2012
DOI: 10.1007/s10114-012-0507-3
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An approach to differential geometry of fractional order via modified Riemann-Liouville derivative

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Cited by 50 publications
(50 citation statements)
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“…In addition, Kolwankar obtained the same formula (4) by using an approach on Cantor space [30]. In addition, Jumarie in [31] gave detailed proofs of the above formulas (see Proposition 3.1 page 1746 and Section 4 (Some Basic Formulae for Fractional Derivative and Integral) page 1748). The above properties play an important role in the fractional mapping method.…”
Section: Mathematical Problems In Engineeringmentioning
confidence: 99%
“…In addition, Kolwankar obtained the same formula (4) by using an approach on Cantor space [30]. In addition, Jumarie in [31] gave detailed proofs of the above formulas (see Proposition 3.1 page 1746 and Section 4 (Some Basic Formulae for Fractional Derivative and Integral) page 1748). The above properties play an important role in the fractional mapping method.…”
Section: Mathematical Problems In Engineeringmentioning
confidence: 99%
“…We have proposed recently a fractional calculus based on fractional difference [9][10][11][12][13][14][15][16] which is slightly different from the classical Riemann-Liouville framework [1][2][3][4][5][6][20][21][22][23][24][25][26][27][28], and results in a useful fractional Taylor series [12] providing (2) as the first term. The fractional calculus so obtained is quite parallel to the classical calculus, and it involves non-commutative derivatives, what seems to be quite consistent with non commutative geometry.…”
Section: Purpose and Organization Of The Articlementioning
confidence: 99%
“…In the sequence we propose an alternative approach by considering fractional space-time instead of fractional space functions, that is, we consider that a coarse-grained space-time, which means that space and time are non-differentiable and considering the chain rule as [2] …”
Section: Introductionmentioning
confidence: 99%
“…It can be shown that the ansatz φ = φ(x α + λt β ) is a solution of the FWE in a coarse-grained space-time [2], subject to the condition λ α,β = ±v β Γ(α+1) Γ(β+1) . The result above gives the insight to redefine the light-cone variables ξ, η as ξ = x α − λt β and η = x α + λt β .…”
Section: Introductionmentioning
confidence: 99%