Results 1 to 10 of about 9,675 (272)

On some systems of collineation groups [PDF]

open access: gold, 1913
SOME systems of collineation groups which arise in connection with the theory of elliptic functions have been investigated by Klein | and HurwitzJ. One of them is a system in n variables each group of which contains an invariant subgroup of order n.
Howard H. Mitchell
openalex   +2 more sources

Ricci Collineations for Non-Degenerate, Diagonal and Spherically Symmetric Ricci Tensors [PDF]

open access: yesGen.Rel.Grav. 32 (2000) 285-294, 1999
The expression of the vector field generator of a Ricci Collineation for diagonal, spherically symmetric and non-degenerate Ricci tensors is obtained. The resulting expressions show that the time and radial first derivatives of the components of the Ricci tensor can be used to classify the collineation, leading to 64 families.
A. H. Bokhari   +11 more
arxiv   +4 more sources

Collineation group as a subgroup of the symmetric group [PDF]

open access: yesOpen Mathematics, 2013
Let ψ be the projectivization (i.e., the set of one-dimensional vector subspaces) of a vector space of dimension ≥ 3 over a field. Let H be a closed (in the pointwise convergence topology) subgroup of the permutation group $\mathfrak{S}_\psi $ of the set
Bogomolov Fedor, Rovinsky Marat
doaj   +2 more sources

symmetries of the Ricci tensor of static space times with maximal symmetric transverse spaces [PDF]

open access: yes, 2006
Static space times with maximal symmetric transverse spaces are classified according to their Ricci collineations. These are investigated for non-degenerate Ricci tensor ($det.(R_{\alpha}) \neq 0$). It turns out that the only collineations admitted by these spaces can be ten, seven, six or four. Some new metrics admitting proper Ricci collineations are
A.Z. Petro   +4 more
arxiv   +4 more sources

Ricci Collineations in Friedmann-Robertson-Walker Spacetimes [PDF]

open access: greenClass.Quant.Grav. 19 (2002) 393-404, 2001
Ricci collineations and Ricci inheritance collineations of Friedmann-Robertson-Walker spacetimes are considered. When the Ricci tensor is non-degenerate, it is shown that the spacetime always admits a fifteen parameter group of Ricci inheritance collineations; this is the maximal possible dimension for spacetime manifolds.
Uğur Camcı, Alan Barnes
arxiv   +3 more sources

Matter collineations of Spacetime Homogeneous Gödel-type Metrics [PDF]

open access: greenClass.Quant.Grav. 20 (2003) 2169, 2003
The spacetime homogeneous G\"odel-type spacetimes which have four classes of metrics are studied according to their matter collineations. The obtained results are compared with Killing vectors and Ricci collineations. It is found that these spacetimes have infinite number of matter collineations in degenerate case, i.e.
Uğur Camcı, M. Sharif
arxiv   +3 more sources

Proper Weyl Collineations in Kantowski-Sachs and Bianchi Type III Space-Times [PDF]

open access: green, 2006
A study of proper Weyl collineations in Kantowski-Sachs and Bianchi type III space-times is given by using the rank of the 6X6 Weyl matrix and direct integration techniques. Studying proper Weyl collineations in each of the above space-times, it is shown that there exists no such possibility when the above space-times admit proper Weyl collineations.
Ghulam Shabbir, ABU BAKAR MEHMOOD
arxiv   +3 more sources

Matter Collineations of Static Spacetimes with Maximal Symmetric Transverse Spaces [PDF]

open access: greenActaPhys.Polon.B38:2003-2030,2007, 2007
This paper is devoted to study the symmetries of the energy-momentum tensor for the static spacetimes with maximal symmetric transverse spaces. We solve matter collineation equations for the four main cases by taking one, two, three and four non-zero components of the vector $\xi^a$.
M. Sharif
arxiv   +3 more sources

Proof of the prime power conjecture for projective planes of order 𝑛 with abelian collineation groups of order 𝑛²

open access: bronze, 2001
Let G be an abelian collineation group of order n 2 of a projective plane of order n. We show that n must be a prime power, and that the p-rank of G is at least b + 1 if n = p b for an odd prime p.
Aart Blokhuis   +2 more
openalex   +2 more sources

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