
If the universe is infinite, what is it expanding into? Here are ways to tackle a cosmic brain teaser
What is the universe expanding into if it's already infinite? – Mael (10), Missoula, Montana
When you bake a loaf of bread or a batch of muffins, you put the dough into a pan. As the dough bakes in the oven it expands into the baking pan. Any chocolate chips or blueberries in the muffin batter become farther away from each other as the muffin batter expands.
The expansion of the universe is, in some ways, similar. But this analogy gets one thing wrong – while the dough expands into the baking pan, the universe doesn't have anything to expand into. It just expands into itself.
It can feel like a brain teaser, but the universe is considered everything within the universe. In the expanding universe, there is no pan. Just dough. Even if there were a pan, it would be part of the universe and therefore it would expand with the pan.
Even for me, a teaching professor in physics and astronomy who has studied the universe for years, these ideas are hard to grasp. You don't experience anything like this in your daily life. It's like asking what direction is farther north of the North Pole.
Another way to think about the universe's expansion is by thinking about how other galaxies are moving away from our galaxy, the Milky Way.
Scientists know the universe is expanding because they can track other galaxies as they move away from ours. They define expansion using the rate that other galaxies move away from us. This definition allows them to imagine expansion without needing something to expand into.
The expanding universe
The universe started with the Big Bang 13.8 billion years ago. The Big Bang describes the origin of the universe as an extremely dense, hot singularity. This tiny point suddenly went through a rapid expansion called inflation, where every place in the universe expanded outward. But the name Big Bang is misleading. It wasn't a giant explosion, as the name suggests, but a time where the universe expanded rapidly.
The universe then quickly condensed and cooled down, and it started making matter and light. Eventually, it evolved to what we know today as our universe.
The idea that our universe was not static and could be expanding or contracting was first published by the physicist Alexander Friedman in 1922. He confirmed mathematically that the universe is expanding.
While Friedman proved that the universe was expanding, at least in some spots, it was Edwin Hubble who looked deeper into the expansion rate. Many other scientists confirmed that other galaxies are moving away from the Milky Way, but in 1929, Hubble published his famous paper that confirmed the entire universe was expanding, and that the rate it's expanding at is increasing.
This discovery continues to puzzle astrophysicists. What phenomenon allows the universe to overcome the force of gravity keeping it together while also expanding by pulling objects in the universe apart? And on top of all that, its expansion rate is speeding up over time.
Many scientists use a visual called the expansion funnel to describe how the universe's expansion has sped up since the Big Bang. Imagine a deep funnel with a wide brim. The left side of the funnel – the narrow end – represents the beginning of the universe. As you move toward the right, you are moving forward in time. The cone widening represents the universe's expansion.
Scientists haven't been able to directly measure where the energy causing this accelerating expansion comes from. They haven't been able to detect it or measure it. Because they can't see or directly measure this type of energy, they call it dark energy.
According to researchers' models, dark energy must be the most common form of energy in the universe, making up about 68% of the total energy in the universe.
The energy from everyday matter, which makes up Earth, the sun and everything we can see, accounts for only about 5% of all energy.
Outside the expansion funnel
So, what is outside the expansion funnel?
Scientists don't have evidence of anything beyond our known universe. However, some predict that there could be multiple universes. A model that includes multiple universes could fix some of the problems scientists encounter with the current models of our universe.
One major problem with our current physics is that researchers can't integrate quantum mechanics, which describes how physics works on a very small scale, and gravity, which governs large-scale physics.
The rules for how matter behaves at the small scale depend on probability and quantised, or fixed, amounts of energy. At this scale, objects can come into and pop out of existence. Matter can behave as a wave. The quantum world is very different from how we see the world.
At large scales, which physicists call classical mechanics, objects behave how we expect them to behave day-to-day. Objects are not quantised and can have continuous amounts of energy. Objects do not pop in and out of existence.
The quantum world behaves kind of like a light switch, where energy has only an on-off option. The world we see and interact with behaves like a dimmer switch, allowing for all levels of energy. But researchers run into problems when they try to study gravity at the quantum level. At the small scale, physicists would have to assume gravity is quantised. But the research many of them have conducted doesn't support that idea.
One way to make these theories work together is the multiverse theory. There are many theories that look beyond our current universe to explain how gravity and the quantum world work together. Some of the leading theories include string theory, brane cosmology and loop quantum theory.
Regardless, the universe will continue to expand, with the distance between the Milky Way and most other galaxies getting farther over time. DM
Nicole Granucci is an instructor of physics at Quinnipiac University in Connecticut.
This story first appeared in our weekly Daily Maverick 168 newspaper, which is available countrywide for R35.
This story first appeared in our weekly Daily Maverick 168 newspaper, which is available countrywide for R35.

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Daily Maverick
23-07-2025
- Daily Maverick
The building blocks of life — how atoms form in extreme heat
Most of the universe is made up of hydrogen and helium atoms, which came into being after the Big Bang cooled down a little. Heavier atoms are formed during high-energy collisions in stars. How do atoms form? – Joshua (7), Shoreview, Minnesota, US Richard Feynman, a famous theoretical physicist who won the Nobel Prize, said that if he could pass on only one piece of scientific information to future generations, it would be that all things are made of atoms. Understanding how atoms form is a fundamental and important question, since they make up everything with mass. The question of where atoms come from requires a lot of physics to be answered completely – and even then, physicists like me only have good guesses to explain how some atoms are formed. What is an atom? An atom consists of a heavy centre, called the nucleus, made of particles called protons and neutrons. An atom has lighter particles called electrons that you can think of as orbiting the nucleus. The electrons each carry one unit of negative charge, the protons each carry one unit of positive charge, and the neutrons have no charge. An atom has the same number of protons as electrons, so it is neutral − it has no overall charge. Now, most of the atoms in the universe are the two simplest kinds: hydrogen, which has one proton, zero neutrons and one electron; and helium, which has two protons, two neutrons and two electrons. Of course, on Earth there are lots of atoms besides these that are just as common, such as carbon and oxygen, but I'll talk about those soon. An element is what scientists call a group of atoms that are all the same, because they all have the same number of protons. The first atoms form Most of the universe's hydrogen and helium atoms formed about 400,000 years after the Big Bang, which is the name for when scientists think the universe began, about 14 billion years ago. Why did they form at that time? Astronomers know from observing distant exploding stars that the size of the universe has been getting bigger since the Big Bang. When the hydrogen and helium atoms first formed, the universe was about 1,000 times smaller than it is now. Before this time, the electrons had too much energy to settle into orbits around the hydrogen and helium nuclei. So, the hydrogen and helium atoms could form only once the universe cooled down to something like 2,760 degrees Celsius. For historical reasons, this process is misleadingly called recombination, but combination would be more descriptive. The helium and deuterium − a heavier form of hydrogen − nuclei formed even earlier, just a few minutes after the Big Bang, when the temperature was above 556 million degrees Celsius. Protons and neutrons can collide and form nuclei like these only at very high temperatures. Scientists believe that almost all the ordinary matter in the universe is made of about 90% hydrogen atoms and 8% helium atoms. How do more massive atoms form? So, the hydrogen and helium atoms formed during recombination, when the cooler temperature allowed electrons to fall into orbits. But you, I and almost everything on Earth is made of many more massive atoms than just hydrogen and helium. How were these atoms made? The surprising answer is that more massive atoms are made in stars. To make atoms with several protons and neutrons stuck together in the nucleus requires the type of high-energy collisions that occur in very hot places. The energy needed to form a heavier nucleus needs to be large enough to overcome the repulsive electric force that positive charges, like two protons, feel. Protons and neutrons also have another property – kind of like a different type of charge – that is strong enough to bind them together once they are able to get very close together. This property is called the strong force, and the process that sticks these particles together is called fusion. Scientists believe that most of the elements from carbon up to iron are fused in stars heavier than our sun, where the temperature can exceed 556 million degrees Celsius – the same temperature that the universe was when it was a few minutes old. But even in hot stars, elements heavier than iron and nickel won't form. These require extra energy, because the heavier elements can more easily break into pieces. In a dramatic event called a supernova, the inner core of a heavy star suddenly collapses after it runs out of fuel to burn. During the powerful explosion this collapse triggers, elements that are heavier than iron can form and get ejected into the universe. Astronomers are still figuring out the details of other fantastic stellar events that form larger atoms. For example, colliding neutron stars can release enormous amounts of energy – and elements such as gold – on their way to forming black holes. Understanding how atoms are made requires learning a little general relativity, plus some nuclear, particle and atomic physics. But to complicate matters, there is other stuff in the universe that doesn't appear to be made from normal atoms at all, called dark matter. Scientists are investigating what dark matter is and how it forms. DM First published by The Conversation. Stephen L Levy is associate professor of physics, applied physics and astronomy at the State University of New York at Binghamton. This story first appeared in our weekly Daily Maverick 168 newspaper, which is available countrywide for R35.

IOL News
04-06-2025
- IOL News
What if the Big Bang wasn't the beginning? It may have taken place inside a black hole
The Big Bang is often described as the explosive birth of the universe. But what if this was not the beginning at all? Image: Vadim Sadovski/Shutterstock Enrique Gaztanaga The Big Bang is often described as the explosive birth of the universe – a singular moment when space, time and matter sprang into existence. But what if this was not the beginning at all? What if our universe emerged from something else – something more familiar and radical at the same time? In a new paper, published in Physical Review D, my colleagues and I propose a striking alternative. Our calculations suggest the Big Bang was not the start of everything, but rather the outcome of a gravitational crunch or collapse that formed a very massive black hole – followed by a bounce inside it. This idea, which we call the black hole universe, offers a radically different view of cosmic origins, yet it is grounded entirely in known physics and observations. Today's standard cosmological model, based on the Big Bang and cosmic inflation (the idea that the early universe rapidly blew up in size), has been remarkably successful in explaining the structure and evolution of the universe. But it comes at a price: it leaves some of the most fundamental questions unanswered. For one, the Big Bang model begins with a singularity – a point of infinite density where the laws of physics break down. This is not just a technical glitch; it's a deep theoretical problem that suggests we don't really understand the beginning at all. To explain the universe's large-scale structure, physicists introduced a brief phase of rapid expansion into the early universe called cosmic inflation, powered by an unknown field with strange properties. Later, to explain the accelerating expansion observed today, they added another 'mysterious' component: dark energy. In short, the standard model of cosmology works well – but only by introducing new ingredients we have never observed directly. Meanwhile, the most basic questions remain open: where did everything come from? Why did it begin this way? And why is the universe so flat, smooth, and large? New model Our new model tackles these questions from a different angle – by looking inward instead of outward. Instead of starting with an expanding universe and trying to trace back how it began, we consider what happens when an overly dense collection of matter collapses under gravity. This is a familiar process: stars collapse into black holes, which are among the most well-understood objects in physics. But what happens inside a black hole, beyond the event horizon from which nothing can escape, remains a mystery. In 1965, the British physicist Roger Penrose proved that under very general conditions, gravitational collapse must lead to a singularity. This result, extended by the late British physicist Stephen Hawking and others, underpins the idea that singularities – like the one at the Big Bang – are unavoidable. The idea helped win Penrose a share of the 2020 Nobel prize in physics and inspired Hawking's global bestseller A Brief History of Time: From the Big Bang to Black Holes. But there's a caveat. These 'singularity theorems' rely on 'classical physics' which describes ordinary macroscopic objects. If we include the effects of quantum mechanics, which rules the tiny microcosmos of atoms and particles, as we must at extreme densities, the story may change. In our new paper, we show that gravitational collapse does not have to end in a singularity. We find an exact analytical solution – a mathematical result with no approximations. Our maths show that as we approach the potential singularity, the size of the universe changes as a (hyperbolic) function of cosmic time. This simple mathematical solution describes how a collapsing cloud of matter can reach a high-density state and then bounce, rebounding outward into a new expanding phase. But how come Penrose's theorems forbid out such outcomes? It's all down to a rule called the quantum exclusion principle, which states that no two identical particles known as fermions can occupy the same quantum state (such as angular momentum, or 'spin'). And we show that this rule prevents the particles in the collapsing matter from being squeezed indefinitely. As a result, the collapse halts and reverses. The bounce is not only possible – it's inevitable under the right conditions. Crucially, this bounce occurs entirely within the framework of general relativity, which applies on large scales such as stars and galaxies, combined with the basic principles of quantum mechanics – no exotic fields, extra dimensions or speculative physics required. 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Daily Maverick
25-05-2025
- Daily Maverick
If the universe is infinite, what is it expanding into? Here are ways to tackle a cosmic brain teaser
It is a real mind-bender, but everything is contained within the cosmos, which is still nevertheless expanding outwards from the Big Bang. What is the universe expanding into if it's already infinite? – Mael (10), Missoula, Montana When you bake a loaf of bread or a batch of muffins, you put the dough into a pan. As the dough bakes in the oven it expands into the baking pan. Any chocolate chips or blueberries in the muffin batter become farther away from each other as the muffin batter expands. The expansion of the universe is, in some ways, similar. But this analogy gets one thing wrong – while the dough expands into the baking pan, the universe doesn't have anything to expand into. It just expands into itself. It can feel like a brain teaser, but the universe is considered everything within the universe. In the expanding universe, there is no pan. Just dough. Even if there were a pan, it would be part of the universe and therefore it would expand with the pan. Even for me, a teaching professor in physics and astronomy who has studied the universe for years, these ideas are hard to grasp. You don't experience anything like this in your daily life. It's like asking what direction is farther north of the North Pole. Another way to think about the universe's expansion is by thinking about how other galaxies are moving away from our galaxy, the Milky Way. Scientists know the universe is expanding because they can track other galaxies as they move away from ours. They define expansion using the rate that other galaxies move away from us. This definition allows them to imagine expansion without needing something to expand into. The expanding universe The universe started with the Big Bang 13.8 billion years ago. The Big Bang describes the origin of the universe as an extremely dense, hot singularity. This tiny point suddenly went through a rapid expansion called inflation, where every place in the universe expanded outward. But the name Big Bang is misleading. It wasn't a giant explosion, as the name suggests, but a time where the universe expanded rapidly. The universe then quickly condensed and cooled down, and it started making matter and light. Eventually, it evolved to what we know today as our universe. The idea that our universe was not static and could be expanding or contracting was first published by the physicist Alexander Friedman in 1922. He confirmed mathematically that the universe is expanding. While Friedman proved that the universe was expanding, at least in some spots, it was Edwin Hubble who looked deeper into the expansion rate. Many other scientists confirmed that other galaxies are moving away from the Milky Way, but in 1929, Hubble published his famous paper that confirmed the entire universe was expanding, and that the rate it's expanding at is increasing. This discovery continues to puzzle astrophysicists. What phenomenon allows the universe to overcome the force of gravity keeping it together while also expanding by pulling objects in the universe apart? And on top of all that, its expansion rate is speeding up over time. Many scientists use a visual called the expansion funnel to describe how the universe's expansion has sped up since the Big Bang. Imagine a deep funnel with a wide brim. The left side of the funnel – the narrow end – represents the beginning of the universe. As you move toward the right, you are moving forward in time. The cone widening represents the universe's expansion. Scientists haven't been able to directly measure where the energy causing this accelerating expansion comes from. They haven't been able to detect it or measure it. Because they can't see or directly measure this type of energy, they call it dark energy. According to researchers' models, dark energy must be the most common form of energy in the universe, making up about 68% of the total energy in the universe. The energy from everyday matter, which makes up Earth, the sun and everything we can see, accounts for only about 5% of all energy. Outside the expansion funnel So, what is outside the expansion funnel? Scientists don't have evidence of anything beyond our known universe. However, some predict that there could be multiple universes. A model that includes multiple universes could fix some of the problems scientists encounter with the current models of our universe. One major problem with our current physics is that researchers can't integrate quantum mechanics, which describes how physics works on a very small scale, and gravity, which governs large-scale physics. The rules for how matter behaves at the small scale depend on probability and quantised, or fixed, amounts of energy. At this scale, objects can come into and pop out of existence. Matter can behave as a wave. The quantum world is very different from how we see the world. At large scales, which physicists call classical mechanics, objects behave how we expect them to behave day-to-day. Objects are not quantised and can have continuous amounts of energy. Objects do not pop in and out of existence. The quantum world behaves kind of like a light switch, where energy has only an on-off option. The world we see and interact with behaves like a dimmer switch, allowing for all levels of energy. But researchers run into problems when they try to study gravity at the quantum level. At the small scale, physicists would have to assume gravity is quantised. But the research many of them have conducted doesn't support that idea. One way to make these theories work together is the multiverse theory. There are many theories that look beyond our current universe to explain how gravity and the quantum world work together. Some of the leading theories include string theory, brane cosmology and loop quantum theory. Regardless, the universe will continue to expand, with the distance between the Milky Way and most other galaxies getting farther over time. DM Nicole Granucci is an instructor of physics at Quinnipiac University in Connecticut. This story first appeared in our weekly Daily Maverick 168 newspaper, which is available countrywide for R35. This story first appeared in our weekly Daily Maverick 168 newspaper, which is available countrywide for R35.