In applied mathematics and mathematical analysis, the fractal derivative or Hausdorff derivative is a non-Newtonian generalization of the derivative dealing with the measurement of fractals, defined in fractal geometry. Fractal derivatives were created for the study of anomalous diffusion, by which traditional approaches fail to factor in the fractal nature of the media. A fractal measure t is scaled according to tα. Such a derivative is local, in contrast to the similarly applied fractional derivative. Fractal calculus is formulated as a generalization of standard calculus.[1]
Porous media, aquifers, turbulence, and other media usually exhibit fractal properties. Classical diffusion or dispersion laws based on random walks in free space (essentially the same result variously known as Fick's laws of diffusion, Darcy's law, and Fourier's law) are not applicable to fractal media. To address this, concepts such as distance and velocity must be redefined for fractal media; in particular, scales for space and time are to be transformed according to (xβ, tα). Elementary physical concepts such as velocity are redefined as follows for fractal spacetime (xβ, tα):[2]
v'=
dx' | = | |
dt' |
dx\beta | |
dt\alpha |
, \alpha,\beta>0
where Sα,β represents the fractal spacetime with scaling indices α and β. The traditional definition of velocity makes no sense in the non-differentiable fractal spacetime.
Based on above discussion, the concept of the fractal derivative of a function f(t) with respect to a fractal measure t has been introduced as follows:[3]
\partialf(t) | |
\partialt\alpha |
=\lim | |
t1 → t |
f(t1)-f(t) | |||||||||
|
, \alpha>0
A more general definition is given by
\partial\betaf(t) | |
\partialt\alpha |
=\lim | |
t1 → t |
| |||||||||||||
|
, \alpha>0,\beta>0
F\alpha
F\alpha
\alpha | |
D | |
F |
y(t)=\left\{ \begin{array}{ll} \underset{x → t}{F-\lim}~
y(x)-y(t) | |||||||||||||||
|
,&if~t\inF;\\ 0,&otherwise. \end{array} \right.
The derivatives of a function f can be defined in terms of the coefficients ak in the Taylor series expansion:
infin | |
f(x)=\sum | |
k=1 |
ak ⋅ (x-x
infin | |
k=1 |
{1\overk!}{dkf\over
k}(x | |
dx | |
0) ⋅ (x-x |
k=f(x | |
0)+f'(x |
0) ⋅ (x-x0)+o(x-x0)
From this approach one can directly obtain:
f'(x0)={f(x)-f(x0)-o(x-x0)\overx-x0}=\lim
x\tox0 |
{f(x)-f(x0)\overx-x0}
This can be generalized approximating f with functions (xα-(x0)α)k:
infin | |
f(x)=\sum | |
k=1 |
\alpha) | |
b | |
0 |
k=f(x | |
0)+b |
\alpha)+o(x | |
0 |
\alpha) | |
0 |
Note that the lowest order coefficient still has to be b0=f(x0), since it's still the constant approximation of the function f at x0.
Again one can directly obtain:
b1=\lim
x\tox0 |
{f(x)-f(x0)\over
\alpha} | |
x | |
0 |
\overset{\underset{def
The Fractal Maclaurin series of f(t) with fractal support F is as follows:
infty | |
f(t)=\sum | |
m=0 |
| ||||||||||
m! |
\alpha | |
(S | |
F |
(t))m
Just like in the Taylor series expansion, the coefficients bk can be expressed in terms of the fractal derivatives of order k of f:
bk={1\overk!}l({d\overdx\alpha}r)
kf(x=x | |
0) |
Proof idea: Assuming
exists, bk can be written as
One can now use
and since
If for a given function f both the derivative Df and the fractal derivative Dαf exist, one can find an analog to the chain rule:
{df\overdx\alpha}={df\overdx}{dx\overdx\alpha}={1\over\alpha}x1-\alpha{df\overdx}
The last step is motivated by the implicit function theorem which, under appropriate conditions, gives us
dx | |
dx\alpha |
=(
dx\alpha | |
dx |
)-1
Similarly for the more general definition:
{d\betaf\overd\alphax}={d(f\beta)\overd\alphax}={1\over\alpha}x1-\alpha\betaf\beta(x)f'(x)