Particle Dark Matter: What Comes Next?


Bertone, G. (2008). Particle Dark Matter: What Comes Next?. Perimeter Institute. https://pirsa.org/08060029


Bertone, Gianfranco. Particle Dark Matter: What Comes Next?. Perimeter Institute, Jun. 02, 2008, https://pirsa.org/08060029


          @misc{ pirsa_08060029,
            doi = {10.48660/08060029},
            url = {https://pirsa.org/08060029},
            author = {Bertone, Gianfranco},
            keywords = {Quantum Fields and Strings, Particle Physics, Cosmology},
            language = {en},
            title = {Particle Dark Matter: What Comes Next?},
            publisher = {Perimeter Institute},
            year = {2008},
            month = {jun},
            note = {PIRSA:08060029 see, \url{https://pirsa.org}}

Gianfranco Bertone University of Padova - Department of Mathematics


After a brief introduction, where I review the properties of the \'good Dark Matter candidate\' and the status of accelerator, direct and indirect Dark Matter searches, I will show that a conclusive identification of DM particles can most likely be achieved only through a \'multidisciplinary\' approach, that combines together different detection techniques. I will place special emphasis on the upcoming Large Hadron Collider, and on the gamma-ray satellite GLAST (scheduled for launch on June 3, i.e. the day after the talk...)