Anthropic Landscape

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	CATEGORIES ABOUT STRING THEORY LANDSCAPE
	physical cosmology
	string theory
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The idea of the string theory landscape has been used to propose a concrete implementation of the Anthropic Principle , the idea that fundamental constants may have the values they have not for fundamental physical reasons, but rather because such values are necessary for life (and hence intelligent observers to measure the constants). In 1987, Steven Weinberg proposed that the observed value of the Cosmological Constant was so small because it is not possible for life to occur in a universe with a much larger cosmological constant. In order to implement this idea in a concrete physical theory, it is necessary to postulate that a Multiverse in which fundamental physical parameters can take different values. This has been realized in the context of Eternal Inflation . Some physicists, starting with Weinberg, have proposed that Bayesian Probability can be used to compute probability distributions for fundamental physical parameters, where the probability $P(x)$ of observing some fundamental parameters $x$ is given by, :$P(x)=P\_\backslash mathrm\{prior\}(x)\; imes\; P\_\backslash mathrm\{selection\}(x),$ where $P\_\backslash mathrm\{prior\}$ is the prior probability, from fundamental theory, of the parameters $x$ and $P\_\backslash mathrm\{selection\}$ is the anthropic selection function, determined by the number of "observers" that would occur in the universe with parameters $x$. These probabilistic arguments are the most controversial aspect of the landscape. Technical criticisms of these proposals have pointed out that: The function $P\_\backslash mathrm\{prior\}$ is completely unknown in string theory and may be impossible to define or interpret in any sensible probablistic way. The function $P\_\backslash mathrm\{selection\}$ is completely unknown, since so little is known about the origin of life and criteria (such as the number of galaxies) must be used as a proxy for the number of observers. Moreover, it may never be possible to compute it for parameters radically different from those of the observable universe. Interpreting probability in a context where it is only possible to draw one Sample from a Distribution is problematic. Various physicists have tried to address these objections, but as yet there is no widespread agreement. These ideas have been reviewed by Carroll . Tegmark ''et al.'' have recently considered these objections and proposed a simplified anthropic scenario for Axion Dark Matter in which they argue that the first two of these problems do not apply. Although few dispute the idea that string theory appears to have an unimaginably large number of metastable vacua, the existence, meaning and scientific relevance of the anthropic landscape remain highly controversial. Prominent proponents of the idea include Michael Douglas , Andrei Linde , Joseph Polchinski , Sir Martin Rees and Leonard Susskind who advocate it as a solution to the Cosmological Constant problem. Opponents, such as David Gross , suggest that the idea is inherently unscientific, unfalsifiable or premature. The term "landscape" comes from Evolutionary Biology (see '' Fitness Landscape '') and was first applied to cosmology by Lee Smolin in his book . It was first used in the context of string theory by Susskind. There are several popular books about the anthropic principle in cosmology. Two popular physics blogs are opposed to the anthropic principle. REFERENCES