
ABSTRACTThe agreement between the observed light element abundances and calculations of homogeneous cosmological nucleosynthesis constrains inhomogenequs models, and suggests that most of the matter in the Universe is invisible Dark Matter. This could be in the form of neutrinos, lightest supersymmetric particles (LSPs) or axions. Interactions between LSPs or axions and nuclear matter are controlled by the spin decomposition of the nucleon.
Astrophysics (astro-ph), FOS: Physical sciences, Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory, Astrophysics, dark matter, Astrophysical cosmology, Observational and experimental questions in relativity and gravitational theory, particle physics, inflation, cosmology, Relativistic cosmology, cosmic microwave background radiation
Astrophysics (astro-ph), FOS: Physical sciences, Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory, Astrophysics, dark matter, Astrophysical cosmology, Observational and experimental questions in relativity and gravitational theory, particle physics, inflation, cosmology, Relativistic cosmology, cosmic microwave background radiation
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
