An Effective Field Theory for Large Oscillons
arXiv:2208.04334 · doi:10.1007/JHEP12(2022)079
Abstract
We consider oscillons - localized, quasiperiodic, and extremely long-living classical solutions in models with real scalar fields. We develop their effective description in the limit of large size at finite field strength. Namely, we note that nonlinear long-range field configurations can be described by an effective complex field which is related to the original fields by a canonical transformation. The action for has the form of a systematic gradient expansion. At every order of the expansion, such an effective theory has a global U(1) symmetry and hence a family of stationary nontopological solitons - oscillons. The decay of the latter objects is a nonperturbative process from the viewpoint of the effective theory. Our approach gives an intuitive understanding of oscillons in full nonlinearity and explains their longevity. Importantly, it also provides reliable selection criteria for models with long-lived oscillons. This technique is more precise in the nonrelativistic limit, in the notable cases of nonlinear, extremely long-lived, and large objects, and also in lower spatial dimensions. We test the effective theory by performing explicit numerical simulations of a -dimensional scalar field with a plateau potential.
arXiv comment43 pages, 9 figures, ancillary video of an oscillon formation; Sec. 5 and Appendix extended, references added; journal version
References in corpus (60)
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- Monodromy in the CMB: Gravity Waves and String Inflation
- Gravity Waves and Linear Inflation from Axion Monodromy
- Universality Class in Conformal Inflation
- Understanding the Core-Halo Relation of Quantum Wave Dark Matter, DM, from 3D Simulations
- Axion Miniclusters and Bose Stars
- Oscillons: Resonant Configurations During Bubble Collapse
- Oscillons After Inflation
- Pseudo-Stable Bubbles
- Gravitational Bose-Einstein condensation in the kinetic regime
- Non-Linear Axion Dynamics and Formation of Cosmological Pseudo-Solitons
- More Axions from Strings
- Early-Universe Simulations of the Cosmological Axion
- Formation and structure of ultralight bosonic dark matter halos
- Dilute and dense axion stars
- Early seeds of axion miniclusters
- Analytic Description of Primordial Black Hole Formation from Scalar Field Fragmentation
- Dense Axion Stars
- Formation and mass growth of axion stars in axion miniclusters
- Flat-top oscillons in an expanding universe
- I-balls
- Gravitational perturbations from oscillons and transients after inflation
- New insights into the formation and growth of boson stars in dark matter halos
- Fine Structure of Oscillons in the Spherically Symmetric Klein-Gordon Model
- Gravitational Waves from Oscillon Preheating
- Radiation and Relaxation of Oscillons
- Small amplitude quasi-breathers and oscillons
- Gravitational Waves from Oscillons with Cuspy Potentials
- On Longevity of I-ball/Oscillon
- End of inflation, oscillons and matter-antimatter asymmetry
- Simulations of Axion Minihalos
- Classical Decay Rates of Oscillons
- Emergence of Oscillons in an Expanding Background
- Radio-emission of axion stars
- Review of non-topological solitons in theories with -symmetry
- Radiation of scalar oscillons in 2 and 3 dimensions
- Computation of the radiation amplitude of oscillons
- Axion Stars in the Infrared Limit
- K-Oscillons: Oscillons with Non-Canonical Kinetic Terms
- Instability of rotating Bose stars
- Long-Lived Localized Field Configurations in Small Lattices: Application to Oscillons
- d-dimensional Oscillating Scalar Field Lumps and the Dimensionality of Space
- Simulations of axion-like particles in the post-inflationary scenario
- Oscillons and Dark Matter
- Cosmic bubble and domain wall instabilities III: The role of oscillons in three-dimensional bubble collisions
- Polarized Vector Oscillons
- Stochastic Gravitational-Wave Background from Axion-Monodromy Oscillons in String Theory During Preheating
- Long-lived oscillons from asymmetric bubbles
- The Structure of the Oscillon: The Dynamics of Attractive Self-Interaction
- Long-Lived Time-Dependent Remnants During Cosmological Symmetry Breaking: From Inflation to the Electroweak Scale
- Oscillons from Pure Natural Inflation
- Classical Nonrelativistic Effective Field Theory and the Role of Gravitational Interactions
- Nonrelativistic Effective Field Theory for Axions
- Beyond Schrödinger-Poisson: Nonrelativistic Effective Field Theory for Scalar Dark Matter
- Recipes for Oscillon Longevity
- Adiabatic Invariance of Oscillons/I-balls
- A Class of Nonperturbative Configurations in Abelian-Higgs Models: Complexity from Dynamical Symmetry Breaking
- Solar mass black holes from neutron stars and bosonic dark matter
- Oscillons in Higher-Derivative Effective Field Theories
- Oscillons during Dirac-Born-Infeld Preheating
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