Oscillon of Ultra-Light Axion-like Particle
arXiv:1909.10805 · doi:10.1088/1475-7516/2020/01/047
Abstract
Ultra-light axion-like particle (ULAP) is one of attractive candidates for cold dark matter. Because the de Broglie wavelength of ULAP with mass is , the suppression of the small scale structure by the uncertainty principle can solve the core-cusp problem. Frequently, ULAP is assumed to be uniformly distributed in the present universe. In typical ULAP potentials, however, strong self-resonance at the beginning of oscillation invokes the large fluctuations, which may cause the formation of the dense localized object, oscillon. % Such a dense object lives for a long time, it may affect the cosmological evolution. In this paper, we confirm the oscillon formation in a ULAP potential by numerical simulation and analytically derive its lifetime.
arXiv comment10 pages, 2 figures
References in corpus (50)
- A Universal Density Profile from Hierarchical Clustering
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Towards the Theory of Reheating After Inflation
- Cold and Fuzzy Dark Matter
- Ultralight scalars as cosmological dark matter
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- Universe Reheating after Inflation
- Monodromy in the CMB: Gravity Waves and String Inflation
- Gravity Waves and Linear Inflation from Axion Monodromy
- Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data
- Universality Class in Conformal Inflation
- Superconformal Inflationary -Attractors
- Understanding the Core-Halo Relation of Quantum Wave Dark Matter, DM, from 3D Simulations
- The Observed properties of Dark Matter on small spatial scales
- First constraints on fuzzy dark matter from Lyman- forest data and hydrodynamical simulations
- A search for ultra-light axions using precision cosmological data
- Axion Miniclusters and Bose Stars
- The Dark Matter Distribution in Disk Galaxies
- A universal attractor for inflation at strong coupling
- Oscillons: Resonant Configurations During Bubble Collapse
- High-resolution dark matter density profiles of THINGS dwarf galaxies: Correcting for non-circular motions
- Oscillons After Inflation
- Pseudo-Stable Bubbles
- Non-Thermal Phase Transitions after Inflation
- Gravitational Bose-Einstein condensation in the kinetic regime
- On the Origin of Cusps in Dark Matter Halos
- Self-resonance after inflation: oscillons, transients and radiation domination
- Formation and structure of ultralight bosonic dark matter halos
- Dilute and dense axion stars
- Cosmological Constraints on Bose-Einstein-Condensed Scalar Field Dark Matter
- Search for axion-like dark matter through nuclear spin precession in electric and magnetic fields
- Galaxy UV-luminosity function and reionization constraints on axion dark matter
- Simple exercises to flatten your potential
- Dense Axion Stars
- Lyman- forest and non-linear structure characterization in Fuzzy Dark Matter cosmologies
- I-balls
- Spin Precession Experiments for Light Axionic Dark Matter
- Phase transitions between dilute and dense axion stars
- Catastrophic Particle Production under Periodic Perturbation
- Axion Dark Matter Search with Interferometric Gravitational Wave Detectors
- The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos
- On Longevity of I-ball/Oscillon
- Gravitational wave forest from string axiverse
- Decay of I-ball/Oscillon in Classical Field Theory
- Constraints on axionlike dark matter with masses down to eV/c
- Pure Natural Inflation
- Oscillons from Pure Natural Inflation
- Adiabatic Invariance of Oscillons/I-balls
- Fragileness of Exact I-ball/Oscillon
Cited by in corpus (19)
- Classical Decay Rates of Oscillons
- The Structure of the Oscillon: The Dynamics of Attractive Self-Interaction
- Friendship in the Axiverse: Late-time direct and astrophysical signatures of early-time nonlinear axion dynamics
- Oscillon collapse to black holes
- Recipes for Oscillon Longevity
- Dipole Radiation and Beyond from Axion Stars in Electromagnetic Fields
- Modifying PyUltraLight to model scalar dark matter with self-interactions
- Oscillon formation from preheating in asymmetric inflationary potentials
- Nonperturbative structure in coupled axion sectors and implications for direct detection
- Oscillon spectroscopy
- Oscillons of Axion-Like Particle: Mass distribution and power spectrum
- Inclusion of radiation in the CCM approach of the model
- Non-topological solitons and quasi-solitons
- Probing Oscillons of Ultra-Light Axion-like Particle by 21cm Forest
- Understanding oscillons: standing waves in a ball
- Anisotropies in Cosmological 21 cm Background by Oscillons/I-balls of Ultra-light Axion-like Particle
- Revisiting oscillon formation in KKLT scenario
- Nonlinear dynamics of oscillons and transients during preheating after single field inflation
- Decay and lifetime of oscillons coupled to an external scalar field: Insights from instability band analysis