中文

A duality relation for fluid spacetime

广义相对论与量子宇宙学 2010-04-06 v1

摘要

We consider the electromagnetic resolution of gravitational field. We show that under the duality transformation, in which active and passive electric parts of the Riemann curvature are interchanged, a fluid spacetime in comoving coordinates remains invariant in its character with density and pressure transforming, while energy flux and anisotropic pressure remaining unaltered. Further if fluid admits a barotropic equation of state, p=(γ1)ρp = (\gamma - 1) \rho where 1γ21 \leq \gamma \leq 2, which will transform to p=(2γ3γ21)ρp = (\frac{2 \gamma}{3 \gamma - 2} - 1) \rho. Clearly the stiff fluid and dust are dual to each-other while ρ+3p=0\rho + 3 p =0, will go to flat spacetime. However the n (ρ3p=0)(\rho - 3 p = 0) and the deSitter (ρ+p=0(\rho + p = 0) universes ar e self-dual.

关键词

引用

@article{arxiv.gr-qc/9801076,
  title  = {A duality relation for fluid spacetime},
  author = {Naresh Dadhich and L. K. Patel and Ramesh Tikekar},
  journal= {arXiv preprint arXiv:gr-qc/9801076},
  year   = {2010}
}

备注

5 pages, LaTeX version, Accepted in Classical Quantum Gravity as a Letter