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I haven't think out a way to detect it to proof or disproof its existence, can you help?
Physics laws are created by men, men don't create particles.
You didn't come out anything you knew besides from books.Can you proof enertron is not there? How you explain electrons not stick to proton? Wait few more years, learn more new theories and discoveries. Science is advancing.
Quote from: Sarah Raphaella RodgersSo why don't electrons stick to protons instead of flying around the nucleus? Magnets do it, so why can't atoms?The present state of physical science does not allow "why" questions. Any answer will have to be speculative.
So why don't electrons stick to protons instead of flying around the nucleus? Magnets do it, so why can't atoms?
Why not? Science should be always allows why questions?
I am very confused. Isn't Newton ask why apple falls so to discover gravitation? Isn't scientist ask why there is red shift so to make big bang theory? Why can't we ask why to any thing we don't understand? Seriously, what is science all about?
You can indeed ask why, but the best a scientist can tell you is how.
In the 1970’s, the study of cosmology went through a major conceptual change. Prior to this time, modern cosmologists asked such questions as; What is the composition of galaxies and where are they located in space? How rapidly is the universe expanding? What is the average density of matter in the cosmos? After this time, in the “new cosmology,” cosmologists began seriously asking questions like: Why does matter exist at all, and where did it come from? Why is the universe as homogenous as it is over such vast distances? Why is the cosmic density of matter such that the energy of expansion of the universe is almost exactly balanced by its energy gravitational attraction? In other words, the nature of the questions changed. “Why?” was added to “What?” and “How? and “Where?”. Alan Guth was one of the young pioneers of the new cosmology, asking the Whys, and his Inflationary Universe theory provided many answers.
So we observe red shift and ask how it can be explained. You can look at the known phenomena of doppler shift and general relativity, and deduce that distant objects in general are moving away from each other, which suggest that at some time they were closer together (or that space was smaller) hence there must have been a starting point before which the universe bore no resemblance to its present state. No "why" because no need for an ultimate purpose - it just is, and apparently was, so let's untangle the mechanism of "how" it got from there to here.
After 4 pages of discussion, I still don't understand this question - Why don't an atom's electrons fall into the nucleus and stick to the protons?Please someone help me to understand, or let me know where else to find answer.
The short answer is that a "proton and electron stuck together" does happen, in a neutron.However, a neutron is unstable, and will break down in about 15 minutes, releasing an electron (beta particle) and proton, plus a ghost-like particle called a neutrino. This decay releases a lot of energy. So, a hydrogen atom (=proton+electron) is much more stable than a isolated neutron.Neutrons can be stable, if they are combined into an atomic nucleus with protons in the right ratio. In this case, the strong nuclear force provides the binding force to keep the nucleus stable.Too many neutrons, and one could decay (releasing an electron, as described above)Too few neutrons, and an inner electron can be captured, forming a neutron, just as you askedThere are other nuclear decay paths too; for more details: http://en.wikipedia.org/wiki/Stable_nuclei
I don't know how important this is for neutron stars, but neutrons in atomic nuclei are certainly magnetic--both protons and neutrons have "nuclear spin" that results in a small magnetic field. I don't know to what extent the spins would arrange themselves to cancel out in a neutron star, but it would only take a small imbalance to have a fairly large magnetic moment. (A neutron has a spin of magnitude 1/2, some of the most out-of balance, but still stable nucleons have a spin of 7/2. Some more extreme nuclear states only last a short while (110Ag has a 12/2 nuclear spin, but a half life of only 253 days, and 43Sc has a 19/2 nuclear spin, but a half-life of only 450 ns!)