Astrophysical structures from primordial quantum black holes
arXiv:1005.2891 · doi:10.1140/epjc/s10052-010-1387-2
Abstract
The characteristic sizes of astrophysical structures, up to the whole observed Universe, can be recovered, in principle, assuming that gravity is the overall interaction assembling systems starting from microscopic scales, whose order of magnitude is ruled by the Planck length and the related Compton wavelength. This result agrees with the absence of screening mechanisms for the gravitational interaction and could be connected to the presence of Yukawa corrections in the Newtonian potential which introduce typical interaction lengths. This result directly comes out from quantization of primordial black holes and then characteristic interaction lengths directly emerge from quantum field theory.
11 pages
References in corpus (5)
- Extended Theories of Gravity and their Cosmological and Astrophysical Applications
- Low surface brightness galaxies rotation curves in the low energy limit of gravity : no need for dark matter?
- The Newtonian Limit of F(R) gravity
- Accelerating cosmologies from non-local higher-derivative gravity
- Fractal large-scale structure from a stochastic scaling law model