As shown in the works [1-3], the asymptotic behavior of the propagator in the Euclidean region of momenta for the model of a complex scalar field φ and a real scalar field χ with the interaction drastically changes depending on the value of the coupling constant. For small values of the coupling, the propagator of the field φ behaves asymptotically as free, while in the strong-coupling region the propagator in the deep Euclidean region tends to be a constant.In this paper, the influence of the vacuum stability problem of this model on this critical behavior is investigated. It is shown that within the framework of the approximations used, the addition of a stabilizing term of type to the Lagrangian leads to a renormalization of ...
[出版社版]Copyright notice(c)1998 American Physical Society. All rights reserved. Publisher's version: ...
We study numerically the gravitational collapse of two massless scalar fields in spherical symmetry ...
A recently proposed normalization condition for the imaginary part of the self-energy of an unstable...
We study 3d O(N) symmetric scalar field theories using Polchinski’s renormalization group. In the in...
Abstract We calculate the vacuum stability conditions and renormalisation group equations for the ex...
The leading-order equations of the $$1/N$$ – expansion for a vector-matrix model with interaction $$...
The critical behavior of a nonlocal scalar field theory is studied. This theory has a nonlocal kinet...
A self-contained analysis is given of the simplest quantum fields from the renormalization group poi...
We calculate analytical vacuum stability or bounded from below conditions for general scalar potenti...
The scalar field theory on the background of cosmological models with n(n#>=#1) spaces of constan...
We present a fast and efficient method for studying vacuum stability constraints in multi-scalar the...
We present a fast and efficient method for studying vacuum stability constraints in multi-scalar the...
We study the stability of static, spherically symmetric solutions to the Einstein equations with a s...
Fields which couple directly to the cosmological constant (Λ) may provide a scenario for explai...
International audienceWe revisit the dynamics of a nonminimally coupled scalar field model in case o...
[出版社版]Copyright notice(c)1998 American Physical Society. All rights reserved. Publisher's version: ...
We study numerically the gravitational collapse of two massless scalar fields in spherical symmetry ...
A recently proposed normalization condition for the imaginary part of the self-energy of an unstable...
We study 3d O(N) symmetric scalar field theories using Polchinski’s renormalization group. In the in...
Abstract We calculate the vacuum stability conditions and renormalisation group equations for the ex...
The leading-order equations of the $$1/N$$ – expansion for a vector-matrix model with interaction $$...
The critical behavior of a nonlocal scalar field theory is studied. This theory has a nonlocal kinet...
A self-contained analysis is given of the simplest quantum fields from the renormalization group poi...
We calculate analytical vacuum stability or bounded from below conditions for general scalar potenti...
The scalar field theory on the background of cosmological models with n(n#>=#1) spaces of constan...
We present a fast and efficient method for studying vacuum stability constraints in multi-scalar the...
We present a fast and efficient method for studying vacuum stability constraints in multi-scalar the...
We study the stability of static, spherically symmetric solutions to the Einstein equations with a s...
Fields which couple directly to the cosmological constant (Λ) may provide a scenario for explai...
International audienceWe revisit the dynamics of a nonminimally coupled scalar field model in case o...
[出版社版]Copyright notice(c)1998 American Physical Society. All rights reserved. Publisher's version: ...
We study numerically the gravitational collapse of two massless scalar fields in spherical symmetry ...
A recently proposed normalization condition for the imaginary part of the self-energy of an unstable...