Dark matter in the standard model?

Dark Matter in the Finely Tuned Minimal Supersymmetric Standard Model

We explore dark matter in the Finely Tuned Minimal Supersymmetric Standard model recently proposed by Arkani-Hamed and Dimopoulos. Relative to the MSSM, there are fewer particles at freezeout, so the calculation of the relic abundance simplifies. Similarly, the predictions for direct detection of the dark matter sharpen. There is a large region of mixed bino–higgsino dark matter where the light...

Particle Dark Matter from Physics Beyond the Standard Model

So far the existence of the dark matter (DM) is our best experimental evidence for new physics beyond the Standard Model. The most recent WMAP data [1] confirm the standard cosmological model and precisely pin down the amount of cold dark matter as 0.094 < ΩCDMh 2 < 0.129, in accord with earlier indications. Nevertheless, the exact nature of the dark matter still remains a mystery, as all known...

Physics beyond the Standard Model and Dark Matter

Dark Matter in Classically Scale-Invariant Two Singlets Standard Model

We consider a model where two new scalars are introduced in the standard model, assuming classical scale invariance. In this model the scale invariance is broken by quantum corrections and one of the new scalars acquires non-zero vacuum expectation value (VEV), which induces the electroweak symmetry breaking in the standard model, and the other scalar becomes dark matter. It is shown that TeV s...

Dark matter, constrained minimal supersymmetric standard model, and lattice QCD.

Recent lattice measurements have given accurate estimates of the quark condensates in the proton. We use these results to significantly improve the dark matter predictions in benchmark models within the constrained minimal supersymmetric standard model. The predicted spin-independent cross sections are at least an order of magnitude smaller than previously suggested and our results have signifi...