HYREC-2: a highly accurate sub-millisecond recombination code
arXiv:2007.14114 · doi:10.1103/PhysRevD.102.083517
Abstract
We present the new recombination code HYREC-2, holding the same accuracy as the state-of-the-art codes HYREC and COSMOREC and, at the same time, surpassing the computational speed of the code RECFAST commonly used for CMB-anisotropy data analyses. HYREC-2 is based on an effective 4-level atom model, accounting exactly for the non-equilibrium of highly excited states of hydrogen, and very accurately for radiative transfer effects with a correction to the Lyman- escape rate. The latter is computed with the original HYREC, and tabulated, as a function of temperature, along with its derivatives with respect to the relevant cosmological parameters. This enables the code to keep the same accuracy as the original HYREC-2 over the full 99.7% confidence region of cosmological parameters currently allowed by Planck, while running in under one millisecond on a standard laptop. Our code leads to no noticeable bias in any cosmological parameters even in the case of an ideal cosmic-variance limited experiment up to = 5000. Beyond CMB anisotropy calculations, HYREC-2 will be a useful tool to compute various observables that depend on the recombination and thermal history, such as the recombination spectrum or the 21-cm signal.
arXiv comment14pages, 7 Figures, version accepted for publication in PRD
References in corpus (56)
- Planck 2015 results. XIII. Cosmological parameters
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Efficient Computation of CMB anisotropies in closed FRW models
- The Simons Observatory: Science goals and forecasts
- The Temperature of the Cosmic Microwave Background
- A New Calculation of the Recombination Epoch
- The Microwave Anisotropy Probe (MAP) Mission
- CMB power spectrum parameter degeneracies in the era of precision cosmology
- Cosmic microwave background limits on accreting primordial black holes
- How exactly did the Universe become neutral?
- Particle decays during the cosmic dark ages
- Effect of Primordial Black Holes on the Cosmic Microwave Background and Cosmological Parameter Estimates
- Detecting Dark Matter Annihilation with CMB Polarization : Signatures and Experimental Prospects
- HyRec: A fast and highly accurate primordial hydrogen and helium recombination code
- Cosmic Complementarity: H_0 and Omega_m from Combining CMB Experiments and Redshift Surveys
- Cosmological constraints on exotic injection of electromagnetic energy
- The Effect of Physical Assumptions on the Calculation of Microwave Background Anisotropies
- Impact of dark matter decays and annihilations on reionization
- Contraints on radiative dark-matter decay from the cosmic microwave background
- Towards a complete treatment of the cosmological recombination problem
- Induced two-photon decay of the 2s level and the rate of cosmological hydrogen recombination
- Ultrafast effective multi-level atom method for primordial hydrogen recombination
- CMB Anisotropy in the Decaying Neutrino Cosmology
- Lines in the Cosmic Microwave Background Spectrum from the Epoch of Cosmological Hydrogen Recombination
- Could the Cosmological Recombination Spectrum Help Us Understand Annihilating Dark Matter?
- Lines in the cosmic microwave background spectrum from the epoch of cosmological helium recombination
- Recombinations to the Rydberg States of Hydrogen and Their Effect During the Cosmological Recombination Epoch
- Primordial helium recombination I: feedback, line transfer, and continuum opacity
- Decaying particles and the reionization history of the Universe
- Cosmological hydrogen recombination: populations of the high level sub-states
- Full covariance of CMB and lensing reconstruction power spectra
- Two-photon transitions in hydrogen and cosmological recombination
- CMB Delensing Beyond the B Modes
- Two-photon transitions in primordial hydrogen recombination
- Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments
- Non-Gaussian structure of the lensed CMB power spectra covariance matrix
- CMB photons shedding light on dark matter
- Cosmological hydrogen recombination: The effect of extremely high-n states
- Two-Photon 2s<->1s Transitions during Recombination of Hydrogen in the Universe
- CosmoSpec: Fast and detailed computation of the cosmological recombination radiation from hydrogen and helium
- Cosmological hydrogen recombination: Lyn line feedback and continuum escape
- Primordial helium recombination III: Thomson scattering, isotope shifts, and cumulative results
- Lyman-alpha transfer in primordial hydrogen recombination
- Precise cosmological parameter estimation using CosmoRec
- Cosmological Hydrogen Recombination: influence of resonance and electron scattering
- Primordial helium recombination II: two-photon processes
- Time-Dependent Corrections to the Ly-alpha Escape Probability During Cosmological Hydrogen Recombination
- Dynamics of Primordial Hydrogen Recombination with Allowance for a Recoil for Scattering in the Ly-alpha Line
- Effective conductance method for the primordial recombination spectrum
- Radiative transfer effects in primordial hydrogen recombination
- Ly alpha escape during cosmological hydrogen recombination: the 3d-1s and 3s-1s two-photon processes
- HeII->HeI Recombination of Primordial Helium Plasma Including the Effect of Neutral Hydrogen
- Effect of Radiative Feedbacks for Resonant Transitions during Cosmological Recombination
- Reionization Constraints on the Contribution of Primordial Compact Objects to Dark Matter
- Metals at the surface of last scatter
- Cosmology with Recombination Spectrum
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- 21cmFirstCLASS II. Early linear fluctuations of the 21cm signal
- Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
- Cosmological perturbations without the Boltzmann hierarchy
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- Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
- Signatures of inhomogeneous dark matter annihilation on 21-cm
- Magnetic fields from small-scale primordial perturbations
- The magnitude of the dark ages 21-cm signal in the context of existing early and late time constraints on CDM
- Probing small-scale baryon and dark matter isocurvature perturbations with cosmic microwave background anisotropies
- ABCMB: A Python+JAX Package for the Cosmic Microwave Background Power Spectrum
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