dc.contributor.author |
Ambjørn, J |
en |
dc.contributor.author |
Anagnostopoulos, K |
en |
dc.contributor.author |
Ichihara, T |
en |
dc.contributor.author |
Jensen, L |
en |
dc.contributor.author |
Kawamoto, N |
en |
dc.contributor.author |
Watabiki, Y |
en |
dc.contributor.author |
Yotsuji, K |
en |
dc.date.accessioned |
2014-03-01T01:46:58Z |
|
dc.date.available |
2014-03-01T01:46:58Z |
|
dc.date.issued |
1998 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/25118 |
|
dc.subject |
Anomalous Dimension |
en |
dc.subject |
Computer Simulation |
en |
dc.subject |
hausdorff dimension |
en |
dc.subject |
Quantum Gravity |
en |
dc.subject |
Space Time |
en |
dc.title |
The quantum space-time of c = −2 gravity |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1016/S0550-3213(97)00659-7 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1016/S0550-3213(97)00659-7 |
en |
heal.publicationDate |
1998 |
en |
heal.abstract |
We study the fractal structure of space-time of two-dimensional quantum gravity coupled to c = −2 conformal matter by means of computer simulations. We find that the intrinsic Hausdorff dimension dH = 3.58 ± 0.04. This result supports the conjecture dH = −2α1/α−1, where αn is the gravitational dressing exponent of a spinless primary field of conformal weight (n + |
en |
heal.journalName |
Nuclear Physics B |
en |
dc.identifier.doi |
10.1016/S0550-3213(97)00659-7 |
en |