Why Do All the Curvature Invariants of a Gravitational Wave Vanish ?

نویسنده

  • Hans-J Urgen Schmidt
چکیده

We prove the theorem valid for (Pseudo)-Riemannian manifolds V n : "Let x 2 V n be a xed point of a homothetic motion which is not an isometry then all curvature invariants vanish at x." and get the Corollary: "All curvature invariants of the plane wave metric ds 2 = 2 du dv + a 2 (u) dw 2 + b 2 (u) dz 2 identically vanish." Analysing the proof we see: The fact that for deenite signature atness can be characterized by the vanishing of a curvature invariant, essentially rests on the compactness of the rotation group S O(n). For Lorentz signature, however, one has the non-compact Lorentz group S O(3; 1) instead of it. A further and independent proof of the corollary uses the fact, that the Geroch limit does not lead to a Hausdorr topology, so a sequence of gravitational waves can converge to the at space-time, even if each element of the sequence is the same pp-wave.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

X iv : g r - qc / 9 40 40 37 v 1 1 9 A pr 1 99 4 Why do all the curvature invariants of a gravitational wave vanish ?

We prove the theorem valid for (Pseudo)-Riemannian manifolds Vn: ”Let x ∈ Vn be a fixed point of a homothetic motion which is not an isometry then all curvature invariants vanish at x.” and get the Corollary: ”All curvature invariants of the plane wave metric ds = 2 du dv + a(u) dw + b(u) dz identically vanish.” Analysing the proof we see: The fact that for definite signature flatness can be ch...

متن کامل

ar X iv : g r - qc / 9 51 20 07 v 1 2 9 N ov 1 99 5 Consequences of the noncompactness of the Lorentz

The following four statements have been proven decades ago already, but they continue to induce a strange feeling: All curvature invariants of a gravitational wave vanish inspite of the fact that it represents a nonflat spacetime. The eigennullframe components of the curvature tensor (the Cartan ”scalars”) do not represent curvature scalars. The Euclidean topology in the Minkowski spacetime doe...

متن کامل

The Weyl tensor in Spatially Homogeneous Cosmological Models

We study the evolution of the Weyl curvature invariant in all spatially homogeneous universe models containing a non-tilted γ-law perfect fluid. We investigate all the Bianchi and Thurston type universe models and calculate the asymptotic evolution of Weyl curvature invariant for generic solutions to the Einstein field equations. The influence of compact topology on Bianchi types with hyperboli...

متن کامل

Geodesic motion in the Kundt spacetimes and the character of envelope singularity

We investigate geodesics in specific Kundt type N (or conformally flat) solutions to Einstein’s equations. Components of the curvature tensor in parallelly transported tetrads are then explicitly evaluated and analyzed. This elucidates some interesting global properties of the spacetimes, such as an inherent rotation of the wave-propagation direction, or the character of singularities. In parti...

متن کامل

The phase coherence of extragalactic light II : why the curvature of space must be precisely zero Richard

Since the advent of General Relativity, it has been part of accepted knowledge that the space curvature parameter K of an expanding Universe is determined by the strength of its incipient gravitational field, the latter measured by the ratio Ω = ρ/ρ c where ρ is the average mass density of the Universe and ρ c is a critical density. In this Letter we calculated the phase behavior of light as it...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1994