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Investigation of new methods for numerical stochastic perturbation theory in φ4 theory
- Source :
- Brida, M D, Garofalo, M & Kennedy, A D 2017, ' Investigation of new methods for numerical stochastic perturbation theory in φ4 theory ', Physical Review D, particles, fields, gravitation, and cosmology, vol. 96, no. 5, 054502, pp. 1-22 . https://doi.org/10.1103/PhysRevD.96.054502
- Publication Year :
- 2017
- Publisher :
- American Physical Society, 2017.
-
Abstract
- Numerical stochastic perturbation theory is a powerful tool for estimating high-order perturbative expansions in lattice field theory. The standard algorithms based on the Langevin equation, however, suffer from several limitations which in practice restrict the potential of this technique. In this work we investigate some alternative methods which could in principle improve on the standard approach. In particular, we present a study of the recently proposed instantaneous stochastic perturbation theory, as well as a formulation of numerical stochastic perturbation theory based on generalized hybrid molecular dynamics algorithms. The viability of these methods is investigated in ${\ensuremath{\varphi}}^{4}$ theory.
- Subjects :
- Physics
Work (thermodynamics)
Lattice field theory
010308 nuclear & particles physics
hep-lat
Stochastic quantization
01 natural sciences
Langevin equation
Renormalization
FIS/02 - FISICA TEORICA, MODELLI E METODI MATEMATICI
Molecular dynamics
0103 physical sciences
High-order perturbation theory
Standard algorithms
Perturbation theory (quantum mechanics)
Statistical physics
010306 general physics
Scaling
Langevin equations
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- Brida, M D, Garofalo, M & Kennedy, A D 2017, ' Investigation of new methods for numerical stochastic perturbation theory in φ4 theory ', Physical Review D, particles, fields, gravitation, and cosmology, vol. 96, no. 5, 054502, pp. 1-22 . https://doi.org/10.1103/PhysRevD.96.054502
- Accession number :
- edsair.doi.dedup.....e9b61189bdc889853c95d512b0481c92
- Full Text :
- https://doi.org/10.1103/PhysRevD.96.054502