24/7 Space News
First observational evidence linking black holes to dark energy
Measurement of coupling strength k by comparing black hole masses in 5 different collections of ancient elliptical galaxies to the black holes in elliptical galaxies today. Measurements cluster around k = 3, implying that black holes contain vacuum energy, instead of a singularity.
First observational evidence linking black holes to dark energy
by Staff Writers
Honolulu HI (SPX) Feb 16, 2023

Searching through existing data spanning 9 billion years, a team of researchers led by scientists at University of Hawai?i at Manoa has uncovered the first evidence of "cosmological coupling" -a newly predicted phenomenon in Einstein's theory of gravity, possible only when black holes are placed inside an evolving universe.

Astrophysicists Duncan Farrah and Kevin Croker led this ambitious study, combining Hawai?i's expertise in galaxy evolution and gravity theory with the observation and analysis experience of researchers across nine countries to provide the first insight into what might exist inside real black holes.

"When LIGO heard the first pair of black holes merge in late 2015, everything changed," said Croker. "The signal was in excellent agreement with predictions on paper, but extending those predictions to millions, or billions of years? Matching that model of black holes to our expanding universe? It wasn't at all clear how to do that."

The team has recently published two papers, one in The Astrophysical Journal and the other in The Astrophysical Journal Letters, that studied supermassive black holes at the hearts of ancient and dormant galaxies.

The first paper found that these black holes gain mass over billions of years in a way that can't easily be explained by standard galaxy and black hole processes, such as mergers or accretion of gas.

The second paper finds that the growth in mass of these black holes matches predictions for black holes that not only cosmologically couple, but also enclose vacuum energy-material that results from squeezing matter as much as possible without breaking Einstein's equations, thus avoiding a singularity.

With singularities absent, the paper then shows that the combined vacuum energy of black holes produced in the deaths of the universe's first stars agrees with the measured quantity of dark energy in our universe.

"We're really saying two things at once: that there's evidence the typical black hole solutions don't work for you on a long, long timescale, and we have the first proposed astrophysical source for dark energy,'' said Farrah, lead author of both papers.

"What that means, though, is not that other people haven't proposed sources for dark energy, but this is the first observational paper where we're not adding anything new to the universe as a source for dark energy: black holes in Einstein's theory of gravity are the dark energy.''

These new measurements, if supported by further evidence, will redefine our understanding of what a black hole is.

Nine billion years ago
In the first study, the team determined how to use existing measurements of black holes to search for cosmological coupling.

"My interest in this project was really born from a general interest in trying to determine observational evidence that supports a model for black holes that works regardless of how long you look at them," Farrah said. "That's a very, very difficult thing to do in general, because black holes are incredibly small, they're incredibly difficult to observe directly, and they are a long, long way away."

Black holes are also hard to observe over long timescales. Observations can be made over a few seconds, or tens of years at most-not enough time to detect how a black hole might change throughout the lifetime of the universe. To see how black holes change over a scale of billions of years is a bigger task.

"You would have to identify a population of black holes and identify their distribution of mass billions of years ago. Then you would have to see the same population, or an ancestrally connected population, at present day and again be able to measure their mass," said co-author Gregory Tarle, a physicist at University of Michigan. "That's a really difficult thing to do."

Because galaxies can have life spans of billions of years, and most galaxies contain a supermassive black hole, the team realized that galaxies held the key, but choosing the right types of galaxy was essential.

"There were many different behaviors for black holes in galaxies measured in the literature, and there wasn't really any consensus," said study co-author Sara Petty, a galaxy expert at NorthWest Research Associates. "We decided that by focusing only on black holes in passively evolving elliptical galaxies, we could help to sort this thing out."

Elliptical galaxies are enormous and formed early. They are fossils of galaxy assembly. Astronomers believe them to be the final result of galaxy collisions, enormous in size with upwards of trillions of old stars.

By looking at only elliptical galaxies with no recent activity, the team could argue that any changes in the galaxies' black hole masses couldn't easily be caused by other known processes. Using these populations, the team then examined how the mass of their central black holes changed throughout the past 9 billion years.

If mass growth of black holes only occurred through accretion or merger, then the masses of these black holes would not be expected to change much at all. However if black holes gain mass by coupling to the expanding universe, then these passively evolving elliptical galaxies might reveal this phenomenon.

The researchers found that the further back in time they looked, the smaller the black holes were in mass, relative to their masses today. These changes were big: The black holes were anywhere from 7 to 20 times larger today than they were 9 billion years ago-big enough that the researchers suspected cosmological coupling could be the culprit.

Unlocking black holes
In the second study, the team investigated whether the growth in black holes measured in the first study could be explained by cosmological coupling alone.

"Here's a toy analogy. You can think of a coupled black hole like a rubber band, being stretched along with the universe as it expands," said Croker. "As it stretches, its energy increases. Einstein's E = mc2 tells you that mass and energy are proportional, so the black hole mass increases, too."

How much the mass increases depends on the coupling strength, a variable the researchers call k.

"The stiffer the rubber band, the harder it is to stretch, so the more energy when stretched. In a nutshell, that's k," Croker said.

Because mass growth of black holes from cosmological coupling depends on the size of the universe, and the universe was smaller in the past, the black holes in the first study must be less massive by the correct amount in order for the cosmological coupling explanation to work.

The team examined five different black hole populations in three different collections of elliptical galaxies, taken from when the universe was roughly one half and one third of its present size. In each comparison, they measured that k was nearly positive 3.

The first observational link
In 2019, this value was predicted for black holes that contain vacuum energy, instead of a singularity by Croker, then a graduate student, and Joel Weiner, a UH Manoa mathematics professor.

The conclusion is profound: Croker and Weiner had already shown that if k is 3, then all black holes in the universe collectively contribute a nearly constant dark energy density, just like measurements of dark energy suggest.

Black holes come from dead large stars, so if you know how many large stars you are making, you can estimate how many black holes you are making and how much they grow as a result of cosmological coupling. The team used the very latest measurements of the rate of earliest star formation provided by the James Webb Space Telescope and found that the numbers line up.

According to the researchers, their studies provide a framework for theoretical physicists and astronomers to further test-and for the current generation of dark energy experiments such as the Dark Energy Spectroscopic Instrument and the Dark Energy Survey-to shed light on the idea.

"If confirmed this would be a remarkable result, pointing the way towards the next generation of black hole solutions," said Farrah.

Croker added, "This measurement, explaining why the universe is accelerating now, gives a beautiful glimpse into the real strength of Einstein's gravity. A chorus of tiny voices spread throughout the universe can work together to steer the entire cosmos. How cool is that?"

Research Report:Observational evidence for cosmological coupling of black holes and its implications for an astrophysical source of dark energy

Related Links
University of Hawaii at Manoa
Stellar Chemistry, The Universe And All Within It

Subscribe Free To Our Daily Newsletters

The following news reports may link to other Space Media Network websites.
A new model for dark matter
Ann Arbor MI (SPX) Jan 24, 2023
Dark matter remains one of the greatest mysteries of modern physics. It is clear that it must exist, because without dark matter, for example, the motion of galaxies cannot be explained. But it has never been possible to detect dark matter in an experiment. Currently, there are many proposals for new experiments: They aim to detect dark matter directly via its scattering from the constituents of the atomic nuclei of a detection medium, i.e., protons and neutrons. A team of researchers-Robert ... read more

Roscosmos is delaying the launch of the replacement Soyuz for crew return

NASA, partners clear Axiom's second private astronaut mission crew

Spacecraft controllers aim for the heights

NASA launches new Framework for Procurement Ideas, Solutions

Japan's H3 rocket fails to leave the launch pad

The roar and crackle of Artemis 1

Russian Progress cargo craft docks at space station suffers loss of coolant

NASA conducts first 2023 test of redesigned SLS rocket engine

Study quantifies global impact of electricity in dust storms on Mars

Complex subsurface of Mars imaged by Chinese rover Zhurong

Perseverance shows off collection of Mars samples

Cloud gazing while we get ready to drill: Sols 3739-3741

China's space station experiments pave way for new space technology

Large number of launches planned

Chinese astronauts complete first walk outside Tiangong space station

Shenzhou XV astronauts take their first spacewalk

SpaceX launches 55 Starlink satellites early Sunday morning

FCC greenlights Amazon's Project Kuiper to deploy 3,236 satellites in LEO

Women and girls in science: the team helping to take us to Mars

AccelerComm, TTP set to soar with 5G NTN LEO Space Cell

'Magic' solvent creates stronger thin films

Space Station research announcement for advanced materials and manufacturing open now

Astroscale wins Dstl funding for exploration of future Space-Based Space Domain Awareness missions

Sidius Space reaches an agreement with a Dutch organization to Deploy Lasercom Mission

Four classes of planetary systems

Team Aims To Find Earth 2.0

New models shed light on life's origin

Researchers focus AI on finding exoplanets

JUICE's final take-off before lift-off

A new ring system discovered in our Solar System

SwRI models explain canyons on Pluto moon

NASA's Juno Team assessing camera after 48th flyby of Jupiter

Subscribe Free To Our Daily Newsletters


The content herein, unless otherwise known to be public domain, are Copyright 1995-2023 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.