Robert H. Sanders is Professor Emeritus at the Kapteyn Astronomical Institute, Groningen, The Netherlands. He has worked in the field of dark matter for many years.
Inhaltsangabe
1. Introduction 2. Early history of the dark matter hypothesis 3. The stability of disk galaxies: the dark halo solutions 4. Direct evidence: extended rotation curves of spiral galaxies 5. The maximum disk: light traces mass 6. Cosmology and the birth of astroparticle physics 7. Clusters revisited: missing mass found 8. CDM confronts galaxy rotation curves 9. The new cosmology: dark matter is not enough 10. An alternative to dark matter: Modified Newtonian Dynamics 11. Seeing dark matter: the theory and practice of detection 12. Reflections: a personal point of view Appendix References Index.
1. Introduction 2. Early history of the dark matter hypothesis 3. The stability of disk galaxies: the dark halo solutions 4. Direct evidence: extended rotation curves of spiral galaxies 5. The maximum disk: light traces mass 6. Cosmology and the birth of astroparticle physics 7. Clusters revisited: missing mass found 8. CDM confronts galaxy rotation curves 9. The new cosmology: dark matter is not enough 10. An alternative to dark matter: Modified Newtonian Dynamics 11. Seeing dark matter: the theory and practice of detection 12. Reflections: a personal point of view Appendix References Index.
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