While there are lots of theories about black holes, a staple of singularity lore is that all black holes have event horizons — a one-way membrane through which particles fall in, never to return. Einstein’s theory of general relativity says that all black holes have an event horizon where nothing, not even light, can escape the gravitational pull of these extremely dense objects.
But some have cast doubt about the existence of these event horizons. Stephen Hawking, one of the architects of modern black hole theory, wrote a paper in 2014 arguing that event horizons are incompatible with quantum theory. He instead proposed a more benign “apparent horizon,” which only temporarily holds matter and energy.
This artist’s impression shows a star crossing the event horizon of a supermassive black hole located in the center of a galaxy.
Credit: Mark A. Garlick/CfA
Another proposed alternative to event horizons is the “hard surface theory,” which suggests that matter within a black hole is destroyed by smashing into a solid surface. Instead of a singularity with no surface area, the black hole is a giant mass with a hard surface, and material being pulled closer — such as a star — would not actually fall into a black hole, but hit this hard surface and be destroyed. If that were the case, the collision should create a large burst of light.
But if event horizons do exist, there wouldn’t be flash of light. Instead, matter would just completely vanish when pulled in.
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This is the first in a sequence of two artist’s impressions that shows a huge, massive sphere in the center of a galaxy, rather than a supermassive black hole. Here a star moves towards and then smashes into the hard surface of the sphere, flinging out debris. The impact heats up the site of the collision.
Credit: Mark A. Garlick/CfA
There are two possible ways to test the event horizon theory versus the hard surface theory. One is direct imaging of a black hole, and astronomers hope to do just that with the Event Horizon Telescope , a powerful array of telescopes around the world that is currently making observations of two supermassive black holes.
But a group of astronomers at the University of Texas at Austin and Harvard University didn’t want to wait for the Event Horizon Telescope data, and used another method to assess this basic principle of black holes. They say that their results, which they describe in a paper published in the journal Monthly Notices of the Royal Astronomical Society, constitute another successful validation of Einstein’s theory.
“Our whole point here is to turn this idea of an event horizon into an experimental science, and find out if event horizons really do exist or not,” said Pawan Kumar, a professor of astrophysics at the University of Texas at Austin, in a statement . “Our motive is not so much to establish that there is a hard surface, but to push the boundary of knowledge and find concrete evidence that, really, there is an event horizon around black holes.”
In this second artist’s impression a huge sphere in the center of a galaxy is shown after a star has collided with it. Enormous amounts of heat and a dramatic increase in the brightness of the sphere are generated by this event. The lack of observation of such flares from the center of galaxies means that this hypothetical scenario is almost completely ruled out.
Credit: Mark A. Garlick/CfA
See how black holes work in this SPACE.com infographic
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Kumar, graduate student Wenbin Lu, and Ramesh Narayan, a theorist from the Harvard-Smithsonian Center for Astrophysics, figured out what a telescope would see when a star hit the hard surface of a supermassive object at the center of a nearby galaxy: The star’s gas would envelope the object, shining for months, maybe even years.
When they knew what to look for, the researchers estimated the rate at which stars fall into supermassive black holes to figure out how often this flash of light should be visible.
“We estimated the rate of stars falling onto supermassive black holes,” Lu said. “Nearly every galaxy has one. We only considered the most massive ones, which weigh about 100 million solar masses or more. There are about a million of them within a few billion light-years of Earth.”
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The team looked at archival data from the 1.8 meter Pan-STARRS telescope in Hawaii, which had recently completed a three-year project to survey half of the northern hemisphere sky while searching for “transients” — distant bursts of light that glow for a while and then fade. Their goal was to find transients with the expected light signature of a star falling toward a supermassive object and hitting a hard surface.
“Given the rate of stars falling onto black holes and the number density of black holes in the nearby universe, we calculated how many such transients Pan-STARRS should have detected over a period of operation of 3.5 years,”Lu said. “It turns out it should have detected more than 10 of them, if the hard-surface theory is true.”
But they found… nothing. No object displayed the expected light signature that would show evidence of the hard surface theory. The team says this non-finding helps demonstrate that event horizons are real, and that matter completely vanishes when pulled into a black hole.
“Our work implies that some, and perhaps all, black holes have event horizons, and that material really does disappear from the observable universe when pulled into these exotic objects, as we’ve expected for decades,”Narayan said. “General Relativity has passed another critical test.”
Of course, no researcher is satisfied with one test. The team hopes to continue its research with an even larger telescope: the 8.4-meter Large Synoptic Survey Telescope (LSST), which is currently under construction in Chile. Like Pan-STARRS, LSST will make repeated surveys of the sky over time, revealing transients with much greater sensitivity.
But in the meantime, keep an eye out for results from the Event Horizon Telescope later this year.
Originally published on Seeker .
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