6533b853fe1ef96bd12ad799

RESEARCH PRODUCT

Critical point Higgs inflation in the Palatini formulation

Vera-maria EnckellEemeli TombergSami NurmiSami NurmiSyksy RäsänenSyksy Räsänen

subject

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesRIEMANNGeneral Relativity and Quantum Cosmology (gr-qc)Parameter spaceINITIAL CONDITIONSkosmologia01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyEINSTEINCritical point (thermodynamics)0103 physical sciencesRenormalization Grouplcsh:Nuclear and particle physics. Atomic energy. Radioactivityteoreettinen fysiikkaGENERAL-RELATIVITY010306 general physicscosmology of theories beyond the SMDISSIPATIONBosonMathematical physicsInflation (cosmology)Physics010308 nuclear & particles physicsYukawa potentialCONSTRAINTSBOSONGRAVITATIONRenormalization groupAFFINE VARIATIONAL-PRINCIPLESCosmology of Theories beyond the SMInflection pointHiggs bosonSCALARONlcsh:QC770-798renormalization groupAstrophysics - Cosmology and Nongalactic Astrophysics

description

We study Higgs inflation in the Palatini formulation with the renormalisation group improved potential in the case when loop corrections generate a feature similar to an inflection point. Assuming that there is a threshold correction for the Higgs quartic coupling $\lambda$ and the top Yukawa coupling $y_t$, we scan the three-dimensional parameter space formed by the two jumps and the non-minimal coupling $\xi$. The spectral index $n_s$ can take any value in the observationally allowed range. The lower limit for the running is $\alpha_s>-3.5\times10^{-3}$, and $\alpha_s$ can be as large as the observational upper limit. Running of the running is small. The tensor-to-scalar ratio is $2.2\times 10^{-17}<r<2\times10^{-5}$. We find that slow-roll can be violated near the feature, and a possible period of ultra-slow-roll contributes to the widening of the range of CMB predictions. Nevertheless, for the simplest tree-level action, the Palatini formulation remains distinguishable from the metric formulation even when quantum corrections are taken into account, because of the small tensor-to-scalar ratio.

10.1007/jhep04(2021)059http://repo.scoap3.org/api