2019
DOI: 10.3390/math7050425
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Solution of Ambartsumian Delay Differential Equation with Conformable Derivative

Abstract: This paper addresses the modelling of Ambartsumian equation using the conformable derivative as an application of the theory of surface brightness in astronomy. The homotopy perturbationmethod is applied to solve this model, where the approximate solution is given in terms of the conformable derivative order and the exponential functions. The present solution reduces to the corresponding one in the relevant literature as a special case. Moreover, a rapid rate of convergence has been achieved for the obtained a… Show more

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Cited by 19 publications
(10 citation statements)
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“…which agrees with the 3-term approximate solution in the literature [4,6] and also agrees with Ref. [7] (see Equation (30)) for ordinary derivative (α → 1).…”
Section: As α →supporting
confidence: 92%
See 1 more Smart Citation
“…which agrees with the 3-term approximate solution in the literature [4,6] and also agrees with Ref. [7] (see Equation (30)) for ordinary derivative (α → 1).…”
Section: As α →supporting
confidence: 92%
“…Patade and Bhalekar [2] obtained the solution of the ordinary model (as α → 1) as a power series. Additional results were also reported by Khaled et al [7] for the Ambartsumian equation using the conformable derivative. However, the FAE has been investigated via the homotopy transform analysis method (HTAM) in Ref.…”
Section: Introductionsupporting
confidence: 74%
“…Additional application of the PDDE arises in astronomy at specific values of α, β, and γ. For declaration, the PDDE model becomes the Ambartsumian model [9][10][11][12][13] when α = −1 and β = γ = 1/q (q > 1). The Ambartsumian model studies the surface brightness in the Milky Way.…”
Section: Introductionmentioning
confidence: 99%
“…The standard Pantograph model has been analyzed by several authors utilizing various techniques [2][3][4][5][6][7][8]. A special case of the Pantograph model is known as Ambartsumian equation which is of practical applications in Astronomy [9][10][11][12][13][14][15][16][17][18][19]. However, an interest is recently given to another special case of such model when γ = −1, given by [20] φ (t) = αφ(t) + βφ (−t) ,…”
Section: Introductionmentioning
confidence: 99%