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Fine Structure of Oscillons in the Spherically Symmetric $\phi^4$ Klein-Gordon Model

3 Pith papers cite this work, alongside 115 external citations. Polarity classification is still indexing.

3 Pith papers citing it
115 external citations · Pith
abstract

We present results from a study of the fine structure of oscillon dynamics in the 3+1 spherically symmetric Klein-Gordon model with a symmetric double-well potential. We show that in addition to the previously understood longevity of oscillons, there exists a resonant (and critical) behavior which exhibits a time-scaling law. The mode structure of the critical solutions is examined, and we also show that the upper-bound to oscillon formation (in $r_0$ space) is either non-existent or higher than previously believed. Our results are generated using a novel technique for implementing non-reflecting boundary conditions in the finite difference solution of wave equations. The method uses a coordinate transformation which blue-shifts and ``freezes'' outgoing radiation. The frozen radiation is then annihilated via dissipation explicitly added to the finite-difference scheme, with very little reflection into the interior of the computational domain.

fields

gr-qc 2 hep-th 1

representative citing papers

Unified theory of oscillons and modes

hep-th · 2026-06-21 · unverdicted · novelty 6.0

Oscillons are reinterpreted as localized resonant modes from threshold or antibound modes via nonlinearity, with wobblerons as new kink-oscillon bound states.

Dynamical Boson Stars

gr-qc · 2012-02-27 · unverdicted · novelty 2.0

Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.

citing papers explorer

Showing 3 of 3 citing papers.

  • Unified theory of oscillons and modes hep-th · 2026-06-21 · unverdicted · none · ref 5 · internal anchor

    Oscillons are reinterpreted as localized resonant modes from threshold or antibound modes via nonlinearity, with wobblerons as new kink-oscillon bound states.

  • Dynamical Boson Stars gr-qc · 2012-02-27 · unverdicted · none · ref 272 · internal anchor

    Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.

  • Testing the nature of dark compact objects: a status report gr-qc · 2019-04-10 · accept · none · ref 126

    Current and future observations can test whether dark compact objects are Kerr black holes or exotic alternatives, with null results strengthening the black hole paradigm.