In this video here posted by Kurzgesagt – In a Nutshell, at 2:01, it is said that particles like electrons and protons don't want to be near each other. Wouldn't oppositely charged particles attract each other and if not for the centrifugal force on the revolving electrons, they would get dragged towards the protons and fall into the nucleus?
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The electron is not spinning and can sit quite stationary in its ground state a set distance from the proton. Its trapped on the couloumb potential. – shai horowitz Feb 06 '21 at 08:06
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1@shaihorowitz The question still stands - Do the electrons and protons not want to be near each other? – Your IDE Feb 06 '21 at 08:09
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There's a potential barrier if they get to close. If this is overcome they can fuse and become a neutron. This is what happens for neutron stars. The exact nature of this barrier is subtle and only occurs at subatomic distance – shai horowitz Feb 06 '21 at 08:13
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why doesnt the earth crash into the sun? why not the moon into the earth? it all has to do with potentials, and atomic systems obey potentials and evolve as per the laws of Quantum Mechanics (Schrodinger Equation). Much in the way that the earth evolves are per the laws of gravity and mechanics, ofcourse there are many differences. – xXx_69_SWAG_69_xXx Feb 06 '21 at 08:29
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1The video is about neutron stars, and "particles like electrons and protons really don't want to be near each other" is clearly a reference to the Pauli exclusion principle. Your question seems to be about something else entirely, and it looks like none of the three answerers so far watched the video. Please clarify if your question is supposed to be about the Pauli exclusion principle or not. – benrg Feb 06 '21 at 18:21
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@benrg I am unsure if it concerns to Pauli exclusion principle. I just wanted to know why e- and p+ don't want to be near each other when opposite charges are supposed to be attractive? Perhaps, it's an over-simplified view that unlike charges attract which seems to be in contradiction to what is mentioned in the video. – Your IDE Feb 09 '21 at 10:25
3 Answers
You are correct, the planetary model of the atom would not work, because the orbiting electron would accelerate and lose energy and fall into the nucleus. This is one of the very reasons QM was invented.
One of the reasons for "inventing" quantum mechanics was exactly this conundrum.
Why don't electrons crash into the nuclei they "orbit"?
By the way, with certain probabilities, electrons do exist inside the nucleus, and sometimes even "crash" into it, we call it electron capture.
https://en.wikipedia.org/wiki/Electron_capture
Now if you accept that the underlying nature of the universe is quantum mechanical, and electrons exist in orbitals (not orbits), and the wavefunction describes the probabilities of the electron existing around the nucleus, then you continue your way towards the Heisenberg Uncertainty Principle.
https://en.wikipedia.org/wiki/Uncertainty_principle
Then you will see that the reason electrons exist around the nucleus in stable orbits is rooted deep in QM because:
the EM force is attracting the electron and the proton
the HUP keeps the electron from existing in a too small region of space, thus balancing the EM force (the reason why electrons exist in quantized stable orbitals is more complicated and needs deeper QM)
And there you have it, the existence of a beautiful balance and an explanation why QM is the dominant description of the atomic level.
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Wouldn't oppositely charged particles attract each other and if not for the centrifugal force on the revolving electrons, they would get dragged towards the protons and fall into the nucleus?
Yes but this is very improbable even in classical-theoretic models. If the electron moves transversally ("around the center") in pure central Coulomb field of the nucleus, this motion is enough to prevent the fall into the nucleus, because in a central Coulomb field there are stable elliptical orbits like there are for planets orbiting the Sun. If we take into account radiation of the electron and the proton, then these orbits are not stable and the electron can fall on the proton.
But if we then take into account the background radiation as well (due to all other bodies in the universe), there are numerical indications that this can prevent the collapse [1]. The simple explanation is that the external radiation keeps kicking the electron out of the proton vicinity.
[1] Cole D. C., Zou Y.:Quantum Mechanical Ground State of Hydrogen Obtained from Classical Electrodynamics, 2003, https://arxiv.org/abs/quant-ph/0307154
In the standard quantum theoretical model of the hydrogen atom, the electron does not have position and velocity. Instead, it is described by a function $\psi$ of coordinates $x,y,z$. This function could get sucked into the proton, if the central field was increasing stronger with decreasing distance than the Coulomb field does. For example, attractive central field that varies as $1/r^4$ is too strong at the singularity and according to the time-dependent Schroedinger equation it will suck the $\psi$ function into the singularity.
But for the Coulomb field there are stable solutions where the $\psi$ function is finite around the proton in a region with dimensions of magnitude 1e-10 m. This "noncollapse" is due to the Schroedinger equation containing quadratic term in momentum.
So, the mechanism varies in different models, but they all are capable to account for the fact that although electron is attracted, it does not fall on the proton too frequently.
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An electron is associated with a wave. The amplitude of the wave at any point determines the probability that it will react with something else at that point. Electron orbitals in an atom are resonant 3D standing wave patterns bounded by the electric field from the nucleus. These patterns are much larger than the nucleus, and the probability of their interacting with something in the nucleus is quite small.
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