The N--P and 1+1+2 correspondence

Fuente: arXiv
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Auteurs principaux: Sherif, Abbas M, Dunsby, Peter K S
Format: Preprint
Publié: 2026
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author Sherif, Abbas M
Dunsby, Peter K S
author_facet Sherif, Abbas M
Dunsby, Peter K S
contents In this letter, we establish a complete correspondence between the Newman--Penrose and 1+1+2 semitetrad covariant formalisms by expressing all Newman--Penrose spin coefficients, Ricci scalars, and Weyl scalars in terms of the scalar, vector, and tensor variables of the 1+1+2 decomposition. This provides a direct dictionary between two widely used approaches to general relativity and gives a geometrical interpretation of Newman--Penrose quantities in terms of covariantly defined 1+1+2 variables. As an application, we derive necessary conditions for the existence of future outer trapping horizons in locally rotationally symmetric class II spacetimes, expressed in terms of the Ricci and Weyl Newman--Penrose scalars and the cosmological constant.
format Preprint
id arxiv_https___arxiv_org_abs_2605_30255
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle The N--P and 1+1+2 correspondence
Sherif, Abbas M
Dunsby, Peter K S
General Relativity and Quantum Cosmology
In this letter, we establish a complete correspondence between the Newman--Penrose and 1+1+2 semitetrad covariant formalisms by expressing all Newman--Penrose spin coefficients, Ricci scalars, and Weyl scalars in terms of the scalar, vector, and tensor variables of the 1+1+2 decomposition. This provides a direct dictionary between two widely used approaches to general relativity and gives a geometrical interpretation of Newman--Penrose quantities in terms of covariantly defined 1+1+2 variables. As an application, we derive necessary conditions for the existence of future outer trapping horizons in locally rotationally symmetric class II spacetimes, expressed in terms of the Ricci and Weyl Newman--Penrose scalars and the cosmological constant.
title The N--P and 1+1+2 correspondence
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2605.30255