AliCPT Sensitivity to Cosmic Reheating
arXiv:2503.21207 · doi:10.1103/jylc-xw4v
Abstract
We present the first assessment of the Ali Cosmic Microwave Background Polarization Telescope's (AliCPT) sensitivity to the reheating epoch after cosmic inflation, based on its ability to detect primordial gravitational waves. We consider three models of inflation, an -attractor T-model, RGI inflation and QCD-driven warm inflation. Assuming a fiducial value of , we find that AliCPT-1, in its fully loaded focal plane detector configuration and combined with Planck, can provide measurements of the order of magnitude of the reheating temperature with an accuracy around . For QCD-driven warm inflation this can be translated into a constraint on the inflaton coupling to gluons, which can be probed independently in axion search experiments. Our results constitute the first demonstration of AliCPT's ability to probe the initial temperature of the hot big bang and the microphysical parameter connecting cosmic inflation and particle physics.
14 pages, 9 figures. Revised version with a more realistic AliCPT-1 sensitivity forecast, extended to three inflationary models, and an expanded discussion of knowledge gain and model testability
References in corpus (68)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Planck 2015 results. XIII. Cosmological parameters
- The Standard Model Higgs boson as the inflaton
- The Simons Observatory: Science goals and forecasts
- Big Bang Nucleosynthesis: 2015
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- Cosmological Backgrounds of Gravitational Waves
- Universality Class in Conformal Inflation
- Nonperturbative Dynamics Of Reheating After Inflation: A Review
- Planck 2018 results. IV. Diffuse component separation
- First CMB Constraints on the Inflationary Reheating Temperature
- Bounds on very low reheating scenarios after Planck
- The Best Inflationary Models After Planck
- Reheating constraints to inflationary models
- Non-thermal fixed points: effective weak-coupling for strongly correlated systems far from equilibrium
- CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
- Self-resonance after inflation: oscillons, transients and radiation domination
- Non-minimal Inflationary Attractors
- Observing the Inflationary Reheating
- Cosmological Attractors and Initial Conditions for Inflation
- Inflation and the Scale Dependent Spectral Index: Prospects and Strategies
- Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization
- Bayesian Analysis of Inflation II: Model Selection and Constraints on Reheating
- Thermalization after/during Reheating
- Constraints on α-attractor inflation and reheating
- Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope
- Gravitational Waves as a Big Bang Thermometer
- Dark Matter Production in Late Time Reheating
- Minimal Warm Inflation
- Gravitational wave background from Standard Model physics: Qualitative features
- Gravitational wave background from Standard Model physics: Complete leading order
- Thermalization Process after Inflation and Effective Potential of Scalar Field
- Reheating temperature from the CMB
- Quantum theory of fermion production after inflation
- Recent developments in warm inflation
- CMB constraints on the inflaton couplings and reheating temperature in -attractor inflation
- BICEP/Keck Constraints on Attractor Models of Inflation and Reheating
- Thermal QCD Axions across Thresholds
- Information Gain on Reheating: the One Bit Milestone
- Freeze-in from Preheating
- On preheating in alpha-attractor models of inflation
- Increasing Temperature toward the Completion of Reheating
- Minimal warm inflation with complete medium response
- Inflaton phenomenology via reheating in light of primordial gravitational waves and the latest BICEP/ data
- Quantifying the reheating temperature of the universe
- Universality and scaling in multi-field -attractor preheating
- What can the CMB tell about the microphysics of cosmic reheating?
- Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
- Shortcomings of New Parametrizations of Inflation
- WarmSPy: a numerical study of cosmological perturbations in warm inflation
- Shapes of non-Gaussianity in warm inflation
- On finite density effects on cosmic reheating and moduli decay and implications for Dark Matter production
- Upper Bound on Thermal Gravitational Wave Backgrounds from Hidden Sectors
- Spillway Preheating
- Radion Assisted Gauge Inflation
- Tibets Window on Primordial Gravitational Waves
- Warm Inflation with the Standard Model
- LiteBIRD and CMB-S4 Sensitivities to Reheating in Plateau Models of Inflation
- Viability of warm inflation with standard model interactions
- From QFT to Boltzmann: Freeze-in in the presence of oscillating condensates
- WI2easy: warm inflation dynamics made easy
- Warm inflation with a heavy QCD axion
- Evolution of coupled scalar perturbations through smooth reheating. I. Dissipative regime
- Connecting Cosmic Inflation to Particle Physics with LiteBIRD, CMB-S4, EUCLID and SKA
- On Sphaleron Heating in the Presence of Fermions
- The Thermal Feedback Effects on the Temperature Evolution during Reheating
- No Warm Inflation From a Vanilla Axion
- Evolution of coupled scalar perturbations through smooth reheating. II. Thermal fluctuation regime