Author:
Lynker Monika,Schimmrigk Rolf
Abstract
Abstract
One of the fundamental questions in inflation is how to characterize the structure of
different types of models in the field theoretic landscape. Proposals in this direction include
attempts to directly characterize the formal structure of the theory by considering complexity
measures of the potentials. An alternative intrinsic approach is to focus on the behavior of the
observables that result from different models and to ask whether their behavior differs among
models. This type of analysis can be applied even to nontrivial multifield theories where a
natural measure of the complexity of the model is not obvious and the analytical evaluation of the
observables is often impossible. In such cases one may still compute these observables
numerically and investigate their behavior. One interesting case is when observables show a
scaling behavior, in which case theories can be characterized in terms of their scaling amplitudes
and exponents. Generically, models have nontrivial parameter spaces, leading to exponents that are
functions of these parameters. In such cases we consider an iterative procedure to determine
whether the exponent functions in turn lead to a scaling behavior. We show that modular inflation
models can be characterized by families of simple scaling laws and that the scaling exponents that
arise in this way in turn show scaling in dependence of the varying energy scales.
Subject
Astronomy and Astrophysics
Cited by
1 articles.
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