Large field polynomial inflation: parameter space, predictions and (double) eternal nature
نویسندگان
چکیده
Simple monomial inflationary scenarios have been ruled out by recent observations. In this work we revisit the next simplest scenario, a single--field model where scalar potential is polynomial of degree four which features concave ``almost'' saddle point. We focus on trans--Planckian field values. reparametrize potential, greatly simplifies procedure for finding acceptbale parameters. This allows first comprehensive scan parameter space consistent with Planck and BICEP/Keck 2018 measurements. Even values tensor--to--scalar ratio $r$ can be as small $\mathcal{O}(10^{-8})$, but also saturate current upper bound. contrast to small--field version model, radiative stability does not lead strong constraints parameters inflaton potential. For very large approximated quartic term; well known, eternal inflation even energy below reduced mass $M_{\rm Pl}$, Hubble $H \sim 10^{-2} M_{\rm Pl}$. More interestingly, find region that supports {\em two phases inflation}. The second epoch only occurs if slope at would--be point small, has 10^{-5} Pl}$; it realized $r 10^{-2}$, within sensitivity range next--generation CMB
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ژورنال
عنوان ژورنال: Journal of Cosmology and Astroparticle Physics
سال: 2022
ISSN: ['1475-7516', '1475-7508']
DOI: https://doi.org/10.1088/1475-7516/2022/12/005