2020
DOI: 10.1007/s00229-020-01236-9
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On a class of geodesic orbit spaces with abelian isotropy subgroup

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Cited by 9 publications
(10 citation statements)
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“…For the necessity part, assume initially that n 1 = • • • = n s = 2 so that H is abelian. Since G is semisimple, the main results in [24] imply that any g.o. metric on G/H is normal, and hence Theorem 1.1 follows in this case.…”
Section: So(nmentioning
confidence: 99%
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“…For the necessity part, assume initially that n 1 = • • • = n s = 2 so that H is abelian. Since G is semisimple, the main results in [24] imply that any g.o. metric on G/H is normal, and hence Theorem 1.1 follows in this case.…”
Section: So(nmentioning
confidence: 99%
“…The classification of g.o. spaces remains an open problem, whereas several partial classifications have been obtained ( [2], [3], [12], [13], [14], [16], [24], [27] to name a few).…”
Section: Introductionmentioning
confidence: 99%
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“…When G is compact semisimple, the classification of the g.o. spaces (G/H, g) with H abelian and H simple has been obtained in the works [20] and [11] respectively. On the other hand, the classification of compact g.o.…”
Section: Introductionmentioning
confidence: 99%
“…Then Equation(19) along with Lemma 4.2 yield0 = λ[a, e 12 ] + λ[a, X 12 ] + 2(λ − µ)f 21 . (20)By the ad(h)-invariance of m ij and the fact that a ∈ h, the first two terms of Equation(20) lie in m 01 and m 12 respectively, while the last term lies in m 01 . Therefore, Equation (20) yields the systemλ[a, e 12 ] + 2(λ − µ)f 21 = 0 (21) λ[a, X 12 ] = 0.…”
mentioning
confidence: 99%