Involutive Spacetime Distributions and p-Brane Dynamics
Mukherjee, Manash
arXiv, 9707013 / Harvested from arXiv
We propose a precise definition of multidimensional fluids generated by self-gravitating extended objects such as strings and membranes: a p-dimensional perfect fluid is a smooth involutive p-dimensional distribution on a spacetime, each integral manifold of which is a timelike, connected, immersed submanifold of dimension, p -- representing the history of a (p-1)-dimensional extended object. This geometric formulation of perfect fluids of higher dimensions naturally leads to the associated stress-energy tensor. Furthermore, the laws of temporal evolution and symmetries of such systems are derived, in general, from the Einstein field equations and the integrability conditions. We also present a matter model based on a 2-dimensional involutive distribution, and it is shown that the stress-energy tensor for self-gravitating strings gives rise to a non-trivial spherically symmetric spacetime with a naked singularity.
Publié le : 1997-07-14
Classification:  Mathematical Physics
@article{9707013,
     author = {Mukherjee, Manash},
     title = {Involutive Spacetime Distributions and p-Brane Dynamics},
     journal = {arXiv},
     volume = {1997},
     number = {0},
     year = {1997},
     language = {en},
     url = {http://dml.mathdoc.fr/item/9707013}
}
Mukherjee, Manash. Involutive Spacetime Distributions and p-Brane Dynamics. arXiv, Tome 1997 (1997) no. 0, . http://gdmltest.u-ga.fr/item/9707013/