AN UNEVEN VACUUM ENERGY FLUID AS Λ, DARK MATTER, MOND AND LENS

DOI10.1142/S021773230802656XzbMATH Open1159.83381arXiv0802.1775OpenAlexW2131663654MaRDI QIDQ3602517

Publication date: 12 February 2009

Published in: Modern Physics Letters A (Search for Journal in Brave)

Abstract: Various TeVeS-inspired and f(R)-inspired theories of gravity have added an interesting twist to the search for dark matter and vacuum energy, modifying the landscape of astrophysics day by day. These theories can be together called a {�f N}on-{�f u}niform Dark Energy fluid (a Nu-Lambda fluid or a

m a t h b f V L a m b d a

fluid); a common thread of these theories, according of an up-to-date summary by HZL cite{Halle}, is a non-uniform vector field, describing an uneven vacuum energy fluid. The so-called "alternative" gravity theories are in fact in the standard GR gravity framework except that the cosmological "constant" is replaced by a non-trivial non-uniform vacuum energy, which couples the effects of Dark Matter and Dark Energy together by a single field. Built initially bottom-up rather than top-down as most gravity theories, TeVeS-inspired theories are healthily rooted on empirical facts. Here I attempt a review of some sanity checks of these fast-developing theories from galaxy rotation curves, gravitational lensing and cosmic acceleration. I will also discuss some theoretical aspects of the vacuum energy, and point out some analogies with electromagnetism and the Casimir effect.

Full work available at URL: https://arxiv.org/abs/0802.1775

zbMATH Keywords

gravitation dark matter gravitational lensing dark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02)