Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas

2); (2)Rudjer Boskovic Institute; Gary B. Tupper (1); Neven Bilic (1; Raoul D. Viollier (1) ((1)University of Cape Town; SA; Zagreb)

arxiv: astro-ph/0111325 · v2 · submitted 2001-11-16 · 🌌 astro-ph · gr-qc· hep-ph

Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas

Neven Bilic (1 , 2) , Gary B. Tupper (1) , Raoul D. Viollier (1) ((1)University of Cape Town , SA , (2)Rudjer Boskovic Institute , Zagreb) This is my paper

classification 🌌 astro-ph gr-qchep-ph

keywords darkenergymattermodelapproximationchaplyginextendformulating

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We extend the world model of Kamenshchik et al. to large perturbations by formulating a Zeldovich-like approximation. We sketch how this model unifies dark matter with dark energy in a geometric setting reminiscent of M-theory.

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