from the very earliest occasions.

An alternate clarification, the researchers observe, is that the X-rays come from materials falling in direction of the black gap that fashioned after the neutron stars merged.

“This could both be the primary time we have seen a kilonova afterglow or the primary time we have seen materials falling onto a black gap after a neutron star merger,” stated co-author Joe Vivid, a UC Berkeley postdoctoral researcher. “Both end result could be extraordinarily thrilling.”

Chandra is now the one observatory nonetheless capable of detect gentle from this cosmic collision. Comply with-up observations by Chandra and radio telescopes may distinguish between the choice explanations, nonetheless. If it’s a kilonova afterglow, radio emission is anticipated to be detected once more within the subsequent few months or years. If the X-rays are being produced by matter falling onto a newly fashioned black gap, then the X-ray output ought to keep regular or decline quickly, and no radio emission will likely be detected over time.

Margutti hopes that LIGO, Virgo and different telescopes will seize gravitational waves and electromagnetic waves from extra neutron star mergers in order that the collection of occasions previous and following the merger might be pinned down extra exactly and assist reveal the physics of black gap formation. Till then, GW170817 is the one instance out there for research.

“Additional research of GW170817 may have far-reaching implications,” stated co-author Kate Alexander, a postdoctoral researcher who is also from Northwestern College. “The detection of a kilonova afterglow would suggest that the merger didn’t instantly produce a black gap. Alternatively, this object might provide astronomers an opportunity to check how matter falls onto a black gap a number of years after its beginning.”

Margutti and her group lately introduced that the Chandra telescope had detected X-rays in observations of GW170817 carried out in December 2021. Evaluation of that knowledge is ongoing. No radio detection related to the X-rays has been reported.

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