2016
DOI: 10.3390/sym8040024
|View full text |Cite
|
Sign up to set email alerts
|

Reply to Frewer et al. Comments on Janocha et al. Lie Symmetry Analysis of the Hopf Functional-Differential Equation. Symmetry 2015, 7, 1536–1566

Abstract: We reply to the comment by Frewer and Khujadze regarding our contribution “Lie Symmetry Analysis of the Hopf Functional-Differential Equation” (Symmetry 2015, 7(3), 1536). The method developed by the present authors considered the Lie group analysis of the Hopf equations with functional derivatives in the equation, not the integro-differential equations in general. It was based on previous contributions (Oberlack and Wacławczyk, Arch. Mech. 2006, 58; Wacławczyk and Oberlack, J. Math. Phys. 2013, 54). In fact, … Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2022
2022
2022
2022

Publication Types

Select...
1

Relationship

0
1

Authors

Journals

citations
Cited by 1 publication
(1 citation statement)
references
References 8 publications
(42 reference statements)
0
1
0
Order By: Relevance
“…It is well known that the n dimensional manifold can always be embedded in Pseudo-Euclidean space of dimensions, and the minimum extra dimensions of pseudo-Euclidean space needed for the embedding is called the embedding Class of . According to this definition, Schwarzschild 's interior and exterior solutions are of Class I and Class II, respectively; the class of general spherical and plane symmetric spacetimes are II and III, respectively; and the well known Kerr metric is of Class V [62][63][64][65].…”
Section: Introductionmentioning
confidence: 99%
“…It is well known that the n dimensional manifold can always be embedded in Pseudo-Euclidean space of dimensions, and the minimum extra dimensions of pseudo-Euclidean space needed for the embedding is called the embedding Class of . According to this definition, Schwarzschild 's interior and exterior solutions are of Class I and Class II, respectively; the class of general spherical and plane symmetric spacetimes are II and III, respectively; and the well known Kerr metric is of Class V [62][63][64][65].…”
Section: Introductionmentioning
confidence: 99%