From University of Arizona: “Einstein’s Description of Gravity Just Got Much Harder to Beat”

From University of Arizona

10.1.20

Dimitrios Psaltis
Department of Astronomy
dpsaltis@arizona.edu

Feryal Özel
Department of Astronomy
fozel@arizona.edu

Pierre Christian
Department of Astronomy
pchristian@arizona.edu

Media contact:
Mikayla Mace
University Communications
520-621-1878
mikaylamace@arizona.edu

Daniel Stolte
University Communications
520-626-4402
stolte@email.arizona.edu

Lee Sandberg
Institute for Advanced Study
609-455-4398
lsandberg@ias.edu

U Arizona researchers put general relativity to a new test with black hole images.

1
Simulation of M87 black hole showing the motion of plasma as it swirls around the black hole. The bright thin ring that can be seen in blue is the edge of what we call the black hole shadow. L. Medeiros; C. Chan; D. Psaltis; F. Özel; University of Arizona; Institute for Advanced Study.

2
Visualization of the new gauge developed to test the predictions of modified gravity theories against the measurement of the size of the M87 shadow. Credit: D. Psaltis, UArizona; EHT Collaboration.

Einstein’s theory of general relativity – the idea that gravity is matter warping spacetime – has withstood over 100 years of scrutiny and testing, including the newest test by University of Arizona astrophysicists from the Event Horizon Telescope collaboration.

According to their findings, Einstein’s theory just got 500 times harder to beat.

Despite its successes, Einstein’s robust theory remains mathematically irreconcilable with quantum mechanics, the scientific understanding of the subatomic world. Testing general relativity is important because the ultimate theory of the universe must encompass both gravity and quantum mechanics.

“We expect a complete theory of gravity to be different from general relativity, but there are many ways one can modify it. We found that whatever the correct theory is, it can’t be significantly different from general relativity when it comes to black holes. We really squeezed down the space of possible modifications,” said UArizona astronomy professor Dimitrios Psaltis, who until recently was the project scientist of the Event Horizon Telescope, or EHT, collaboration.

Psaltis is lead author of a new paper, published in Physical Review Letters, that details the researchers’ findings.

“This is a brand new way to test general relativity using supermassive black holes,” said Keiichi Asada, an EHT science council member and an expert on radio observations of black holes for Academia Sinica Institute of Astronomy and Astrophysics.

To perform the test, the team used the first image ever taken of the supermassive black hole at the center of nearby galaxy Messier 87 obtained with the EHT last year.

Messier 87*, The first image of a black hole. This is the supermassive black hole at the center of the galaxy Messier 87. Image via JPL/ Event Horizon Telescope Collaboration.

EHT map.

The first results had shown that the size of the black-hole shadow was consistent with the size predicted by general relativity.

“At that time, we were not able to ask the opposite question: How different can a gravity theory be from general relativity and still be consistent with the shadow size?” said UArizona Steward Theory Fellow Pierre Christian. “We wondered if there was anything we could do with these observations in order to cull some of the alternatives.”

The team did a very broad analysis of many modifications to the theory of general relativity to identify the unique characteristic of a theory of gravity that determines the size of a black hole shadow.

“In this way, we can now pinpoint whether any alternative to general relativity is in agreement with the Event Horizon Telescope observations, without worrying about any other details,” said Lia Medeiros, a postdoctoral fellow at the Institute for Advanced Study who has been part of the EHT collaboration since her time as a UArizona graduate student.

The team focused on the range of alternatives that had passed all the previous tests in the solar system.

“Using the gauge we developed, we showed that the measured size of the black hole shadow in M87 tightens the wiggle room for modifications to Einstein’s theory of general relativity by almost a factor of 500, compared to previous tests in the solar system,” said UArizona astronomy professor Feryal Özel, a senior member of the EHT collaboration. “Many ways to modify general relativity fail at this new and tighter black hole shadow test.”

“Black hole images provide a completely new angle for testing Einstein’s theory of general relativity,” said Michael Kramer, director of the Max Planck Institute for Radio Astronomy and EHT collaboration member.

“Together with gravitational wave observations, this marks the beginning of a new era in black hole astrophysics,” Psaltis said.

Testing the theory of gravity is an ongoing quest: Are the general relativity predictions for various astrophysical objects good enough for astrophysicists to not worry about any potential differences or modifications to general relativity?

“We always say general relativity passed all tests with flying colors – if I had a dime for every time I heard that,” Özel said. “But it is true, when you do certain tests, you don’t see that the results deviate from what general relativity predicts. What we’re saying is that while all of that is correct, for the first time we have a different gauge by which we can do a test that’s 500 times better, and that gauge is the shadow size of a black hole.”

Next, the EHT team expects higher fidelity images that will be captured by the expanded array of telescopes, which includes the Greenland Telescope and the 12-meter Telescope on Kitt Peak near Tucson and the Northern Extended Millimeter Array Observatory in France.

NSF CfA Greenland telescope, at the Summit Station research camp, located at the highest point of the Greenland ice sheet at an altitude of 3,210 meters (10,530 feet).

NRAO 12m Radio Telescope, Kitt Peak National Observatory, In the Arizona-Sonoran Desert on the Tohono O’odham Nation Arizona USA,Altitude 1,914 m (6,280 ft).

“When we obtain an image of the black hole at the center of our own galaxy, then we can constrain deviations from general relativity even further,” Özel said.

Will Einstein still be right, then?

See the full article here .


five-ways-keep-your-child-safe-school-shootings
Please help promote STEM in your local schools.

Stem Education Coalition

The University of Arizona (UA) is a place without limits-where teaching, research, service and innovation merge to improve lives in Arizona and beyond. We aren’t afraid to ask big questions, and find even better answers.

In 1885, establishing Arizona’s first university in the middle of the Sonoran Desert was a bold move. But our founders were fearless, and we have never lost that spirit. To this day, we’re revolutionizing the fields of space sciences, optics, biosciences, medicine, arts and humanities, business, technology transfer and many others. Since it was founded, the UA has grown to cover more than 380 acres in central Tucson, a rich breeding ground for discovery.

U Arizona mirror lab-Where else in the world can you find an astronomical observatory mirror lab under a football stadium?

University of Arizona’s Biosphere 2, located in the Sonoran desert. An entire ecosystem under a glass dome? Visit our campus, just once, and you’ll quickly understand why the UA is a university unlike any other.