Warsaw, Poland
03 · Cosmology
Inflation under ACT DR6 and DESI DR2
Institute of Theoretical Physics · University of Warsaw
Primordial models enter a narrow observational corridor; only some emerge intact.
← Return to cosmologyHow strongly do present CMB and large-scale-structure constraints discriminate among non-minimally coupled inflationary scenarios?
FormalismThe mathematical structure will appear here.Derivations · assumptions · limiting cases
ComputationThe numerical experiment will appear here.Simulation · inference · verification
ObservablesThe physical evidence will appear here.Figures · diagnostics · interpretation
The horizon
This page will later hold the model atlas: frame transformations, slow-roll trajectories, parameter scans, and the observational boundary that separates viable histories from elegant failures.