Cosmological structure formation with negative mass
arXiv:1804.03067 · doi:10.1103/PhysRevD.98.023514
Abstract
We construct a family of models with negative gravitational mass in the context of Newtonian gravity. We focus in particular on a model that reproduces the features of the so-called Dirac-Milne universe, a matter-antimatter symmetric universe that was recently proposed as an alternative cosmological scenario [A. Benoit-Levy and G. Chardin, A&A 537, A78 (2012)]. We perform one-dimensional N-body simulations of these negative-mass models for an expanding universe and study the associated formation of gravitational structures. The similarities and differences with the standard cosmological model are highlighted and discussed.
Equation 14 has been corrected (NB: typo in the published PRD version)
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- On the existence of exotic matter in classical Newtonian mechanics
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- The Dark Matter Enigma
- Antimatter Gravity Experiments, the Astronomical Challenges to Lambda-CDM Cosmology and the Quantum Vacuum as a Possible Source of Gravity in the Universe
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- Newtonian restricted three-body gravitational problem with positive and negative point masses
- Large scale structures: from inflation to today: a brief report