Cosmological super inflation using Hamilton's approach

Omar E. Núñez, J. Socorro, José Venegas

The Friedmann-Robertson-Walker (FRW) cosmology is analyzed with a particular potential $\mathrm{V}(\varphi )={\mathrm{V}}_0{\mathrm{e}}^{-\sqrt{3}\varphi }$ in the quintessence field scenario, which emerges in the super…