The information locked inside black holes could be detected by feeling their 'hair,' new research suggests.
Black holes are celestial objects with such massive gravity that not even light can escape their clutches once it crosses the event horizon, or point-of-no-return. The event horizons of black holes lock secrets deep within them — secrets that could completely revolutionize our understanding of physics.
Unfortunately, for decades many scientists thought whatever information falls into a black hole might be lost forever. But new research suggests that ripples in space-time, or gravitational waves may carry a faint whisper of this hidden information by revealing the presence of wispy "hairs" on a black hole's surface.
A hairy question?
As far as we understand them (which, admittedly, is not very much), black holes are suspiciously simple objects. Regardless of what falls in, whether stars, clouds of gas and dust, or your worst enemies, black holes can be described by three and only three simple numbers: charge, mass and spin.
That means that if you had two black holes of the exact same size, exact same electric charge, and spinning at exactly the same rate, you wouldn't be able to tell them apart. The reason this is suspicious is that something had to happen to all that juicy information that fell into those two black holes. Did it get destroyed? Lost below the event horizon? Stuck in some inaccessible portion of the universe?
The simplest solution is the theorem, first coined by the American physicist John Wheeler, that "black holes have no hair" — they have no extra information encoded in them or on them. Just their mass, electric charge and spin. Everything else is simply destroyed (somehow) beyond the event horizon, locked away from the universe forever and ever.
A paradox of information
But in 1974, Stephen Hawking proposed a revolutionary idea: black holes aren't inescapable cosmic vacuum cleaners; rather, subatomic particles might flee black holes through an exotic quantum process, which would result in the release of radiation from their surfaces. Over time, this Hawking radiation, as it is called, would cause black holes to slowly lose energy (and therefore mass). Eventually, after eons of gradually losing energy, the black holes would evaporate entirely.
This is all fine and dandy, except for the pesky no-hair idea. If black holes can evaporate, what happens to all the information that fell into them?
As far as we know, Hawking radiation doesn't carry any information away with it. And we really, really don't think that information can be created or destroyed in this universe (it's certainly possible, but would make a bunch of known physics pretty wonky, which would violate observations and experiments).
And hence, the black hole information paradox. Information goes into a black hole, the black hole disappears, and we don't know what happens to the information.
To fix this paradox, either we need to fix what we know about black holes or fix what we know about Hawking radiation. Or both.
Maybe the information gets locked deep inside the black hole, near the singularity, and evaporation stops just before that point, leaving behind a tiny little ball chock full of information.
Or maybe black holes aren't entirely hairless. Maybe, just maybe, they maintain the information of anything that's fallen into them on their surfaces, contained in something called the "stretched horizon", a surface just above the event horizon containing quantum mechanical information. As black holes dissolve, the Hawking radiation carries away the information contained in the stretched horizon, solving the paradox and preserving our reality as we know it.
Great idea, but how do we test it?
Ripples in space-time
A new study, published June 22 to the arXiv database (but not yet peer reviewed), suggests one way to find these silky strands: a gravitational wave detection.
When black holes merge, they release a fury of gravitational waves that ripple throughout the cosmos. Despite the incredible energies of these collisions, the gravitational waves from these cosmic smashups are exceptionally weak. By the time these waves wash over Earth, they're barely capable of nudging individual atoms.
But we have LIGO — the Laser Interferometer Gravitational-Wave Observatory, a globe-spanning observatory — which can detect those subtle motions through the tiny changes in how long it takes light to travel from far-flung detectors. LIGO has observed the aftermath of dozens of potential black hole collisions throughout the universe, which even led to a Nobel Prize award in 2017. So far, those observations are consistent with the "no-hair theorem," suggesting there is no extra information encoded on the surfaces of black holes.
But there's still a chance. There could be "soft hair" on the black holes — just a little bit of information, structured in a way that is challenging to detect.
Of course physicists want to test this idea, because if we could demonstrate that black holes have hair, we would not only solve a major riddle in modern physics, but likely pave the way toward a better understanding of quantum gravity, or the theory that would reconcile general relativity, which governs the universe on a large scale, with quantum mechanics, which describes reality on the tiniest scales.Now comes the real hard work of science: connecting neat ideas to actual observation. The new arXiv paper suggests a way to find these soft hairs. The new study authors, Lawrence Crowell of the Alpha Institute for Advanced Studies in Budapest, Hungary and Christian Corda, a physicist at Istanbul University in Turkey, discovered that during the merging process, normally-quiet hairs can get excited, so to speak. In this energized state,, these hairs would intertwine with the outgoing gravitational radiation, altering those waves in subtle ways.
Those changes to the gravitational waves can't be detected yet, but future versions of LIGO might have the sensitivity to do it. And then we might be able to finally tell whether black holes are hairy or not.
Originally published in Live Science.
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Paul M. Sutter is an astrophysicist at SUNY Stony Brook and the Flatiron Institute in New York City. Paul received his PhD in Physics from the University of Illinois at Urbana-Champaign in 2011, and spent three years at the Paris Institute of Astrophysics, followed by a research fellowship in Trieste, Italy, His research focuses on many diverse topics, from the emptiest regions of the universe to the earliest moments of the Big Bang to the hunt for the first stars. As an "Agent to the Stars," Paul has passionately engaged the public in science outreach for several years. He is the host of the popular "Ask a Spaceman!" podcast, author of "Your Place in the Universe" and "How to Die in Space" and he frequently appears on TV — including on The Weather Channel, for which he serves as Official Space Specialist.
Gravity is at once a mirror; another form of duality. As I see it, the weaker the gravity the more ghostly the mirror and the stronger the gravity the more real the mirror mirroring information, including, of course, matter and energy. Ultimately, you might say, a constant of Big Bang energy from a constant of Big Crunch mass, but in lesser dimension still the same principle. It would be instantly quicker, and I mean quicker, than any other means of putting back what was coming to; of reversing the direction of flow to nowhere.Reply
It doesn't necessarily have to be to the local area, or local plain, or local dimension, of the blackhole either. It could be something similar to "spooky action at a distance" (...teleportation elsewhere...many elsewheres? Transformation or translation to new information? Come to think of it, such might be neutral, new and old; primordial, available for work. An infinite Universe || infinite mass Big Crunch / infinitesimal mass Big Hole never really losing nor gaining?). But then again, such transformation, translation, or travel, might be " the looking glass" of the black to somewhere else, or everywhere else, anyway. Same thing, different exit.
Existence is eternal. We are here, surrounded by matter and order because no process has ever destroyed it. Including black holes or heat deaths in previous big bang contents. Order even survived coming through our Big Bang. Order can't be created or destroyed. This all goes to show that one day all that went into black holes will come out again, both matter and order.:)Admin said:Hair may record the information swallowed by the gravitational monsters.
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