Due to universality and attractor properties, α-attractor quintessential inflation establishes direct relations between inflationary observables such as the scalar tilt ns and the tensor-to-scalar ratio r, and late-time dark energy equation of state parameters w0 and wa. In this work, we examine three different physically motivated regimes, considering complete freedom in the parameter α, models inspired by supergravity where α takes on values up to α=7/3, and Starobinsky inflation (α=1). We investigate the consistency and constraints imposed by Cosmic Microwave Background measurements from the Planck satellite, B-mode polarization data from the BICEP/Keck collaboration, and low-redshift observations. Additionally, we consider small-scale CMB measurements released by the Atacama Cosmology Telescope, which give results approaching the Harrison-Zel’dovich spectrum (ns≈1). Here α-attractors lead to an improved fit over ΛCDM. For the large-scale CMB measurements, α≳2 models can provide equally good fits as ΛCDM.
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