Dark matters |
| |
| Institution: | 1. Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW 2006, Australia;2. School of Aerospace, Mechanical and Mechatronic Engineering, J07, The University of Sydney, NSW 2006, Australia;1. Department of Biochemistry and Molecular Genetics, University of Colorado Denver, Anschutz Medical Campus, Aurora, CO, USA;2. International Consultancy in Blood Component Quality/Safety Improvement, Audit/Inspection and DDR Strategies, London, UK;1. Observatoire des Sciences de l''Univers en région Centre, UMS 3116, Université d''Orléans, 1A rue de la Férollerie, 45071 Orléans, France;2. Pôle de Physique, Collegium Sciences et Techniques, Université d''Orléans, Rue de Chartres, 45100 Orléans, France;3. Laboratoire de Physique et Chimie de l''Environnement et de l''Espace, UMR 7328 Centre Nationale de la Recherche Scientifique, LPC2E, Campus CNRS, 3A Avenue de la Recherche Scientifique, 45071 Orléans, France;4. Theoretical Particle Physics and Cosmology Group, Physics Department, King''s College London, Strand, London WC2R 2LS, United Kingdom;5. Theoretical Physics Department, CERN, CH-1211 Genève 23, Switzerland;6. Department of Physics, New York University, 4 Washington Place, New York, NY 10003, United States;7. Physics Department, Manhattan College, 4513 Manhattan College Parkway, Riverdale, NY 10471, United States;8. Experimental Physics Department, CERN, CH-1211 Genève 23, Switzerland;9. Department of Physics, The University of Texas at Arlington, 502 Yates Street, Box 19059, Arlington, TX 76019, United States |
| |
| Abstract: | Despite the new results on the estimate of cosmological parameters, the need for dark matter, both baryonic and nonbaryonic, galactic and intergalactic, is still with us. For baryonic dark matter the remaining possibilities are mostly either intergalactic hot gas or massive compact halo objects. For nonbaryonic dark matter the most likely candidates are the so-called WIMPs, the prototype of which could be the lightest supersymmetric particle. These particles are actively searched for at accelerators and, in our neighborhood, through direct detection or by their annihilation products. |
| |
| Keywords: | |
| 本文献已被 ScienceDirect 等数据库收录！ |
|
