exponent137 said:
lpetrich said:
The nature of dark matter and dark energy are obscure, though they cannot be Standard-Model particles.
Is this sure? Why not to built all matter?
exponent137, consider what would happen if a putative dark-matter particle has QCD or electromagnetic interactions.
Short-short summary: it would act just like baryonic matter, the familiar kind, and it would produce various anomalies that we don't observe. See if you can try to work out some of them. Imagine some particle between 10 GeV and 10 TeV, say, 100 GeV or 1 TeV, with electric charge +1 or -1, or QCD multiplicity 3 (quarklike; electric charge -1/3+n), 3* (antiquarklike; electric charge +1/3+n), or 8 (gluonlike; electric charge n).
Seems like a good exercise for students in a particle-physics or astrophysics course.
So the only Standard-Model that has the right interactions for a dark-matter particle are neutrinos. But there's a problem: neutrinos' masses are too small, <~ 0.1 eV. They aren't massive enough to become "cold dark matter", the most common kind.
That's why dark-matter elementary particles cannot be Standard-Model particles.
The question appears a lot of times, what gives mass to Higgs boson?
In the Standard Model, the Higgs particle is self-interacting, and its self-interactions generate its mass.
For field strength f, its potential looks like V(f) = (1/2)*V
2*f
2 + (1/2)*V
4*f
4
The second term is a self-interaction term.
Find its minimum. That requires solving dV(f)/df = 0, giving f*(V
2 + V
4*f
2) = 0
Consider each solution's stability. Find d
2V/df
2 = V
2 + 3*V
4*f
2.
If > 0, then it's stable; if < 0, then it's unstable; if = 0, then it's borderline.
Solutions.
f = 0. Second derivative = V
2
If V
2 < 0, then there's another solution:
f = sqrt(- V
2/V
4)
The f = 0 solution is unstable, but this solution has second derivative -2V
2 > 0, meaning that it's stable. A Higgs particle will have V
2 < 0, making this solution stable, complete with nonzero f.
That's what's behind the analogy of a marble in a bowl with a central hump.