The primordial gravitational waves have been generated by inflationary
amplification of the primordial (quantum) fluctuations. It is true that they
have not been recorded directly so far, but their spectrum can help a lot in
solving the basic puzzles of the early universe as Inflation (high) energy
scale. In the present work, we give a straightforward method to calculate the
spectral energy density of the relic gravitons different from that used in e.
g. \cite{ mirza04,Latham 2005, Yuki 2006}. The evolution equations are written
in terms of the scale factor (instead of conformal time) and are obtained
through the Lagrange formalism (instead of the transfer function). The presence
of the Hubble parameter allows to calculate the power spectrum in the different
dynamical regimes. The corresponding diagram shows in the universe including
Cosmological Constant the spectral energy density is noticeably enhanced.Comment: 6 pages, 1 figur, 1 tabl