Quintessential Inflation: A Tale of Emergent and Broken Symmetries

Quintessential inflation provides a unified description of inflation and dark energy in terms of a single scalar degree of freedom, the cosmon. We present here a comprehensive overview of this appealing paradigm, highlighting its key ingredients and keeping a reasonable and homogeneous level of details. After summarizing the cosmological evolution in a simple canonical case, we discuss how quintessential inflation can be embedded in a more general scalar-tensor formulation and its relation to variable gravity scenarios. Particular emphasis is placed on the role played by symmetries. In particular, we discuss the evolution of the cosmon field in terms of ultraviolet and infrared fixed points potentially appearing in quantum gravity formulations and leading to the emergence of scale invariance in the early and late Universe. The second part of the review is devoted to the exploration of the phenomenological consequences of the paradigm. First, we discuss how direct couplings of the cosmon field to matter may affect neutrinos masses and primordial structure formation. Second, we describe how Ricci-mediated couplings to spectator fields can trigger the spontaneous symmetry breaking of internal symmetries such as, but not limited to, global (1) or Z(2) symmetries, and affect a large variety of physical processes in the early Universe.

Automated summary

The Quintessential inflation model provides a unified description of inflation and dark energy by introducing a scalar degree of freedom called the cosmon. This paper presents a comprehensive overview of this model, discussing its key ingredients and their implications. It explores the cosmological evolution, the embedding of quintessential inflation in a scalar-tensor framework, and the role of symmetries in the model. The paper also explores the phenomenological consequences of the model, such as its impact on neutrino masses, primordial structure formation, and the spontaneous symmetry breaking of internal symmetries.