Variotional perturbation theory and nonperturbative calculations in QCDVariotional
perturbation theory and nonperturbative calculations in QCD
Variational perturbation theory: nonperturbative calculations in QCDVariational
perturbation theory: nonperturbative calculations in QCD
Is it Possible to Match Higher-Twist Contributions with Chiral Perturbation Theory?Is it Possible to Match Higher-Twist Contributions with Chiral
Perturbation Theory?
Rotational evolution of exoplanets under the action of gravitational and magnetic perturbations and magnetic
perturbations. The planet is assumed to be dynamically symmetrical and to be magnetised along its
The nonlinear theory of a spin system's reaction on an external perturbationThe line shape of magnetic resonance absorption is calculated by the nonlinear
theory Hybrid Metric-Palatini Gravity: Black Holes, Wormholes, Singularities, and Instabilities static,
spherically symmetric vacuum solutions of HMPG with the aid of its scalar-tensor
theory (STT
The screening Horndeski cosmologies their
perturbations stay bounded at late times. However, they all turn out to be unstable in the past
Scalar wormholes in a cosmological setting and their instabilityWe construct exact nonstatic nonhomogeneous
spherically symmetric solutions in the
theory Nonlinear electrodynamics and self-gravitating particle-like configurations of such configurations (with respect to
spherically symmetric
perturbations) for all gauge non-invariant Lagrangians L