A Scientist Thinks the Universe Bounced Out of a Black Hole
A new hypothesis from physicists at the University of Portsmouth in the U.K. challenges the long-standing Big Bang Theory as the ultimate origin of the universe.
This new 'Black Hole Universe' hypothesis, suggests that our universe possibly 'bounced' from the formation of larger black hole in another parent universe.
While intriguing, the Big Bang Theory is the undisputed cosmological champ for a reason, so it'll take lots of rigorous experiments to confirm its theoretical conclusions.
Throughout human history, there has been no greater question than 'where do we come from?' This existential curiosity has spawned entire religions, philosophies, and (more recently) serious scientific inquiry. Amazingly, as science and technology have progressed over the past century, we've begun to actually answer that age-old question. Thanks to groundbreaking discoveries in the 20th century—not the least of which was the accidental discovery of the cosmic microwave background in the 1960s—we now know that the universe most likely formed from a rapid expansion of matter known formally as the Big Bang.
But just because the Big Bang is our best answer for the beginning of everything, that doesn't mean it's the only one. In the early years, the main competitor to Big Bang Cosmology was the Steady State Universe (though the discovery of the CMB largely put that idea to rest). But in recent years, new alternatives have emerged to challenge the Big Bang's cosmological supremacy. One of the latest in this contrarian family is detailed in a new paper published in the journal Physical Review D, in which physicists from the University of Portsmouth in the U.K. theorize that maybe our universe formed within an interior black hole of a larger parent universe.
Yeah, let's dig into it.
Comparisons between black holes and the cosmology of our universe make some sense—after all, both contain singularities of a sort and horizons beyond which we can't hope to glimpse. However, this new theory, which is called the 'Black Hole Universe,' suggests that our black hole-generated universe is just one step in a cosmological cycle driven by gravity and quantum mechanics.
'The Big Bang model begins with a point of infinite density where the laws of physics break down. This is a deep theoretical problem that suggests the beginning of the Universe is not fully understood,' Enrique Gaztanaga, lead author of the study from the University of Portsmouth, said in a press statement. 'We've questioned that model and tackled questions from a different angle—by looking inward instead of outward. Instead of starting with an expanding Universe and asking how it began, we considered what happens when an overdensity of matter collapses under gravity.'
The genesis of this theory and others like it stems from the fact that we simply don't know what goes on the heart of black hole. And because knowledge (like nature) abhors a vacuum, scientists begin crafting hypotheses in an attempt to understand this unknown. In Gaztanaga and his team's case, they've shown that a gravitational collapse doesn't necessarily end in a singularity, but can instead 'bounce' into a new expansion phase.
'Crucially, this bounce occurs entirely within the framework of general relativity, combined with the basic principles of quantum mechanics,' Gaztanaga's team said in a press statement. 'We now have a fully worked-out solution that shows the bounce is not only possible—it's inevitable under the right conditions. One of the strengths of this model is that it makes predictions that can be thoroughly tested.'
As a science coordinator on the ESA mission Analysis of Resolved Remnants of Accreted galaxies as a Key Instrument for Halo Surveys, or ARRAKIHS (a true master-class in science acronym-ing), Gaztanaga hopes to use the instrument's ability to analyze ultra-low surface brightness structures in the outskirts of galaxies to see if data points to a 'Black Hole Universe' or the undisputed scientific champ, the Big Bang.
Presenting alternative ideas to long-standing theories is a key function of the scientific method, as it rigorously tests what we think we know from new angles. Even if ARRAKIHS confirms our Big Bang suspicions (as it most likely will), this alternative hypothesis still take us one step closer to truly understanding a question that's followed our species for hundreds of thousands of years.
You Might Also Like
The Do's and Don'ts of Using Painter's Tape
The Best Portable BBQ Grills for Cooking Anywhere
Can a Smart Watch Prolong Your Life?
Hashtags

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles
Yahoo
2 hours ago
- Yahoo
Did 'primordial' black holes born right after the Big Bang help our universe's 1st stars form?
When you buy through links on our articles, Future and its syndication partners may earn a commission. New research suggests that primordial black holes created during the Big Bang could have played a major role in forming the universe's first stars. The findings could help to assess how suitable primordial black holes are as candidates for dark matter, the universe's most mysterious "stuff." But the study team isn't sure yet whether these black holes helped star formation, acting as "cosmic midwives" by ferrying matter to sites of stellar birth, or if they acted to suppress starbirth! The role primordial black holes played in the formation of so-called "Population III (POP III) stars" ( a confusing name for the first generation of stars) all depends on what masses these hypothetical original black holes have. "We investigated how primordial black holes — ancient black holes that may have formed in the very early universe — could have influenced the birth of the first stars," team member Stefano Profumo of the University of California at Santa Cruz (UCSC) told "Using advanced computer simulations, we found that, depending on their mass and abundance, these black holes could either speed up or delay the formation of the first stars." Profumo added that, in some cases, primordial black holes likely acted like "cosmic seeds," helping matter clump together earlier than expected. However, in other scenarios, Profumo and colleagues found that these black holes could have disrupted gas clouds, actually preventing stars from forming promptly. Primordial black holes: Friend or foe to star formation? Primordial black holes are thought to have formed as a result of density fluctuations in matter in the early universe. This is quite different from the origin of so-called stellar-mass black holes, which are created when massive stars collapse and erupt in supernovas at the end of their lives. This means that primordial black holes didn't have to wait for the first generation of stars to live and die before they could be created. Also, it doesn't place the same kinds of mass limits on primordial black holes that exist for stellar-mass black holes, as the former are created directly from early cosmic material rather than from collapsing stars, which can only be so massive. However, because primordial black holes are yet to be discovered, there isn't much else scientists can firmly say about them. Profumo explained how primordial black holes could play a role in star formation. "Massive primordial black holes can serve as powerful gravitational centers. In the early universe, they could have pulled in gas and dark matter more quickly, jump-starting the formation of small galaxies and stars," he said. "This could explain how some of the earliest galaxies we now see — thanks to the James Webb Space Telescope (JWST) — managed to form so surprisingly fast after the Big Bang." However, primordial black holes must have a certain mass to play a positive role in star birth, according to the team's simulations, which were performed using a software package called GIZMO, running the hydrodynamics of the universe's initial gas and dust. "To boost early star formation in the way we observed, the black holes would need to be quite massive — about a thousand to ten thousand times the mass of our sun," Profumo said. "At those sizes, and in the right numbers, they'd have a noticeable effect on how quickly the first stars formed." More massive primordial black holes would do this by causing density fluctuations in matter to increase. This would create more so-called dark matter haloes, vast clusters of this mysterious form of matter within which the building blocks of stars and galaxies could gather en masse. If there are too many of these massive primordial black holes, however, then stars and galaxies would form too fast, thus not reflecting our picture of the early universe. But the team found that primordial black holes with masses smaller than around 100 times that of the sun wouldn't increase density fluctuations. Instead, the team's simulations indicated that, if there were enough of these less massive primordial black holes, the influence of their gravity would generate tidal forces within vast clouds of gas and heat them. This is problematic for star formation, because stellar bodies are born when cold and over-dense clumps of gas and dust collapse under the influence of their own gravity. The more low-mass primordial black holes in the early universe, the more gas is heated and the more star formation is stunted. Thus, this is a really Goldilocks situation. To assist in star formation, the masses and population sizes of primordial black holes need to be "just right." Further investigation of these competing scenarios could tell scientists more about dark matter. Primordial black holes and dark matter Dark matter is so problematic to scientists because, despite accounting for about 85% of the matter in the universe, it remains effectively invisible. That means everything we see — stars, planets, moons, asteroids, comets, each other, and so forth — accounts for just 15% of the stuff in the universe. Scientists can gather that dark matter isn't made up of particles like electrons, protons, and neutrons, which compose the atoms of "normal" matter, because those particles interact with light, and whatever dark matter is doesn't. This has spurred a search for particles beyond the standard model of particle physics. The fact that this hunt has turned up empty has kept primordial black holes in the frame as dark matter suspects. "This research tells us that if primordial black holes do make up some or all of the dark matter, they can't just have any mass or be present in any amount," Profumo said. "If there are too many, or if they're too massive, they would cause the first stars to form much too early — before we see any signs of them. "On the other hand, if they're too small and too abundant, they can get in the way of star formation. This gives us a new way to rule out certain black hole scenarios for dark matter." Of course, primordial black holes remain hypothetical. Barring the detection of these Big Bang-generated black holes, there are other ways that astronomers could find evidence supporting the team's theory about their role in early star formation. "The effects we studied would show up during what's called the cosmic dawn — roughly 100 to 200 million years after the Big Bang. In some of our most extreme scenarios, star formation could start as early as 15 million years after the Big Bang — much earlier than traditional models suggest," Profumo said. "If telescopes like JWST or future instruments can find galaxies or stars forming very, very early in the universe, that would support the idea that something like primordial black holes helped cosmic structures form faster than usual." Related Stories: — A 'primordial' black hole may zoom through our solar system every decade — Primordial black holes may flood the universe. Could one hit Earth? — Tiny black holes left over from the Big Bang may be prime dark matter suspects The next step for the team is to move beyond the assumption that all primordial black holes would have the same masses. "Most theories suggest a mix of masses, and we want to model that more realistically," Profumo said. "We're also planning to improve the physical modeling of star formation, and to simulate larger patches of the early universe to understand how primordial black holes might have influenced not just the first stars but also the formation of early galaxies." The team's research is available as a preprint on the paper repository arXiv. Solve the daily Crossword


WIRED
5 hours ago
- WIRED
This Might Be the Most Massive Black Hole Ever Discovered
Aug 13, 2025 5:47 AM New measurements of the galaxy at the heart of the 'Cosmic Horseshoe' indicate that it could house the most massive object ever seen in the universe. Astronomers have identified what could be a new supermassive black hole, and with an estimated mass 36 billion times that of the sun, it is about 10,000 times heavier than the black hole at the center of the Milky Way. This would make it among the most massive objects ever detected. The finding, published in the Monthly Notice of the Royal Astronomical Society, was made by researchers from the Institute of Cosmology and Gravitation at the University of Portsmouth in the UK in collaboration with the Federal University of Rio Grande in Brazil. The scientists located the signs of the new supermassive black hole within a gravitational lens known as the 'Cosmic Horseshoe,' pictured below. A gravitational lens occurs when the gravity of a massive object, such as a galaxy, is so great that it bends light and time that passes near it, distorting light traveling from behind. The Cosmic Horsehoe was discovered by the Hubble telescope in 2007. The galaxy LRG 3-757 sits at its center, while the blue horseshoe shape surrounding this yellow-colored object is distorted light emitted from another galaxy beyond it. LRG 3-757 is one of the most massive galaxies ever observed by astronomers, having a mass 100 times that of the Milky Way, and it sits approximately 5.6 billion light-years away from Earth. The gravitational lens known as the Cosmic Horseshoe, so named because of the appearance of the incomplete ring of blue light that surrounds its central galaxy, LRG 3-757. Photograph: NASA/ESA Thanks to this luminous structure, astronomers have been able to calculate the mass of the black hole that presumably lies at the center of LRG 3-757 (while not definitively proven, large galaxies are assumed to have a black hole at their center). Although there are no direct observations of this black hole, measurements of the motion of light in the ring and the velocity of stars in the inner regions of the galaxy are consistent with the presence of an ultramassive black hole. 'By combining these two measurements we can be completely confident that the black hole is real,' Thomas Collett, professor of astrophysics at the University of Portsmouth, said in a press statement. Collett also suggests that a black hole of such proportions could only originate from the merger of two supermassive black holes resulting from the collision of galaxies. Astronomers are still debating whether this will be the shared fate of our galaxy, the Milky Way, and neighboring Andromeda. What About TON 618 and the Like? Any astronomy enthusiast knows that the most massive object found in the universe so far is potentially TON 618. According to the most widespread estimates, this black hole has a mass equivalent to 66 billion suns, almost twice that of the Cosmic Horseshoe. However, scientists are cautious about labelling TON 618 as the most massive object ever seen. Being located more than 10 billion light-years away, its host galaxy and surrounding objects cannot be observed in detail. What little is known about it comes from analysis of its brightness and from theoretical models that allow us to estimate its size. The uncertainty is too high to consider it the most massive black hole known. In contrast, the Portsmouth researchers argue that the Cosmic Horseshoe black hole offers greater observational certainty, unlike distant, almost mythological holes like TON 618. As such, they claim that their discovery could represent the most massive black hole confirmed to date. This story originally appeared on WIRED en Español and has been translated from Spanish.
Yahoo
2 days ago
- Yahoo
36 Billion Suns: Record Black Hole Discovery Could Be as Big as They Get
A black hole deep in the cosmos, some 5 billion light-years away, could be the most massive ever found. The galaxy SDSS J1148+1930 harbors a behemoth, around 36.3 billion times the mass of our Sun, according to new measurements. That places the black hole's mass very close to the practical upper limit. For context, the Milky Way's central black hole is a piddling 4.3 million solar masses. This newly discovered black hole no longer fits within the category of supermassive – the giant beast of a thing is ultramassive. Related: Black Holes Could Get So Humongous, Astronomers Came Up With a New Size Category "This is amongst the top 10 most massive black holes ever discovered, and quite possibly the most massive," says astrophysicist Thomas Collett of the University of Portsmouth in the UK. "Most of the other black hole mass measurements are indirect and have quite large uncertainties, so we really don't know for sure which is biggest. However, we've got much more certainty about the mass of this black hole thanks to our new method." Supermassive black holes, larger than about a million solar masses, are thought to lurk in the heart of every full-sized galaxy, the gravitational hub around which everything else in the galaxy revolves. Theoretically, there's no limit to how massive a black hole could grow. In practical terms, other constraints, such as the growth rate, suggest that the maximum mass a black hole could achieve within the current 13.8-billion-year lifespan of the Universe is about 50 billion solar masses. The only way we can test these upper limits, however, is by finding the black holes involved. Which brings us to a fascinating feature in Earth's sky known as the Cosmic Horseshoe. This is a horseshoe-shaped smear of light arcing around a central glowing blob – the result of a rare cosmic alignment called a gravitational lens. Each of the two components – the smear and the blob – are along the same line of sight, at different distances. The blob is actually a galaxy so massive that its gravitational field warps and magnifies the light from a more distant light source. That's what makes the smear. We can learn a lot about distant stars and galaxies magnified this way, but in this case, it's the foreground blob in which a team of astronomers led by Carlos Melo-Carneiro of the Federal University of Rio Grande do Sul in Brazil discovered their astonishing black hole. "This discovery was made for a 'dormant' black hole – one that isn't actively accreting material at the time of observation," Melo-Carneiro says. "Its detection relied purely on its immense gravitational pull and the effect it has on its surroundings." In a lensed system, the extent of the lensing reveals the strength of the gravitational field, which is linked to the mass of the foreground object. Since the masses of supermassive black holes are proportional to the masses of their galaxies, this is one way to calculate the mass of a black hole at a galactic center. Another tool for determining the mass of quiescent black holes involves stellar kinematics – the way stars and other material whirl around. Long-term observations of orbits around the Milky Way's galactic center, for example, confirmed the presence of the black hole therein and provided a measure for its mass. The Cosmic Horseshoe was discovered in 2007. Observations taken at intervals since then allowed the researchers to determine the motions at play in the galactic center. Combined with analysis of the radial arc of the more distant galaxy, the results gave what the researchers say is a very robust measurement. Heavier black holes have been detected, but the measurements are perhaps a little less confident. TON-618 is a famous example. Its mass was initially thought to be around 66 billion solar masses; however, this was revised down in 2019 to about 40 billion solar masses based on galactic kinematics. What makes SDSS J1148+1930 a little more exciting, however, is that it's what is known as a fossil galaxy. This is a single, massive blob of a galaxy that was once a galaxy cluster. The researchers believe that, over time, the galaxies in the cluster – each with a supermassive black hole in its center – merged, their black holes also eventually glomming into one big 36 billion solar mass black hole. It's a huge clue about one of the Universe's many open questions: how supermassive black holes get so enormous. In the Cosmic Horseshoe, "we're seeing the end state of galaxy formation and the end state of black hole formation," Collett says. The discovery has been published in the Monthly Notices of the Royal Astronomical Society. Related News NASA Rovers Keep Getting Stuck, And We Finally Know Why Wild New Theory Suggests Gravitational Waves Shaped The Universe August's Full Sturgeon Moon Is Here: What It Is And How to See It Solve the daily Crossword