Cosmological consequences of a dynamical dark matter in the light of DESI DR2 measurements

Recent DESI results exhibit preference for a Null Energy Condition violating dynamical dark energy, with early phantom behaviour. We explore an alternative interpretation in which this preference arises from unconventional dark matter dynamics rather than from dynamical dark energy. We propose a dynamical dark matter (DDM) model, with a non-zero equation of state (EoS) that smoothly interpolates between early time and late time asymptotes across a transition scale factor a t, and study its consequences against cosmological datasets including CMB, DESI DR2 BAO, SNeIa (PantheonPlus, Union3, and DESY5) and growth rate data. We find the early time EoS to be consistent with zero, while the present day value is negative at a significance ranging from 0.42 sigma to 3.02 sigma depending on the dataset combination. The strongest preference occurs from the combination of CMB, DESI, and DESY5 giving the present day EoS to be-0.060+0.013-0.028 and a t = 0.41+0.088-0.13 at 68% CL. This preference for a non-zero, late time DM EoS persists when growth rate data are included and across all three SNeIa compilations considered, while the matter density m mildly shifts to higher values relative to CDM. The model also predicts a lower sigma 8 and S 8 than CDM, in better agreement with weak-lensing data, while H 0 remains unchanged and in tension with local distance-ladder measurements. The DDM model is preferred over CDM (chi squared MAP = -14.093, DIC = -7.838 for Planck+DESI+DESY5) but disfavored relative to the CPL parameterization of DE (chi squared MAP = 6.755, DIC = 7.966). This preference is consistent among other combination of datasets as well.