We present a new mechanism that allows to unify inflation and dark energy. We use a scalar field φ with a potential ν(φ) that has two at regions at high and low energies that are associated with inflation and dark energy respectively. After inflation φ decays com- pletely and reheat the universe. Eventually φ is regenerated at late times close to present via a quantum process and the dark energy epoch begins. The φ particles production starts at low energies and this explains the cosmological coincidence problem. Copyright © 2012 by World Scientific Publishing Co. Pte. Ltd.
De La Macorra, A., Briscese, F. (2012). How to obtain dark energy at low energy (late time). In 12th Marcel Grossmann Meeting on Recent Dev. in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories - Proc. of the MG 2009 Meeting on General Relativity (pp.1259-1261). World Scientific Publishing Co. Pte Ltd [10.1142/9789814374552_0184].
How to obtain dark energy at low energy (late time)
Briscese F.
2012-01-01
Abstract
We present a new mechanism that allows to unify inflation and dark energy. We use a scalar field φ with a potential ν(φ) that has two at regions at high and low energies that are associated with inflation and dark energy respectively. After inflation φ decays com- pletely and reheat the universe. Eventually φ is regenerated at late times close to present via a quantum process and the dark energy epoch begins. The φ particles production starts at low energies and this explains the cosmological coincidence problem. Copyright © 2012 by World Scientific Publishing Co. Pte. Ltd.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
