The problem of spin diffusion is studied numerically in one-dimensional classical Heisenberg model using a deterministic odd even spin precession dynamics. We demonstrate that spin diffusion in this model, like energy diffusion, is normal and one obtains a long time diffusive tail in the decay of autocorrelation function (ACF). Some variations of the model with different coupling schemes and with anisotropy are also studied and we find normal diffusion in all of them. A systematic finite size analysis of the Heisenberg model also suggests diffusive spreading of fluctuation, contrary to previous claims of anomalous diffusion.The classical Heisenberg model [1,2] has been extensively studied, both analytically and numerically, for several decades and has become a prototypical model for magnetic insulators. However, one important question that still awaits a conclusive answer is regarding the time dependent behavior of the spins, particularly at very high temperature. In the hydrodynamic limit, the dominant mode of fluctuation spreading in this system is believed to obey of the standard diffusion phenomenology. In absence of any microscopic theoretical formalism, studies were mostly numerical, generally involving calculation of time correlation functions. Although the phenomenology of spin diffusion is an old concept [3,4], its validity in classical Heisenberg model has been vigourously debated in recent times. Although much effort [13][14][15][16][17][18][19][20] has been devoted to understand whether spin diffusion in this system is normal or anomalous, a convincing conclusion is yet to be reached. Settling this question is not only conceptually important e.g., in understanding transport properties of spin systems, but also has direct implications in routinely performed experiments e.g., NMR and ESR in magnetic compounds [5][6][7][8][9]. In the following, we present a brief outline of the diffusion phenomenology and review some of the earlier studies in this direction.Let us consider a one-dimensional chain containing Heisenberg spins { S i } (three dimensional unit vectors) where, i = 1, 2, . . . , N with periodic boundary conditions, i.e., S N +1 ≡ S 1 . The Hamiltonian is given by,where K i is the interaction strength between the spins S i and S i+1 ; the spin-spin coupling is ferromagnetic for K i > 0 and anti-ferromagnetic if K i < 0. The microscopic equation of motion can be written as, is the local molecular field experienced by the spin at site i. Clearly, Eq. (2) conserves (i) the total energy, and (ii) the total spin S = i S i . Since there is no long range order in this system at any finite temperature and because of the conservation of total spin, the spin fluctuation in the hydrodynamic limit is expected to follow a continuity (diffusion) equation ∂ t S q (t) = −D s q 2 S q (t), where S q (t) is the (discrete) Fourier transform of S i (t) and D s is the spin diffusion constant. A similar equation holds for the energy density (since total energy is also a constant of motion). The continuity equation im...