First Integrals of Shear-Free Fluids and Complexity

被引:3
|
作者
Gumede, Sfundo C. [1 ,2 ]
Govinder, Keshlan S. [1 ]
Maharaj, Sunil D. [1 ]
机构
[1] Univ KwaZulu Natal, Astrophys Res Ctr, Sch Math Stat & Comp Sci, Private Bag X54001, ZA-4000 Durban, South Africa
[2] Mangosuthu Univ Technol, Dept Math Sci, POB 12363, ZA-4026 Jacobs, South Africa
基金
新加坡国家研究基金会;
关键词
shear-free fluids; Einstein field equations; first integrals; SYMMETRIC PERFECT FLUID; DISTRIBUTIONS; SPHERES;
D O I
10.3390/e23111539
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
A single master equation governs the behaviour of shear-free neutral perfect fluid distributions arising in gravity theories. In this paper, we study the integrability of y(xx)=f(x)y(2), find new solutions, and generate a new first integral. The first integral is subject to an integrability condition which is an integral equation which restricts the function f(x). We find that the integrability condition can be written as a third order differential equation whose solution can be expressed in terms of elementary functions and elliptic integrals. The solution of the integrability condition is generally given parametrically. A particular form of f(x)& SIM;1x(5)1-1x(-15/7) which corresponds to repeated roots of a cubic equation is given explicitly, which is a new result. Our investigation demonstrates that complexity of a self-gravitating shear-free fluid is related to the existence of a first integral, and this may be extendable to general matter distributions.
引用
收藏
页数:12
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