The Chini integrability condition in second order Lovelock gravity

Abstract We analyse neutral and charged matter distributions in second order Lovelock gravity, also known as Einstein–Gauss–Bonnet gravity, in arbitrary dimensions for a static, spherically symmetric spacetime. We first transform the charged condition of pressure isotropy, an Abel differential equation of the second kind, into canonical form. We then determine a systematic approach to integrate the condition of pressure isotropy by showing that the canonical form is a Chini differential equation. The Chini invariant, which allows the master differential equation to be separable, is identified. This enables us to find three new general solutions, in implicit form, to the condition of pressure isotropy. We also show that previously obtained exact specific solutions arise as special cases in our general class of models. The Chini invariant does not arise in general relativity; it is a distinguishing feature of Einstein–Gauss–Bonnet gravity.

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Publication Details

Journal
The European Physical Journal C
Published
2024-12-29
DOI
https://doi.org/10.1140/epjc/s10052-024-13660-2
Citations
4
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
1.33
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article

The Chini integrability condition in second order Lovelock gravity

M. N. Ismail, Byron P. Brassel, Sunil D. Maharaj
4 citations
The European Physical Journal C
Cosmology and Gravitation Theories
1.33
article

The Chini integrability condition in second order Lovelock gravity

M. N. Ismail, Byron P. Brassel, Sunil D. Maharaj
article en
4 citations

Abstract

Abstract We analyse neutral and charged matter distributions in second order Lovelock gravity, also known as Einstein–Gauss–Bonnet gravity, in arbitrary dimensions for a static, spherically symmetric spacetime. We first transform the charged condition of pressure isotropy, an Abel differential equation of the second kind, into canonical form. We then determine a systematic approach to integrate the condition of pressure isotropy by showing that the canonical form is a Chini differential equation. The Chini invariant, which allows the master differential equation to be separable, is identified. This enables us to find three new general solutions, in implicit form, to the condition of pressure isotropy. We also show that previously obtained exact specific solutions arise as special cases in our general class of models. The Chini invariant does not arise in general relativity; it is a distinguishing feature of Einstein–Gauss–Bonnet gravity.

The European Physical Journal CVol. 84(12)
Durban University of Technology (ZA), University of KwaZulu-Natal (ZA)
Openalex Percentile: Top 18%
Cosmology and Gravitation Theories
1.33
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