Gravitating M(atrix) Q-Balls
| dc.creator | Rey, Soo-Jong | |
| dc.date | 1997-11-11 | |
| dc.date | 1997-11-12 | |
| dc.date.accessioned | 2026-07-07T04:23:51Z | |
| dc.date.available | 2026-07-07T04:23:51Z | |
| dc.description | Q-ball configuration that represents oscillating or spinning closed membrane is constructed via M(atrix) theory. Upon gravitational collapse Q-balls are expected to form Schwarzschild black holes. For quasi-static spherical membrane, we probe spacetime geometry induced by monopole moment via D0-parton scattering off the Q-ball. We find a complete agreement with long distance potential calculated using eleven-dimensional supergravity. Generalizing to heterotic M(atrix) theory, we also construct Q-ball configurations of real projective and disk membranes. The latter Q-ball configuration arises as twisted sector of heterotic M(atrix) theory, hence, are expected to form a charged black hole after gravitational collapse. | |
| dc.description | Latex, no figures | |
| dc.identifier | https://arxiv.org/abs/hep-th/9711081 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9711081 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/55194 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Gravitating M(atrix) Q-Balls | |
| dc.type | text |