SCIENCE

We still don’t know how “hot” the hot Big Bang was | by Ethan Siegel | Starts With A Bang! | Oct, 2025

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The early Universe was full of matter and radiation, and was so hot and dense that it prevented all composite particles, like protons and neutrons from stably forming for the first fraction-of-a-second. There was only a quark-gluon plasma, as well as other particles (such as charged leptons, neutrinos, and other bosons) zipping around at nearly the speed of light. This primordial soup consisted of particles, antiparticles, and radiation: a highly symmetric state. Today’s Universe, by comparison, is more asymmetric, with more matter than antimatter. Presently known physics does not account for this, and we also do not know what the hottest temperatures achieved during the hot Big Bang were. (Credit: Models and Data Analysis Initiative/Duke University)

We’ve long known we can’t go back to infinite temperatures and densities. But the hottest part of the hot Big Bang remains a cosmic mystery.

In many ways, the Big Bang was the biggest idea to ever come out of Einstein’s General theory of Relativity. This tremendously successful theory gave us everything from gravitational waves to black holes based on one profound insight: that the fabric of spacetime itself would evolve, curve, and even ripple based on the properties and behavior of the matter and energy within it. When we applied Einstein’s equations to the entire Universe as a whole, along with the idea that the Universe was filled nearly uniformly with matter and energy on the largest scales, we wound up with an expanding Universe. Extrapolating back in time, we arrived at a very hot, dense, and uniform early state, where all of the Universe’s matter and energy was concentrated into a tiny, minuscule volume.

And yet, if we look at the evidence that persists in the Universe today, left over from those early cosmic stages, we find that the hot Big Bang couldn’t have risen all the way up to the hottest possible temperatures: temperatures corresponding to the Planck scale. Those high energies, corresponding to around 10¹⁹ GeV or 10³² K…


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