Dynamics of mean spherical model with correlated noise
The dynamics of the mean spherical model [1, 2, 3] with a dissipative term and a correlated noise is investigated. This noise obeys a fractional brownian motion [4] with Hurst index $H$, and some mathematical techniques are proposed to obtain asymptotically exact results for large times. The analysis is based on the two-time autocorrelation and response function, and the results are compared to the work of Godr?che-Luck [5], where the noise is uncorrelated (it is worth noting that this problem has been considered before [6]). Comparing the two dynamics (which differ in the nature of the noise only), the present case shows a richer behavior, which is expected due to the presence of an extra parameter $H$; nevertheless, one can also observe the realization of some non-trivial interplay between dissipative part and noise term.
[1] T. H. Berlin and M. Kac, Phys. Rev. 86, 821 (1952)
[2] H. W. Lewis and G. H. Wannier, Phys. Rev. 88, 682 (1952)
[3] H. W. Lewis and G. H. Wannier, Phys. Rev. 90, 1131 (1953)
[4] B. B. Mandelbrot and J. W. Van Ness, SIAM Review 10, 422 (1968)
[5] C. Godr?che and J. -M. Luck, J. Phys. A 33, 9141 (2000)
[6] G. Ronca, J. Chem. Phys. 68, 3737 (1978)