Constraints on attractor models of inflation and reheating from P l a n c k , BICEP/Keck, ACT DR6, and SPT-3G data
King's College London · European Organization for Nuclear Research · +3 more institutions
Abstract
We analyze the latest cosmic microwave background (CMB) constraints on the scalar spectral index n s and tensor-to-scalar ratio r from 2018, BICEP/Keck 2018, the Atacama Cosmology Telescope Data Release 6 (ACT DR6), and the South Pole Telescope (SPT-3G) data, focusing on their implications for attractor models of inflation. We compare systematically observational bounds with theoretical predictions for both E-model ( α -Starobinsky) and T-model potentials. The observational constraints accommodate E-models with α ≲ 25 , with the canonical Starobinsky model ( α = 1 ) predicting n s = 0.958 – 0.963 for reheating temperatures between 100 − 10 10 GeV , in good agreement with 2018 data and…
Citation impact
- FWCI
- 59.82
- Percentile
- 100%
- References
- 141
Authors
4- JEJohn EllisCorresponding
King's College London, European Organization for Nuclear Research
- MAMarcos A. G. García
Universidad Nacional Autónoma de México
- KAKeith A. Olive
University of Minnesota System
- SVSarunas Verner
University of Chicago
Topics & keywords
- Inflation (cosmology)
- Attractor
- Stability (learning theory)
- Constraint (computer-aided design)
- Decent work and economic growth
Funding
- UDU.S. Department of Energy
- CNConsejo Nacional de Ciencia y TecnologíaAward: CF-2023-I-17
- KIKavli Institute for Cosmological Physics, University of Chicago
- SAScience and Technology Facilities CouncilAward: ST/T000759/1
- DGDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoAward: IA100525