Kinetic recoupling of dark matter
arXiv:2310.20513 · doi:10.1088/1475-7516/2024/07/049
Abstract
We study the possibility that dark matter re-enters kinetic equilibrium with a radiation bath after kinetic decoupling, a scenario we dub kinetic recoupling. This naturally occurs, for instance, with certain types of resonantly-enhanced interactions, or as the result of a phase transition. While late kinetic decoupling damps structure on small scales below a cutoff, kinetic recoupling produces more complex changes in the power spectrum that depend on the nature and extent of the recoupling period. We explore the features that kinetic recoupling imprints upon the matter power spectrum, and discuss how such features can be traced to dark matter microphysics with future observations.
23 pages, 6 figures. Accepted to JCAP
References in corpus (107)
- Dark Matter Substructure in Galactic Halos
- Where are the missing galactic satellites?
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- Observational evidence for self-interacting cold dark matter
- In the Realm of the Hubble tension a Review of Solutions
- Small-Scale Challenges to the CDM Paradigm
- Too big to fail? The puzzling darkness of massive Milky Way subhaloes
- Cold collapse and the core catastrophe
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- Tensions between the Early and the Late Universe
- Dark Matter Self-interactions and Small Scale Structure
- The Kinematics of the Ultra-Faint Milky Way Satellites: Solving the Missing Satellite Problem
- Challenges for CDM: An update
- Reionization and the abundance of galactic satellites
- Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data
- The Core-Cusp Problem
- The Milky Way's bright satellites as an apparent failure of LCDM
- Asymmetric Dark Matter
- The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
- Hydrogen Epoch of Reionization Array (HERA)
- The tumultuous lives of galactic dwarfs and the missing satellites problem
- Formation and evolution of galaxy dark matter halos and their substructure
- Dark Matter Halos as Particle Colliders: A Unified Solution to Small-Scale Structure Puzzles from Dwarfs to Clusters
- New physics in light of the tension: an alternative view
- Dynamical dark energy in light of the latest observations
- Cold dark matter: controversies on small scales
- Review of asymmetric dark matter
- Testing General Relativity in Cosmology
- Substructure and halo density profiles in a Warm Dark Matter Cosmology
- Lyman-alpha constraints on warm and on warm-plus-cold dark matter models
- The Effects of Photoionization on Galaxy Formation - II: Satellites in the Local Group
- A White Paper on keV Sterile Neutrino Dark Matter
- Reconciling Planck with the local value of in extended parameter space
- The first WIMPy halos
- Damping scales of neutralino cold dark matter
- Sommerfeld Enhancements for Thermal Relic Dark Matter
- A Lower Bound on the Mass of Cold Thermal Dark Matter from Planck
- Density Profiles of Cold Dark Matter Substructure: Implications for the Missing Satellites Problem
- Is dark matter with long-range interactions a solution to all small-scale problems of ΛCDM cosmology?
- Small scale problems of the CDM model: a short review
- ETHOS - An Effective Theory of Structure Formation: Dark matter physics as a possible explanation of the small-scale CDM problems
- The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
- Particle Models and the Small-Scale Structure of Dark Matter
- Too Big to Fail in the Local Group
- ETHOS - An Effective Theory of Structure Formation: From dark particle physics to the matter distribution of the Universe
- Resolving the Hubble Tension with New Early Dark Energy
- A Baryonic Solution to the Missing Satellites Problem
- There is No Missing Satellites Problem
- The power spectrum of SUSY-CDM on sub-galactic scales
- What mass are the smallest protohalos?
- A ménage à trois of eV-scale sterile neutrinos, cosmology, and structure formation
- Redefining the Missing Satellites Problem
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
- Effects of cold dark matter decoupling and pair annihilation on cosmological perturbations
- Dark Matter Cores and Cusps: The Case of Multiple Stellar Populations in Dwarf Spheroidals
- Constraining Dark Matter candidates from structure formation
- Big Bang Nucleosynthesis and Particle Dark Matter
- Can Feedback Solve the Too Big to Fail Problem?
- Constraints on Large-Scale Dark Acoustic Oscillations from Cosmology
- Constraints on Dark Matter interactions from structure formation: Damping lengths
- Dark Matter from Early Decays
- Update on Coupled Dark Energy and the tension
- SuperWIMP Solutions to Small Scale Structure Problems
- Narrowing the window for millicharged particles by CMB anisotropy
- Using the Milky Way satellites to study interactions between cold dark matter and radiation
- Interacting Dark Matter disguised as Warm Dark Matter
- Alleviating the and anomalies with a decaying dark matter model
- Implications of a transition in the dark energy equation of state for the and tensions
- Limits on Dark Radiation, Early Dark Energy, and Relativistic Degrees of Freedom
- Probing the Small-Scale Matter Power Spectrum with Large-Scale 21-cm Data
- Kinetic decoupling of neutralino dark matter
- Non-thermal Histories and Implications for Structure Formation
- Charged-particle decay and suppression of small-scale power
- Quantifying the tension with the Redshift Space Distortion data set
- How cold is Dark Matter? Constraints from Milky Way Satellites
- Light dark photon and fermionic dark radiation for the Hubble constant and the structure formation
- MeV Dark Matter and Small Scale Structure
- Suppressing structure formation at dwarf galaxy scales and below: late kinetic decoupling as a compelling alternative to warm dark matter
- Dark matter-radiation interactions: the structure of Milky Way satellite galaxies
- The effect of quark interactions on dark matter kinetic decoupling and the mass of the smallest dark halos
- Accurate estimate of the relic density and the kinetic decoupling in non-thermal dark matter models
- The Galactic Halo in Mixed Dark Matter Cosmologies
- Concentrated Dark Matter: Enhanced Small-scale Structure from Co-Decaying Dark Matter
- A Step in Understanding the Tension
- Self-Interacting Dark Matter and Small-Scale Gravitational Lenses in Galaxy Clusters
- Structure of Dark Matter Halos in Warm Dark Matter models and in models with Long-Lived Charged Massive Particles
- Signatures of Self-Interacting Dark Matter in the Matter Power Spectrum and the CMB
- Testing Dark energy models in the light of tension
- Reannihilation of self-interacting dark matter
- Cannibalism hinders growth: Cannibal Dark Matter and the tension
- Kinetic decoupling of WIMPs: analytic expressions
- Comprehensive Assessment of the Too-Big-to-Fail Problem
- Kinetic Decoupling and Small-Scale Structure in Effective Theories of Dark Matter
- A new astrophysical solution to the Too Big To Fail problem - Insights from the MoRIA simulations
- Investigating the Hubble Constant Tension -- Two Numbers in the Standard Cosmological Model
- Linear scale bounds on dark matter--dark radiation interactions and connection with the small scale crisis of cold dark matter
- ETHOS -- An Effective Theory of Structure Formation: Impact of Dark Acoustic Oscillations on Cosmic Dawn
- Effects of electrically charged dark matter on cosmic microwave background anisotropies
- Millicharged Relics Reveal Massless Dark Photons
- Late Kinetic Decoupling of Light Magnetic Dipole Dark Matter
- Breit-Wigner Enhancement Considering the Dark Matter Kinetic Decoupling
- MIND THE GAP: Is The Too Big To Fail Problem Resolved?
- Constraining structure formation using EDGES
- Snowmass2021 Cosmic Frontier: Report of the CF04 Topical Group on Dark Energy and Cosmic Acceleration in the Modern Universe
- Trading kinetic energy: How late kinetic decoupling of dark matter changes
- Report of the Topical Group on Cosmic Frontier 5 Dark Energy and Cosmic Acceleration: Cosmic Dawn and Before for Snowmass 2021