Lisa! said:
Thank you very much.
could you please tell me about other condidates?
The parameters are somewhat defined.
The evidence is pretty clear that dark matter must be non-baryonic. In other words, matter made up of protons, neutrons and similar particles are pretty well ruled out (particles containing quarks other than protons and neutrons are not stable). Thus, very dim stars or large planets (known as MACHOs), interstellar gas, and the like are ruled out. The evidence is also not friendly to black holes as candidates.
The evidence pretty well rules out neutrinos, for reasons discussed before.
There is not evidence that dark matter is electrically charged. Thus, free electrons are ruled out.
We know that dark matter needs to be massive and not emit photons. Gravitons are also not believed to themselves be massive if they exist. Thus, photons themselves are ruled out. Gluons and W/Z particles are either confined to particles composed of quarks or are short lived remnants of them.
This is all rather unfortunate. Because, the evidence has pretty well ruled out all forms of particles known to the standard model.
Also the version of dark matter theory that is the best fit for the evidence is called CDM for Cold Dark Matter. This means that it needs to be relatively slow moving. Basically, we'd like to discover a neutrino-like particle that is massive, electrically neutral and slow moving, that does not interact very strong with anything, just like a neutrino. The acronymn for particles that fit this profile is WIMP for weakly interacting massive particle.
Two of the prime candidates are the proposed "Higgs Boson" a massive particle which mediates a field in the universe that gives rise to inertia, and any of a number of "supersymmetric" particles, such as the neutralino.
Supersymmetry theories are a class of theories which argue for reasons of mathematical symmetry that the world would make more sense if every, or almost every familiar standard model particle had a supersymmetric partner which would be much more massive than the plain vanilla version we see in our particle accellerators, and hence beyond our ability to discover. These would have been common in the early universe and most would have decayed away by now. But, if some kind of supersymmetric particle such as a neutralino (and there are dozens of candidates out there, don't imply consensus from my failure to list them all), that behaved like a WIMP, then this could explain DM.
The big problem with CDM theory is that it requires the bulk of the massive particles in the universe to be made up of some sort of WIMP that isn't made out of anything found in the standard model of particle physics. Thus, while it has the virtue of allowing general relativity's equations to remain essentially unmodified (most CDM theories also require a cosmological constant or some other form of dark energy), we have to go invent some new particle and one can be forgiven for being skeptical of the fact that a ubiquitous constituent of the universe has not yet been encountered. (Have my biases shown here, just a little?)
Now, the trouble is, that if there isn't some new particle, and in fairness, we've discovered all sorts of new particles in the past fifty years, we have to do some major open heart surgery on Einstein's Theory of General Relativity, that remains consistent with all known evidence while modifying those equations in a way that replicates that data currently explained by the majority view in the astrophysical community with dark matter, and has survived nearly a century unmodified, while we've discovered scads of new particles, many of which like the strange and charm and beauty and top quarks, we had no reason to expect existed.
Theoretical physics is in something of a crisis right now, in my view, because the astrophysical data is increasingly suggesting that either the standard model of particle physics, or Einstein's theory of general relativity, which are two of the most fundamental theories of modern physics, must be incomplete (i.e. wrong). Until this is resolved, boards like this one will be interesting places.
The case for the neutralino is made here:
http://web.mit.edu/~redingtn/www/netadv/specr/6/node1.html
Several candidates are evaluated here: http://www.amherst.edu/~rloldershaw/TWIN.HTM which also places boundaries on the properties of dark matter given current data.
Links to many journal articles here: http://www.nu.to.infn.it/Dark_Matter/
This article mentions 20 possible candidate, with the axion, a proposed particle related to charge parity law violations, being the most significant non-supersymmetric candidate. http://arxiv.org/PS_cache/hep-ph/pdf/0404/0404175.pdf