ar X iv : g r - qc / 0 20 20 81 v 1 2 1 Fe b 20 02 The non - existence of a Lanczos potential for the Weyl curvature tensor in dimensions n ≥ 7

نویسندگان

  • S. Brian Edgar
  • A. Höglund
چکیده

In this paper it is shown that a Lanczos potential for the Weyl curvature tensor does not exist for all spaces of dimension n ≥ 7. Whether there exists a Lanczos potential [1] for Weyl curvature tensors in dimensions n > 4 has still not been determined. Although Lanczos's original proof [1] for existence was flawed [2], there have subsequently been complete proofs for existence in four dimensions [2, 3, 4]. The latter two proofs [3, 4] are in spinors, although in [4] a translation into tensors is given which is explicitly for four dimensions, independent of signature. The detailed and complicated proof given by Bampi and Caviglia [2] is also explicitly for four dimensions, although they also discuss briefly the possibility of existence in higher dimensions. An important aspect of all of these proofs is that they are not only valid for Weyl curvature tensors C abcd , but for Weyl candidate tensors W abcd , i.e., any 4-tensor having the index symmetries of the Weyl curvature tensor, W abcd = W [ab]cd = W ab[cd] = W cdab W a bad = 0. (1a) 0 = W a[bcd] (1b) In a recent paper [5] we have shown that a Lanczos potential for a Weyl candidate tensor does not generally exist for dimensions n > 4. In particular, we have shown that in flat and conformally flat spaces with dimensions n > 4, the assumed existence of a Lanczos potential for an arbitrary Weyl candidate imposes non-trivial conditions on the Weyl candidate. However, this result does not say anything about the existence of a Lanczos potential for a Weyl curvature tensor in spaces with non-zero conformal curvature in dimensions n > 4. In this paper we will address the problem of Weyl curvature tensors directly, and show explicitly, that A Lanczos potential for the Weyl curvature tensor does not exist for all spaces of dimension n ≥ 7.

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

ar X iv : g r - qc / 9 90 20 80 v 2 1 3 Ja n 20 00 LOCAL EXISTENCE OF SPINOR - AND TENSOR POTENTIALS

We give new simple direct proofs in all spacetimes for the existence of asymmetric (n, m + 1)-spinor potentials for completely symmetric (n + 1, m)-spinors and for the existence of symmetric (n, 1)-spinor potentials for symmetric (n + 1, 0)-spinors. These proofs introduce a 'superpotential', i.e., a potential of the potential, which also enables us to get explicit statements of the gauge freedo...

متن کامل

ar X iv : g r - qc / 9 90 20 80 v 1 2 5 Fe b 19 99 LOCAL EXISTENCE OF SPINOR POTENTIALS

We present a new, simple proof of existence for the Lanczos spinor potential in 3+1 dimensions that introduces a potential T ABCD = T (ABC)D of the Lanczos potential together with several generalizations to other index configurations and metric signatures. The potential T ABCD can also be used to express, in a concise way, the gauge freedom left in the Lanczos potential after the differential g...

متن کامل

ar X iv : g r - qc / 0 21 20 56 v 2 2 3 Ja n 20 03 The Weyl - Lanczos Equations and the Lanczos Wave Equation in 4 Dimensions as Systems in Involution

Using the work by Bampi and Caviglia, we write the Weyl-Lanczos equations as an exterior differential system. Using Janet-Riquier theory, we compute the Cartan characters for all spacetimes with a diagonal metric and for the plane wave spacetime since all spacetimes have a plane wave limit. We write the Lanczos wave equation as an exterior differential system and, with assistance from Janet-Riq...

متن کامل

ar X iv : g r - qc / 0 20 21 02 v 1 2 8 Fe b 20 02 The family of regular interiors for non - rotating black holes

We find the general solution for the spacetimes describing the interior of static black holes with an equation of state of the type T 0 0 = T 1 1 (T being the stress-energy tensor). This form is the one expected from taking into account different quantum effects associated with strong gravitational fields. We recover all the particular examples found in the literature. We remark that all the so...

متن کامل

ar X iv : g r - qc / 9 90 10 01 v 2 2 5 Fe b 20 02 Multidimensional cosmological and spherically symmetric solutions with intersecting p - branes

Multidimensional model describing the " cosmological " and/ or spherically symmetric configuration with (n + 1) Einstein spaces in the theory with several scalar fields and forms is considered. When electromagnetic composite p-brane ansatz is adopted, n " internal " spaces are Ricci-flat, one space M 0 has a non-zero curvature, and all p-branes do not " live " in M 0 , a class of exact solution...

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 2002