The measure problem in cosmology concerns how to compute fractions of universes of different types within a multiverse. It typically arises in the context of eternal inflation but can apply even with non-eternal inflation and a finite universe. The problem arises because different approaches to calculating these fractions yield different results, and it's not clear which approach (if any) is correct.
Contents
Measures can be evaluated by whether they predict observed physical constants, as well as whether they avoid counterintuitive implications, such as the youngness paradox or Boltzmann brains. While dozens of measures have been proposed, few physicists consider the problem to be solved.
The problem
Infinite multiverse theories are becoming increasingly popular, but because they involve infinitely many instances of different types of universes, it's unclear how to compute the fractions of each type of universe. Alan Guth put it this way:
In a single universe, cows born with two heads are rarer than cows born with one head. [But in an infinitely branching multiverse] there are an infinite number of one-headed cows and an infinite number of two-headed cows. What happens to the ratio?Sean M. Carroll offered another informal example:
Say there are an infinite number of universes in which George W. Bush became President in 2000, and also an infinite number in which Al Gore became President in 2000. To calculate the fraction N(Bush)/N(Gore), we need to have a measure — a way of taming those infinities. Usually this is done by “regularization.” We start with a small piece of universe where all the numbers are finite, calculate the fraction, and then let our piece get bigger, and calculate the limit that our fraction approaches.However, different procedures for computing the limit of this fraction may yield different answers.
This is important because in order to compare cosmological theories in an infinite multiverse, we need to know which types of universes theories predict to be more common than others.
Proper-time cutoff
The proper-time cutoff measure considers the probability
This measure has the advantage of being stationary in the sense that probabilities remain the same over time in the limit of large
Scale-factor cutoff
Time can be parameterized in different ways than proper time. One choice is to parameterize by the scale factor of space
This approach can be generalized to a family of measures in which a small region grows as
The scale-factor cutoff measure takes
This measure is very sensitive to the choice of
De Simone et al. (2010) consider the scale-factor cutoff measure to be a very promising solution to the measure problem. This measure has also been shown to produce good agreement with observational values of the cosmological constant.
Stationary
The stationary measure proceeds from the observation that different processes achieve stationarity of
Andrei Linde and coauthors have suggested that the stationary measure avoids both the youngness paradox and Boltzmann brains. However, the stationary measure predicts extreme (either very large or very small) values of the primordial density contrast
Causal diamond
Reheating marks the end of inflation. The causal diamond is the finite four-volume formed by intersecting the future light cone of an observer crossing the reheating hypersurface with the past light cone of the point where the observer has exited a given vacuum. Put another way, the causal diamond is
the largest swath accessible to a single observer traveling from the beginning of time to the end of time. The finite boundaries of a causal diamond are formed by the intersection of two cones of light, like the dispersing rays from a pair of flashlights pointed toward each other in the dark. One cone points outward from the moment matter was created after a Big Bang — the earliest conceivable birth of an observer — and the other aims backward from the farthest reach of our future horizon, the moment when the causal diamond becomes an empty, timeless void and the observer can no longer access information linking cause to effect.The causal diamond measure multiplies the following quantities:
Different prior probabilities of vacuum types yield different results. Entropy production can be approximated as the number of galaxies in the diamond.
An attraction of this approach is that it avoids comparing infinities, which is the original source of the measure problem.
Watcher
The watcher measure imagines the world line of an eternal "watcher" that passes through an infinite number of big crunch singularities.