In this paper, we analyze the bending of light by galaxies or clusters of galaxies in the presence of the Λ term. Using Friedmann-Robertson-Walker (FRW) coordinates, which are used for the description of actual observations, we demonstrate that the cosmological constant does not practically influence the lensing effect.
| Original language | English |
|---|---|
| Pages (from-to) | 2255-2259 |
| Number of pages | 5 |
| Journal | International Journal of Modern Physics D |
| Volume | 17 |
| Issue number | 12 |
| DOIs | |
| State | Published - 1 Nov 2008 |
ID: 36641506