Abstract
We examine some cosmological consequences of gravity coupling with different strength to fermions and bosons. We show that this leads to a different perturbation of the standard picture of primordial nucleosynthesis than the addition of extra neutrino types or overall scaling of the value of . Observed abundances of deuterium and place bounds on the ratio of the bosonic gravitational constant () to the fermionic gravitational constant () of at and at . A value of can reconcile the current “tension” between the abundances of deuterium and predicted by primordial nucleosynthesis. We comment briefly on other cosmological effects.
- Received 3 June 2004
DOI:https://doi.org/10.1103/PhysRevD.70.103515
©2004 American Physical Society