Nonperturbative renormalization in a scalar model within Light-Front Dynamics
| dc.creator | Bernard, D. | |
| dc.creator | Cousin, Th. | |
| dc.creator | Karmanov, V. A. | |
| dc.creator | Mathiot, J. -F. | |
| dc.date | 2001-09-27 | |
| dc.date.accessioned | 2026-07-07T11:31:55Z | |
| dc.date.available | 2026-07-07T11:31:55Z | |
| dc.description | Within the covariant formulation of Light-Front Dynamics, in a scalar model with the interaction Hamiltonian $H=-gψ^{2}(x)ϕ(x)$, we calculate nonperturbatively the renormalized state vector of a scalar "nucleon" in a truncated Fock space containing the $N$, $Nπ$ and $Nππ$ sectors. The model gives a simple example of non-perturbative renormalization which is carried out numerically. Though the mass renormalization $δm^2$ diverges logarithmically with the cutoff $L$, the Fock components of the "physical" nucleon are stable when $L\to\infty$. | |
| dc.description | 22 pages, 5 figures | |
| dc.identifier | https://arxiv.org/abs/hep-th/0109208 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0109208 | |
| dc.identifier | Phys.Rev.D65:025016,2002 | |
| dc.identifier | doi:10.1103/PhysRevD.65.025016 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197430 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Nonperturbative renormalization in a scalar model within Light-Front Dynamics | |
| dc.type | text |