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 ?

نویسنده

  • Jürgen Schmidt
چکیده

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 characterized by the vanishing of a curvature invariant, essentially rests on the compactness of the rotation group SO(n). For Lorentz signature, however, one has the non-compact Lorentz group SO(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 Hausdorff topology, so a sequence of gravitational waves can converge to the flat space-time, even if each element of the sequence is the same pp-wave. AMS number: 53 B 30 Lorentz metrics, indefinite metrics PACS number: 0430 Gravitational waves: theory

برای دانلود رایگان 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

ar X iv : g r - qc / 9 80 40 05 v 2 1 4 A pr 1 99 8 Curvature invariants in type N spacetimes

Scalar curvature invariants are studied in type N solutions of vacuum Einstein's equations with in general non-vanishing cosmological constant Λ. Zero-order invariants which include only the metric and Weyl (Riemann) tensor either vanish, or are constants depending on Λ. Even all higher-order invariants containing covariant derivatives of the Weyl (Riemann) tensor are shown to be trivial if a t...

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

ar X iv : g r - qc / 9 90 40 15 v 1 6 A pr 1 99 9 Errors on the inverse problem solution for a noisy spherical gravitational wave antenna

A single spherical antenna is capable of measuring the direction and polarization of a gravitational wave. It is possible to solve the inverse problem using only linear algebra even in the presence of noise. The simplicity of this solution enables one to explore the error on the solution using standard techniques. In this paper we derive the error on the direction and polarization measurements ...

متن کامل

ar X iv : g r - qc / 9 80 40 05 v 1 2 A pr 1 99 8 Curvature invariants in type N spacetime

Scalar curvature invariants are studied in type N solutions of vacuum Einstein's equations with in general non-vanishing cosmological constant Λ. Zero-order invariants which include only the metric and Weyl (Riemann) tensor either vanish, or are constants depending on Λ. Even all higher-order invariants containing covariant derivatives of the Weyl (Riemann) tensor are shown to be trivial if a t...

متن کامل

ar X iv : g r - qc / 9 90 40 27 v 1 1 2 A pr 1 99 9 Vacuum structure for expanding geometry

We consider gravitational wave modes in the FRW metrics in a de Sitter phase and show that the state space splits into many unitarily inequivalent representations of the canonical commutation relations. Non-unitary time evolution is described as a trajectory in the space of the representations. The generator of time evolution is related to the entropy operator. The thermo-dynamic arrow of time ...

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

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1994