dc.contributor.author | Anagnostopoulos, K | en |
dc.contributor.author | Azuma, T | en |
dc.contributor.author | Nishimura, J | en |
dc.date.accessioned | 2014-03-01T01:59:01Z | |
dc.date.available | 2014-03-01T01:59:01Z | |
dc.date.issued | 2010 | en |
dc.identifier.uri | https://dspace.lib.ntua.gr/xmlui/handle/123456789/28831 | |
dc.relation.uri | http://arxiv.org/abs/1010.0957 | en |
dc.subject | Configuration Space | en |
dc.subject | Density of State | en |
dc.subject | Eigenvalues | en |
dc.subject | Factorization Method | en |
dc.subject | Finite Size Scaling | en |
dc.subject | Free Energy | en |
dc.subject | Matrix Model | en |
dc.subject | Moment of Inertia | en |
dc.subject | Monte Carlo Simulation | en |
dc.subject | Numerical Method | en |
dc.subject | Path Integral | en |
dc.subject | String Theory | en |
dc.subject | Symmetry Breaking | en |
dc.subject | Space Time | en |
dc.title | A Study of the Complex Action Problem in a Simple Model for Dynamical Compactification in Superstring Theory Using the Factorization Method | en |
heal.type | journalArticle | en |
heal.publicationDate | 2010 | en |
heal.abstract | The IIB matrix model proposes a mechanism for dynamically generating fourdimensional space--time in string theory by spontaneous breaking of the tendimensional rotational symmetry $\textrm{SO}(10)$. Calculations using theGaussian expansion method (GEM) lend support to this conjecture. We study asimple $\textrm{SO}(4)$ invariant matrix model using Monte Carlo simulationsand we confirm that its rotational symmetry breaks down, showing | en |
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