Constraints on interacting dynamical dark energy and a new test for $$\Lambda $$ CDM

The European Physical Journal C - Tập 79 - Trang 1-8 - 2019
Marco Bonici1,2, Nicola Maggiore1,2
1Dipartimento di Fisica, Università di Genova, Genova, Italy
2I.N.F.N.-Sezione di Genova, Genova, Italy

Tóm tắt

We consider a generic description of interacting dynamical Dark Energy, characterized by an equation of state with a time dependent coefficient w(t), and which may interact with both radiation and matter. Without referring to any particular cosmological model, we find a differential equation which must be satisfied by w(t) and involving the function Q(t) which describes the interaction between Dark Energy and the other cosmological fluids. The relation we find represents a constraint for various models of interacting dynamical Dark Energy. In addition, an observable is proposed, depending on kinematic variables and on density parameters, which may serve as a new test for $$\Lambda $$ CDM.

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