Abstract
The issue of whether the present observational evidence that the mean mass density of the universe is less than the critical density (i.e., μ<1) implies an infinite future expansion of the universe is discussed. Although in conventional cosmological scenarios μ<1 necessarily leads to a universe that will grow infinitely old, this conclusion can be avoided in ways which are reasonably natural. One of these is to assume the existence of a small negative cosmological constant. Another way is to postulate the existence of unstable fields with a long time scale for the onset of the instability. An example is a scalar field with a negative squared mass and ¦m¦≲10−32eV. Other examples include fields for which the instability is generated by quantum corrections in curved space-time. All of these are capable of halting the expansion of an open universe and forcing it to recollapse into a “big crunch.”
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This essay received the fourth award from the Gravity Research Foundation for the year 1986—Ed.
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Ford, L.H. Does μ<1 imply that the universe will expand forever?. Gen Relat Gravit 19, 325–329 (1987). https://doi.org/10.1007/BF00767271
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DOI: https://doi.org/10.1007/BF00767271