Peculiar motions, accelerated expansion, and the cosmological axis
Abstract
Peculiar velocities change the expansion rate of any observer moving relative to the smooth Hubble flow. As a result, observers in a galaxy like our Milky Way can experience accelerated expansion within a globally decelerating universe, even when the drift velocities are small. The effect is local, but the affected scales can be large enough to give the false impression that the whole cosmos has recently entered an accelerating phase. Generally, peculiar velocities are also associated with dipolelike anisotropies, triggered by the fact that they introduce a preferred spatial direction. This implies that observers experiencing locally accelerated expansion, as a result of their own drift motion, may also find that the acceleration is maximized in one direction and minimized in the opposite. We argue that, typically, such a dipole anisotropy should be relatively small and the axis should probably lie fairly close to the one seen in the spectrum of the cosmic microwave background.
- Publication:
-
Physical Review D
- Pub Date:
- September 2011
- DOI:
- 10.1103/PhysRevD.84.063503
- arXiv:
- arXiv:1107.4045
- Bibcode:
- 2011PhRvD..84f3503T
- Keywords:
-
- 98.80.-k;
- 95.36.+x;
- 98.80.Jk;
- Cosmology;
- Dark energy;
- Mathematical and relativistic aspects of cosmology;
- Astrophysics - Cosmology and Extragalactic Astrophysics;
- General Relativity and Quantum Cosmology
- E-Print:
- Typos corrected. Published version