Journal article
Dark Matter in Galaxies: Conference Summary
- Abstract:
-
The competition between CDM and MOND to account for the `missing mass' phenomena is asymmetric. MOND has clearly demonstrated that a characteristic acceleration $a_0$ underlies the data and understanding what gives rise to $a_0$ is an important task. The reason for MOND's success may lie in either the details of galaxy formation, or an advance in fundamental physics that reduces to MOND in a suitable limit. CDM has enjoyed great success on large scales. The theory cannot be definitively teste...
Expand abstract
Actions
Authors
Bibliographic Details
- Publication date:
- 2003-10-08
Item Description
- Keywords:
- Pubs id:
-
pubs:167467
- UUID:
-
uuid:8c1d716d-441a-4415-92ca-0784aced9cdb
- Local pid:
- pubs:167467
- Source identifiers:
-
167467
- Deposit date:
- 2013-02-20
Terms of use
- Copyright date:
- 2003
- Notes:
-
Revised in light of preprint by Milgrom and Sanders (astro-ph/0309617).
To appear in IAU Symposium 220, "Dark Matter in Galaxies", ed. Stuart Ryder,
D.J. Pisano, Mark walker and Ken Freeman, Publ. Astron. Soc. Pac
Metrics
If you are the owner of this record, you can report an update to it here: Report update to this record