English

Algebraic Rainich conditions for the tensor V

General Relativity and Quantum Cosmology 2015-05-18 v1

Abstract

Algebraic conditions on the Ricci tensor in the Rainich-Misner-Wheeler unified field theory are known as the Rainich conditions. Penrose and more recently Bergqvist and Lankinen made an analogy from the Ricci tensor to the Bel-Robinson tensor BαβμνB_{\alpha\beta\mu\nu}, a certain fourth rank tensor quadratic in the Weyl curvature, which also satisfies algebraic Rainich-like conditions. However, we found that not only does the tensor BαβμνB_{\alpha\beta\mu\nu} fulfill these conditions, but so also does our recently proposed tensor VαβμνV_{\alpha\beta\mu\nu}, which has many of the desirable properties of BαβμνB_{\alpha\beta\mu\nu}. For the quasilocal small sphere limit restriction, we found that there are only two fourth rank tensors BαβμνB_{\alpha\beta\mu\nu} and VαβμνV_{\alpha\beta\mu\nu} which form a basis for good energy expressions. Both of them have the completely trace free and causal properties, these two form necessary and sufficient conditions. Surprisingly either completely traceless or causal is enough to fulfill the algebraic Rainich conditions. Furthermore, relaxing the quasilocal restriction and considering the general fourth rank tensor, we found two remarkable results: (i) without any symmetry requirement, the algebraic Rainich conditions only require totally trace free; (ii) with a symmetry requirement, we recovered the same result as in the quasilocal small sphere limit.

Keywords

Cite

@article{arxiv.1005.0674,
  title  = {Algebraic Rainich conditions for the tensor V},
  author = {Lau Loi So},
  journal= {arXiv preprint arXiv:1005.0674},
  year   = {2015}
}

Comments

17 pages

R2 v1 2026-06-21T15:18:40.778Z