Swapnil Kumar SinghCosmology · Gravitation · Engineering

03 · Cosmology

Inflation under ACT DR6 and DESI DR2

Institute of Theoretical Physics · University of Warsaw

March — July 2025Warsaw, Poland

Primordial models enter a narrow observational corridor; only some emerge intact.

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The question

How 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.