Bubbling AdS and Vacuum String Field Theory
dc.contributor.area | Physics | en_US |
dc.contributor.author | Bonora, Loriano | en_US |
dc.contributor.author | Maccaferri, Carlo | en_US |
dc.contributor.author | Scherer Santos, Ricardo Jose | en_US |
dc.contributor.author | Tolla, Driba Demissie | en_US |
dc.contributor.department | Elementary Particle Theory | en_US |
dc.date.accessioned | 2006-04-12T09:01:49Z | en_US |
dc.date.accessioned | 2011-09-07T20:27:40Z | |
dc.date.available | 2006-04-12T09:01:49Z | en_US |
dc.date.available | 2011-09-07T20:27:40Z | |
dc.date.issued | 2006-04-12T09:01:49Z | en_US |
dc.description.abstract | We show that a family of 1/2--BPS states of $\N=4$ SYM is in correspondence with a family of classical solutions of VSFT with a $B$--field playing the role of the inverse Planck constant. We show this correspondence by relating the Wigner distributions of the $N$ fermion systems representing such states, to low energy space profiles of systems of VSFT D-branes. In this context the Pauli exclusion principle appears as a consequence of the VSFT projector equation. The family of 1/2--BPS states maps through coarse--graining to droplet LLM supergravity solutions. We discuss the possible meaning of the corresponding coarse graining in the VSFT side. | en_US |
dc.format.extent | 291607 bytes | en_US |
dc.format.mimetype | application/pdf | en_US |
dc.identifier.citation | Nucl. Phys. B 749 (2006) 338-357 | en_US |
dc.identifier.uri | https://openscience.sissa.it/handle/1963/1810 | en_US |
dc.language.iso | en_US | en_US |
dc.relation.ispartofseries | SISSA;04/2006/EP | en_US |
dc.relation.ispartofseries | arXiv.org;hep-th/0602015 | en_US |
dc.relation.uri | 10.1016/j.nuclphysb.2006.05.029 | en_US |
dc.title | Bubbling AdS and Vacuum String Field Theory | en_US |
dc.type | Preprint | en_US |