Abstract
Certain gravitational eigenstates make excellent candidates for Dark Matter. We discuss these eigenstates, whose invisibility, lifetimes and substantial thermal isolation from the rest of the universe distinguish them from visible baryonic particles with Maxwellian/localisation-determined eigensprectra.
| Original language | English |
|---|---|
| Title of host publication | 20th Australian Institute of Physics Congress, Sydney |
| Subtitle of host publication | incorporating the 37th Australian Conference on Optical Fibre Techology |
| Place of Publication | Sydney |
| Publisher | AIP |
| Pages | 1-4 |
| Number of pages | 4 |
| ISBN (Print) | 9780858259911 |
| Publication status | Published - 2010 |
| Event | Australian Institute of Physics Congress - Melbourne, Vic., Australia Duration: 05 Dec 2010 → 09 Dec 2010 |
Conference
| Conference | Australian Institute of Physics Congress |
|---|---|
| Country/Territory | Australia |
| Period | 05/12/10 → 09/12/10 |