Method for simulating O(N) lattice models at finite density

dc.creatorEndres, Michael G.
dc.date2006-10-03
dc.date2007-03-21
dc.date.accessioned2026-07-07T10:24:48Z
dc.date.available2026-07-07T10:24:48Z
dc.descriptionWe present a method for simulating relativistic and nonrelativistic scalar field theories at finite density, with matter transforming in the fundamental representation of the global symmetry group O(N). The method avoids the problem of complex probability weights which is present in conventional path integral Monte Carlo algorithms. To verify our approach, we simulate the free and interacting relativistic U(1)=O(2) theory in 2+1 dimensions. We compute the two-point correlation function and charge density as a function of chemical potential in the free theory. At weak phi^4 coupling and zero temperature we map the m^2-mu phase diagram and compare our numerical results with perturbative calculations. Finally, we compute properties of theT-mu phase diagram in the vicinity of the phase transition and at bare self-couplings large compared to the temperature and chemical potential.
dc.description27 pages, 14 figures
dc.identifierhttps://arxiv.org/abs/hep-lat/0610029
dc.identifierhttp://arxiv.org/abs/hep-lat/0610029
dc.identifierPhys.Rev.D75:065012,2007
dc.identifierdoi:10.1103/PhysRevD.75.065012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176317
dc.subjectHigh Energy Physics - Lattice
dc.titleMethod for simulating O(N) lattice models at finite density
dc.typetext

Files

Collections