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What If the Universe Had No Beginning? Part 2: No Boundary, No Problem
(This is Part 2 of a series on Hawking’s no-boundary proposal. Read Part 1 first.)
I thought the whole point of this program was that we couldn’t just…get to the beginning of the universe, and now, thanks to the magic of Wheeler and DeWitt, we have the precise machinery we need to solve the beginning of the universe….if only we knew one thing, just one tiny piece of information, just one measly morsel…and we could do it.
Hawking did it. Well, he had an idea, which is more than anyone else had at the time.
Two decades after Wheeler and DeWitt, Stephen Hawking comes along and connects, as he usually does, several different lines of thought, and he realizes that the problem for one thing is actually the solution to another.
Check this out: Hawking is staring at the Wheeler-DeWitt equation. It’s a puzzle that reveals the universe, but all the puzzle pieces are scattered around, AND we don’t have the picture on the front of the box. If we know how to place just ONE piece, we can put together the quantum wave function of the universe.
We just need the first piece. The boundary condition that defines the beginning state of the universe. But we can’t measure it, we can’t read any device or look through any telescope to figure it out. Nothing gives us access to the first moment of the big bang. AND we have no theory of quantum gravity around the corner to just ASK.
So that leaves us with…taking a wild guess and seeing if it sticks.
Hawking decided that his wild guess would be as grounded as possible. He argued that the best boundary condition of the universe, the best statement that you can make about how it all gets started, had to be SELF-JUSTIFYING. That means the guess about the beginning of the universe couldn’t come from anywhere else: you can’t point to God or Wheeler or ANYTHING to just HAND you the answer, because the universe is every single thing to ever exist, in totality, and you can’t reach OUTSIDE that. There’s no hidden corner of the cabinet that exists outside the universe to just give us the boundary.
And the most self-justifying statement Hawking could make about the beginning of the universe is that it had no beginning.
In other words, what if the reason you can’t find the boundary at the beginning of the universe is not because it’s hidden or inaccessible, but because it genuinely isn’t there?
Now this is a very lovely thought to have. But we’re not here for lovely thoughts, we’re here for down and dirty physics. It’s one thing to say something crazy, it’s another to turn that into a working theory of nature. Thankfully, Hawking had exactly what he needed.
One of the defining features of the Wheeler-DeWitt equation is that it doesn’t involve time. It doesn’t know or care that the universe evolves, expands, does interesting things, heads out to dinner on a Tuesday night just because it’s wild like that.
The key that can unlock the Wheeler-DeWitt equation is a solid statement ABOUT time, specifically, the most important time of all: the beginning of the universe. So we NEED to involve time SOMEHOW in all this mess if we’re going to make progress.
So Hawking…involves time. Instead of just looking at space, he stitches together these geometries back to back like frames in a film. He makes a sequence of them, representing an evolution to the history of the universe. These frames tell the story of the cosmos. Now, we don’t know what that story is (I mean, from Wheeler and DeWitt’s machine; we can observe it and so we KNOW it, but we’re trying to EXPLAIN it), so Hawking constructs all these…paths. Possible histories of the universe. Trajectories, evolutions, stories. In some stories, the universe gets really big really fast and fizzles out to nothing. In others, it never even expands. In still others, there’s nothing but matter. And others, nothing but…nothing.
Now all of these paths, all of these histories of the universe, all share one thing in common: they’re in the usual spacetime that we know and love. Cause and effect, past and future, speed of light, all that. And they all have a BEGINNING. A first frame in the movie of the universe.
Well, what if we just made time behave differently? Now I’m going to share a term with you, and when I say it it’s going to sound really wrong, like icky, deep in your gut. But I’m going to say it, then I’m going to explain it. It…will still feel icky, but at least it will have an explanation.
Here goes: imaginary time.
Yeah, imaginary time. Time, but imaginary. Listen, I don’t know how much you know about imaginary numbers. But they’re really cool and fun and DEFINITELY worth bringing up in your next workplace all-hands meeting. The core idea behind imaginary numbers is to pretend to take the square root of, I don’t know, negative 4. The square root of regular four is 2, but the square root of negative four is…uh….what? In normal grade school math this is where your teacher scoffs at you and says you can’t take the square root of a negative number.
But this isn’t grade school. We’re not going to take the square root of a negative number. Instead, we’re going to say that the square roots of negative numbers are an ENTIRELY NEW KIND OF NUMBER. A brand new category. You have whole numbers, rational numbers, negatives, and now you have imaginary numbers, which are all the square roots of the negative numbers.
Phew, I swear I’m going somewhere with this.
The trick Hawking pulled was that he took all these histories of spacetime and replaced “time” with “imaginary time”. He multiplied the passage of time by the square root of negative one. Now, we actually do this in quantum mechanics all the time (or should I say imaginary time?) as a TRICK. Sometimes when we get equations that are really, really hard to solve, we replace time with imaginary time and they become easier. Then we solve them, then we swap back. Just a little reshuffling in the backend to work through some thorny problems.
But when Hawking does this to the spacetime of the universe, he gets a bonus. It’s not a party trick anymore. It’s a statement. You see, in normal spacetime, the universe has a beginning. But when you replace time with imaginary time, the beginning…goes away. This procedure actually puts space and time on equal footing. It makes them all creatures of curvature and geometry, with no separate identity. Which makes the beginning of the universe no special time at all. It becomes like the south pole, which is really just any other point on the globe. You reach the south pole and keep walking, and it’s only ever north from there. You reach the beginning of the universe, and it’s not special or unique (maybe a little hot); all you have is the future in front of you.
No beginning. No start. No boundary. A universe that justifies itself.
By making the switch to imaginary time, Hawking could ENCODE his “the universe has no beginning” idea, AND he could crunch through the math.
Voila: a key that unlocks the Wheeler-DeWitt equation and the know-how to run the mathematical machinery.
And what do you get for all this work? Nothing less than a wave function for the universe.
In Part 3, the wave function delivers something Hawking didn’t even ask for: our universe, more or less, for free.
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With Blanche Nomination at Stake, Payouts to Trump Allies Continue
A seven-figure settlement is announced two days before a scheduled Senate committee vote on Todd Blanche’s nomination to be attorney general.
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A Wandering Black Hole Meets a Wandering Star
What happens when a black hole and a star meet in the middle of nowhere in a galaxy? It sounds like it could be a dramatic science fiction backdrop, with some hapless starship caught in the crunch. Actually, such encounters in real life are pretty rare. They happen maybe once every 100,000 years. But when they do occur, the immense gravity of the supermassive black hole tears the star apart. It’s an eerie-looking process. The star gets “spaghettified” — that is, pulled on one side by the black hole. That rips out a stream of gas from the star, which eventually loops around in a disk around the black hole as the star’s orbit spirals into the black hole.
A computer graphics simulation of a star being disrupted by the gravitational pull of a nearby supermassive black hole. This part of a tidal disruption event emits radiation that can be detected and reveal the presence of the black hole. Courtesy Danielhamesprice CC BY-SA 4.0
As the material in the disk gets heated by friction in the magnetic field, it starts to glow in visible and other forms of light. Eventually, a jet forms, sending a stream of superheated material away from the site of the event. The glow is what allows astronomers to witness the action, called a “tidal disruption event” (TDE).
About a hundred or so TDEs have been observed optically (i.e., in visible light) since the late 20th century. They’ve also been detected with X-ray, infrared, and radio instruments, which gives astronomers an idea of how powerful the action is when they occur. Usually TDEs happen in the cores of galaxies, where the central supermassive black holes exist surrounded by orbiting stars and gas clouds. But there’s nothing that says they all occur there. Some happen well away from the core, or “off-nuclear” as the astronomers like to say.
Observing a Recent TDE
A team of researchers at the University of North Carolina-Chapel Hill recently used the Southern Astrophysical Research Telescope (SOAR) to watch a flaring event called TDE 2025abcr. They identified it as a possible TDE using an AI classification program adapted to search for TDEs away from galactic cores, according to team member Akash Anumarlapudi. “By removing the assumption that these events only happen in the galactic center, we were able to find a black hole that might have otherwise been missed,” explained Anumarlapudi. Once the AI identified a candidate, the team then turned to SOAR to do optical observations.
TDE 2025abcr was the first optical TDE discovered on the outskirts of a host galaxy. It’s not only nowhere near the core of its home galaxy, but the event occurred some 30,000 light-years away. For reference, our Sun lies some 26,000 light-years away from the core of the Milky Way, and we’re out in a spiral arm, not near the core. According to study leader Jonathan Carney, a PhD student in astrophysics at Chapel Hill, TDE 2025abcr turns out to be the most offset such event ever seen.
“Almost every tidal disruption event we’ve ever observed has occurred at the center of a galaxy, right where we expect the biggest black holes to be,” Carney said. “The tidal disruption event we discovered happened tens of thousands of light-years away from the center, revealing a massive black hole in a place we would not normally expect to find one. We know that wandering black holes exist in massive galaxies, but they are difficult to study because, with the exception of when they briefly disrupt a star, they produce no light.”
A Hubble Space Telescope optical image of the TDE Swift J1644+57. It sported a relativistic jet that flowed away from the TDE for about a year and a half. Courtesy NASA/ESA/STScI
Learning About the Black Hole
For a black hole to disrupt a star like this, it has to be quite massive. The team estimates this one is probably about a million times the mass of the Sun. It’s pretty rare to have such a monster just wandering around in space like this one does. So, that raises questions about how it got to where it was when it encountered the hapless star. It’s possible that the black hole was part of a galaxy collision in the distant past. During that event, it could have been kicked out from the center of one of the participating galaxies. Or, it could have been one of several black holes at the core of a galaxy and gotten nudged out of place through interactions with one or more of the others.
Observations of this event show that astronomers have a way to spot wandering black holes away from the cores of their galaxies. Normally, black holes don’t give off much, if any, radiation or other clues to pinpoint their locations. But if one tangles with a star that gets too close, the resulting electromagnetic radiation from the collision gives away the black hole’s location. TDE 2025abcr’s discovery is a template for how astronomers can do visible-light observations of other such black hole entanglements from Earth. That means they’ll be able to discover and study hundreds of thousands of TDEs per year ranging out to great distances from the Milky Way. The Vera C. Rubin Observatory, for example, could be a major contender in the hunt for black holes that tangle with nearby stars.
Ongoing TDE studies with Rubin and other observatories can also reveal more information about the life cycles of the stars that get swept up into a TDE event. TDEs also release enormous amounts of energy, and that can help astronomers study gravitational forces and matter that occur under conditions that cannot be studied in the lab.
For More Information
UNC-Chapel Hill Astronomers Detect One of the Universe’s Rarest Black Hole Events
TDE 2025abcr: A Tidal Disruption Event in the Outskirts of a Massive Galaxy
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Magnitude 4.2 earthquake rattles Northern California

A magnitude 4.2 earthquake was reported Tuesday at 7:40 p.m., eight miles from Healdsburg, Calif., according to the U.S. Geological Survey.
According to the agency, the epicenter was about five miles east-southeast of Cloverdale, around 19 miles from Clearlake and 22 miles from Santa Rosa. The quake occurred at a depth of 3.4 miles.
It caused light to moderate shaking at an intensity expected to cause, at most, very light damage, according to the USGS.
Quakebot, a computer application that monitors the latest earthquakes detected by the USGS, contributed to this report. A Times editor reviewed the post before it was published. If you’re interested in learning more about the system, visit our list of frequently asked questions.
To get prepared for earthquakes, sign up for The Times’ Unshaken newsletter.
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