PIRSA:05030121

Evaluation of effective rigidity of membrane energy dominated universe model

(2005). Evaluation of effective rigidity of membrane energy dominated universe model. Perimeter Institute. https://pirsa.org/05030121

Evaluation of effective rigidity of membrane energy dominated universe model. Perimeter Institute, Mar. 24, 2005, https://pirsa.org/05030121 

          @misc{ pirsa_PIRSA:05030121,
            doi = {10.48660/05030121},
            url = {https://pirsa.org/05030121},
            author = {},
            keywords = {},
            language = {en},
            title = {Evaluation of effective rigidity of membrane energy dominated universe model},
            publisher = {Perimeter Institute},
            year = {2005},
            month = {mar},
            note = {PIRSA:05030121 see, \url{https://pirsa.org}}
          }
Talk number
PIRSA:05030121
Collection
Talk Type
Abstract
A joint Guelph-Waterloo Gravity Group/Perimeter Institute Seminar --------------------------------------------------------------------------- Observational evidence suggests that the large scale dynamics of the universe is presently dominated by dark energy, meaning a non-luminous cosmological constituent with a negative value of the pressure to density ratio w, which would be unstable if purely fluid, but could be stable if effectively solid with sufficient rigidity. It was suggested by Bucher and Spergel that such a solid constituent might be constituted by an effectively cold (meaning approximately static) distribution of cosmic strings with w=-1/3, or membranes with the observationally favoured value w=-2/3, but it was not established whether the rigidity in such models actually would be sufficient for stabilisation. For cases (exemplified by an approximately O(3) symmetric scalar field model) in which the number of membranes meeting at a junction is even (though not if it is odd) it is easy to obtain an explicit evaluation of the rigidity to density ratio, which is shown to 3/15 in both string and membrane cases, and it is confirmed that this is indeed sufficient for stabilisation.