The homogeneous cooling state (HCS) of a granular gas described by the inelastic Boltzmann equation is reconsidered. As usual, particles are taken as inelastic hard disks or spheres, but now the coefficient of normal restitution α is allowed to take negative values α ∈ [−1, 1], a simple way of modeling more complicated inelastic interactions. The distribution function of the HCS is studied at the long-time limit, as well as for intermediate times. At the long-time limit, the relevant information of the HCS is given by a scaling distribution function φ s (c), where the time dependence occurs through a dimensionless velocity c. For α −0.75, φ s remains close to the gaussian distribution in the thermal region, its cumulants and exponential tails being well described by the first Sonine approximation. On the contrary, for α −0.75, the distribution function becomes multimodal, its maxima located at c = 0, and its observable tails algebraic. The latter is a consequence of an unbalanced relaxationdissipation competition, and is analytically demonstrated for α ≃ −1 thanks to a reduction of the Boltzmann equation to a Fokker-Plank-like equation. Finally, a generalized scaling solution to the Boltzmann equation is also found φ(c, β). Apart from the time dependence occurring through the dimensionless velocity, φ(c, β) depends on time through a new parameter β measuring the departure of the HCS from its longtime limit. It is shown that φ(c, β) describes the time evolution of the HCS for almost all times. The relevance of the new scaling is also discussed.