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Nuclei in sentence

37 examples of Nuclei in a sentence

What we see are, first of all, a very active culture, a lot of divisions, and then very clear nuclei once the cells have separated.
Now let's go and grab all of the nuclei from a typical car.
How many cars' nuclei would you have to put into the box to have your one-foot-box have the same density of the nucleus?
Look at the nuclei.
The nuclei in the cell on the left is in the animal, the one on the right is in a dish.
And then we took the dead nucleus from the dead tissue of the extinct frog and we inserted those nuclei into that egg.
The biological clock tells us when it's good to be up, when it's good to be asleep, and what that structure does is interact with a whole raft of other areas within the hypothalamus, the lateral hypothalamus, the ventrolateral preoptic nuclei.
If the Higgs field were only a few times more intense, we would see atoms shrinking, neutrons decaying inside atomic nuclei, nuclei disintegrating, and hydrogen would be the only possible chemical element in the universe.
This soup contains all the nuclei that once were a mouse brain.
Now, the beauty of a soup is that because it is soup, you can agitate it and make those nuclei be distributed homogeneously in the liquid, so that now by looking under the microscope at just four or five samples of this homogeneous solution, you can count nuclei, and therefore tell how many cells that brain had.
So you take two small nuclei, you put it together, and you make helium, and that's very nice.
So the problem is, those two nuclei, they are both positively charged, so they don't want to fuse.
The forest emits smells, and these smells are condensation nuclei, which form drops in the atmosphere.
Today, things are largely made up of atoms, but hundreds of seconds after the Big Bang, it was too hot for electrons to join atomic nuclei to make atoms.
A few seconds after the Big Bang, it was hotter still, hot enough to overpower the forces that usually hold protons and neutrons together in atomic nuclei.
The quarks, these pink things, are the things that make up protons and neutrons that make up the atomic nuclei in your body.
The strong force, the strong nuclear force, which sticks nuclei together, gets weaker.
But what this cataclysmic eruption leaves behind might be even more remarkable: a ball of matter so dense that atomic electrons collapse from their quantum orbits into the depths of atomic nuclei.
This process produces an incredible amount of energy, and in some materials the neutrons produced by one fission are absorbed by nearby atoms, splitting additional nuclei.
If the expansion of the universe continues to accelerate, it will eventually overcome not only the gravitational force – tearing apart galaxies and solar systems– but also the electromagnetic, weak, and strong nuclear forces which hold atoms and nuclei together.
And strong interactions are happening millions of times each second in every atom of our bodies, holding the atomic nuclei together.
Stars are fueled by how the nuclei in those atoms react together.
And, as we've learned in the last few years, galaxies are held together by the gravitational pull of so-called dark matter: particles in huge swarms, far smaller even than atomic nuclei.
Because iron is the most bound nuclei in the universe, which means that we cannot extract energy by burning iron.
Connection between life and radioactive nuclei is straightforward.
And we call them active galactic nuclei.
Because that is the way to suppress the energetic phenomena that we see in active galactic nuclei.
But small atoms want to join together, small nuclei want to join together to make bigger ones to go towards iron.
These two nuclei, when they're far apart, are charged.
And, ultimately, these are some slides from an early project I did, computing where the bits are stored quantum-mechanically in the nuclei of atoms, so programs rearrange the nuclear structure of molecules.