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Sometimes, we don’t get to decide what our show’s about. So many threads come together at the same time driving the decision for us. This is one of those situations. We’ve gotten so many questions from listeners in just the last week about antimatter that our show had just been chosen for it. You command, we obey. Let’s talk about antimatter.
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A photon however is its own anti-particle! Another interesting point about anti-matter was that it was theorized before it was discovered. It just naturally comes out of combining Special Relativity with Quantum Mechanics, antimatter *must* exist for both theories to be correct. Neutrinos were also predicted before being discovered. In that case, there needed to be a particle to conserve and carry away the lepton number in weak interactions. BTW I just discovered the AstronomyCast, so I haven't had a chance to listen to them all yet, have they mentioned Supersymmetry yet? That's even cooler. Each fermion/boson would have a boson/fermion superpartner. Photoninos, winos, sleptons, neutralinos, all sorts of crazy names! |
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I would like to hear more about anti-neutrons in a followup show. Is it possible to sequester anti-neutrons in a deuterium atom? Or are the processes that hold atoms stable specific to one flavor of matter?
Oh, and while I'm thinking about it, would it be possible to have a particle with 1 1/3rd charge by combining quarks and anti-quarks? And while we are on the subject of atomic nuclei, what effects do we expect to see of neutron stars as an environment where the strong and weak forces dominate over the electromagnetic force? Kirk Job Sluder, Bloomington, IN |
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I'm not sure about the strong force (i.e. the residual color force between quarks) between a proton and anti-neutron. Obviously mesons can form so there is an attraction, but I don't know how the residual strong force between a hadron and anti-hadron would work out. Quote:
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Or to put it another way, most of the popular science stuff I've read hasn't explained to me how we know that white dwarfs and neutron stars have the properties attributed to them, in contrast to black holes where there is often abundant explanation about density and the emission effects of infalling matter. So a show that talks about the continuum of density and how we infer that neutron stars are made of super-condensed neutrons would be very interesting to me. Neutron stars appear to suffer from the "middle child" syndrome of science writing.
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Pretty much the only technicial explanation I've read was in the big old Gravitation book by Wheeler Thorne and Misner, in fact, I gave a presentation on it in grad school. There are these equations of state that describe how the density and pressure vary as a function of the radial distance from the center of the star. A white dwarf is modelled as a degenerate gas of electrons. Degenerate meaning that the electrons are squeezed as close together as they can possibly can, occupyng all the lowest energy states. This "Fermi pressure" is what keeps the star from collapsing any further. This state is fairly incompressible up to the point where reverse electron capture starts occuring and the electrons start interacting with the quarks in the nucleus via the weak nuclear force. An electron and an up quark get changed into a neutrino and down quark via a W particle exhange. Which basically turns all the protons into neutrons. At that point there's a different equation of state used for the neutron gas. I believe they're still a little unsure as to the exact state of matter in the core though.
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