What If the Universe Had No Beginning? Part 1: A Wave Function for the Universe

The equations of general relativity give up at the singularity. Decades before Stephen Hawking dared to guess what came before, John Wheeler and Bryce DeWitt built the strange mathematical machinery that would make the question askable in. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.

This matters because astronomy does not advance on single detections. The field builds confidence by accumulating independent observations across different wavelengths, instruments and epochs until isolated signals become defensible conclusions. What looks convincing in one dataset can dissolve when a second instrument looks at the same target, and what looks marginal can solidify when follow-up campaigns confirm the original reading. The current standard requires that a result survive this triangulation before the community treats it as settled. Decades before Stephen Hawking dared to guess what came before, John Wheeler and Bryce DeWitt built the strange mathematical machinery that would make the question askable in the. All you need to do to figure out the mystery of the beginning of the universe is to take your general theory of relativity and run the clock backwards to see what happens, you.

Our journey to the beginning of the universe doesn't start with Hawking. Not to the big bang, the 1960's.

In fact, he was one of the few people in HISTORY to be able to confidently talk about both fields with relative ease, because that's the kind of guy he was. Back in the 60's quantum mechanics was all the rage.

And once you had a quantum theory of a tiny, high-energy thing, you could do all sorts of cool stuff like predicting new particles and understanding how stars worked. For an electron, we replace something like its position with a wave equation describing where the electron MIGHT BE the next time we go looking for it.

What gives the story weight is not just the object itself, but the way the measurement trims the range of plausible physical explanations. Astronomy has accumulated enough cases to know that the most interesting results are rarely the ones that confirm expectations cleanly; they are the ones that confirm some expectations while complicating others, or that open a parameter space that previous instruments could not reach. The scientific community evaluates these contributions by asking whether the new data constrain a model in a way that older data could not, and whether those constraints survive systematic review.

And for the universe, we replace ONE SPECIFIC UNIVERSE (with galaxies over here, some bends and wiggles in space over there) with a whole. CORNUCOPIA. That's because we're dealing with quantum probabilities.

Because this item comes through Universe Today as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.

The next step is to see whether other instruments and other wavelengths tell the same story. Campaigns with JWST, the VLT, the forthcoming Extremely Large Telescopes and radio arrays will provide the spectral coverage and spatial resolution needed to move from detection to physical characterization. The timeline for that kind of confirmation is typically measured in years, not months, which is worth keeping in mind when reading the current result.

Source