Answers are grounded in this paper and cite their sources.
In [1] V. Guillemin and D. Kazhdan introduced the following definition of spectral rigidity of a Riemannian manifold. Let (M, g) be a compact boundaryless Riemannian manifold. A family g of Riemannian metrics on M smoothly depending on the parameter τ ∈ [−2, 2] is called the deformation of the metric g if g = g. A deformation is called trivial if there exists a one-parameter family of diffeomorphisms φ : M → M such that φ = Id, and g = (φ )∗g0. Given a deformation g (−2 ≤ τ ≤ 2), let ∆ : C∞(M) → C∞(M) be the Laplace-Beltrami operator corresponding to the metric g . The deformation is called isospectral if, for all −2 ≤ τ ≤ 2 spectra of the operators ∆ and ∆ coincide (counting multiplicities). A Riemannian manifold (M, g) is called spectrally rigid if it does not admit non-trivial isospectral deformations. The main result of the present article is the following
No takes yet. Share an insight, caveat, or question.
Croke et al. (1998) studied this question.
Synapse has enriched 3 related papers. Consider them for comparative context: