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This paper investigates Higgs-like inflation within a specific framework of modified gravity (scalar-torsion $f(T,φ)$ gravity). It's significant because it explores whether a well-known inflationary model (Higgs-like inflation) remains viable when gravity is described by torsion instead of curvature, and it tests this model against the latest observational data from CMB and large-scale structure surveys. The paper's importance lies in its contribution to understanding the interplay between inflation, modified gravity, and observational constraints.
Reference

Higgs-like inflation in $f(T,φ)$ gravity is fully consistent with current bounds, naturally accommodating the preferred shift in the scalar spectral index and leading to distinctive tensor-sector signatures.