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Analysis

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.

Analysis

This paper explores an extension of the Standard Model to address several key issues: neutrino mass, electroweak vacuum stability, and Higgs inflation. It introduces vector-like quarks (VLQs) and a right-handed neutrino (RHN) to achieve these goals. The VLQs stabilize the Higgs potential, the RHN generates neutrino masses, and the model predicts inflationary observables consistent with experimental data. The paper's significance lies in its attempt to unify these disparate aspects of particle physics within a single framework.
Reference

The SM+$(n)$VLQ+RHN framework yields predictions consistent with the combined Planck, WMAP, and BICEP/Keck data, while simultaneously ensuring electroweak vacuum stability and phenomenologically viable neutrino masses within well-defined regions of parameter space.