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arxiv: astro-ph/9601147 · v1 · pith:4HKZGZQHnew · submitted 1996-01-25 · 🌌 astro-ph · gr-qc· hep-ph· hep-th

A Low-Density Closed Universe

classification 🌌 astro-ph gr-qchep-phhep-th
keywords universecloseddensitymatterarisebackgroundcasecausally-connected
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Matter with an equation of state $p=-\rho/3$ may arise in certain scalar field theories, and the energy density of this matter decreases as $a^{-2}$ with the scale factor $a$ of the Universe. In this case, the Universe could be closed but still have a nonrelativistic-matter density $\Omega_0<1$. Furthermore, the cosmic microwave background could come from a causally-connected region at the other side of the Universe. This model is currently viable and might be tested by a host of forthcoming observations.

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