Search for Dark Matter by GENIUSTF and GENIUS.pdfVIP

1 Search for Dark Matter by GENIUS-TF and GENIUS H.V. Klapdor-Kleingrothaus a∗ aMax-Planck-Institut f¨ur Kernphysik, P.O. Box 10 39 80, D-69029 Heidelberg, GERMANY 2 0 The new project GENIUS will cover a wide range of the parameter space of predictions of SUSY for neutralinos 0 as cold dark matter. Together with DAMA it will be the only experiment which can probe the seasonal modulation 2 signal. Concerning hot dark matter GENIUS will be able to fix the (effective) neutrino mass with high accuracy. n A GENIUS Test Facility has just been funded and will come into operation by end of 2002. u J 5 1. GENERAL SITUATION sively analysed in many variants of SUSY models. 2 Fig. 1 represents the present situation. The Dark matter is at present one of the most ex- SUSY predictions are from the MSUGRA model 1 citing fields of particle physics and cosmology. [2] and the MSSM with relaxed unification con- v Recent investigations of the CMB (MAXIMA, ditions [1]. Fig. 2 shows the result of a study 0 5 BOOMERANG, DASI) together with large scale ’at Post-LEP Benchmark points’ based again on 2 structure results fix the non-baryonic dark mat- the MSUGRA [3]. Present experiments only just 6 ter contribution to the mass of the Universe to ∼ touch the border of the area predicted by the 0 25%, of which still up to 38% could be hot (neu- MSSM. The experimental DAMA evidence for 2 trinos). With the early nucleosynthesis constraint dar