. | . |
Resolving the black hole 'fuzzball or wormhole' debate by Laura Arenschield for OSU News Columbus OH (SPX) Jan 05, 2022
Black holes really are giant fuzzballs, a new study says. The study attempts to put to rest the debate over Stephen Hawking's famous information paradox, the problem created by Hawking's conclusion that any data that enters a black hole can never leave. This conclusion accorded with the laws of thermodynamics, but opposed the fundamental laws of quantum mechanics. "What we found from string theory is that all the mass of a black hole is not getting sucked in to the center," said Samir Mathur, lead author of the study and professor of physics at The Ohio State University. "The black hole tries to squeeze things to a point, but then the particles get stretched into these strings, and the strings start to stretch and expand and it becomes this fuzzball that expands to fill up the entirety of the black hole." The study, published Dec. 28 in the Turkish Journal of Physics, found that string theory almost certainly holds the answer to Hawking's paradox, as the paper's authors had originally believed. The physicists proved theorems to show that the fuzzball theory remains the most likely solution for Hawking's information paradox. The researchers have also published an essay showing how this work may resolve longstanding puzzles in cosmology; the essay appeared in December in the International Journal of Modern Physics. Mathur published a study in 2004 that theorized black holes were similar to very large, very messy balls of yarn - "fuzzballs" that become larger and messier as new objects get sucked in. "The bigger the black hole, the more energy that goes in, and the bigger the fuzzball becomes," Mathur said. The 2004 study found that string theory, the physics theory that holds that all particles in the universe are made of tiny vibrating strings, could be the solution to Hawking's paradox. With this fuzzball structure, the hole radiates like any normal body, and there is no puzzle. After Mathur's 2004 study and other, similar works, "many people thought the problem was solved," he said. "But in fact, a section of people in the string theory community itself thought they would look for a different solution to Hawking's information paradox. They were bothered that, in physical terms, the whole structure of the black hole had changed." Studies in recent years attempted to reconcile Hawking's conclusions with the old picture of the hole, where one can think of the black hole as being "empty space with all its mass in the center." One theory, the wormhole paradigm, suggested that black holes might be one end of a bridge in the space-time continuum, meaning anything that entered a black hole might appear on the other end of the bridge - the other end of the wormhole - in a different place in space and time. In order for the wormhole picture to work, though, some low-energy radiation would have to escape from the black hole at its edges. This recent study proved a theorem - the "effective small corrections theorem" - to show that if that were to happen, black holes would not appear to radiate in the way that they do. The researchers also examined physical properties from black holes, including topology change in quantum gravity, to determine whether the wormhole paradigm would work. "In each of the versions that have been proposed for the wormhole approach, we found that the physics was not consistent," Mathur said. "The wormhole paradigm tries to argue that, in some way, you could still think of the black hole as being effectively empty with all the mass in the center. And the theorems we prove show that such a picture of the hole is not a possibility." Other Ohio State researchers who worked on this study include Madhur Mehta, Marcel R. R. Hughes and Bin Guo.
Research Report: "Contrasting the fuzzball and wormhole paradigms for black holes"
Astronomers capture black hole eruption spanning 16 times the full Moon in the sky Perth, Australia (SPX) Dec 27, 2021 Astronomers have produced the most comprehensive image of radio emission from the nearest actively feeding supermassive black hole to Earth. The emission is powered by a central black hole in the galaxy Centaurus A, about 12 million light years away. As the black hole feeds on in-falling gas, it ejects material at near light-speed, causing 'radio bubbles' to grow over hundreds of millions of years. When viewed from Earth, the eruption from Centaurus A now extends eight degrees across t ... read more
|
|
The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - 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. |