Is There Chaos in Low-Energy String Cosmology?
نویسنده
چکیده
Bianchi type IX, ’Mixmaster’ universes are investigated in low-energyeffective-action string cosmology. We show that, unlike in general relativity, there is no chaos in these string cosmologies for the case of the tree-level action. The characteristic Mixmaster evolution through a series of Kasner epochs is studied in detail. In the Einstein frame an infinite sequence of chaotic oscillations of the scale factors on approach to the initial singularity is impossible, as it was in general relativistic Mixmaster universes in the presence of a massless scalar field. A finite sequence of oscillations of the scale factors described by approximate Kasner metrics is possible, but it always ceases when all expansion rates become positive. In the string frame the evolution through Kasner epochs changes to a new form which reflects the duality symmetry of the theory. Again, we show that chaotic oscillations must end after a finite time. The need for duality symmetry appears to ∗E-mail:[email protected] †E-mail:[email protected] 1 be incompatible with the presence of chaotic behaviour as t → 0. We also obtain our results using the Hamiltonian qualitative cosmological picture for Mixmaster models. We also prove that a time-independent pseudoscalar axion field h is not admitted by the Bianchi IX geometry. PACS number(s): 98.80.Hw, 04.50.+h, 11.25.Mj, 98.80.Cq
منابع مشابه
String Cosmology and Chaos
We briefly review three aspects of string cosmology: (1) the " stochas-tic " approach to the pre-big bang scenario, (2) the presence of chaos in the generic cosmological solutions of the tree-level low-energy effective actions coming out of string theory, and (3) the remarkable link between the latter chaos and the Weyl groups of some hyperbolic Kac-Moody algebras. Talk given at the Francqui Co...
متن کاملString Cosmology and Chaos
We investigate Bianchi type IX ”Mixmaster” universes within the framework of the low-energy tree-level effective action for string theory, which (when the ”stringy” 2-form axion potential vanishes) is formally the same as the Brans-Dicke action with ω = −1. We show that, unlike the case of general relativity in vacuum, there is no Mixmaster chaos in these string cosmologies. In the Einstein fra...
متن کاملChaos and Symmetry in String Cosmology
We review the recently discovered interplay between chaos and symmetry in the general inhomogeneous solution of many string-related Einstein-matter systems in the vicinity of a cosmological singularity. The Belinsky-Khalatnikov-Lifshitz-type chaotic behaviour is found, for many Einstein-matter models (notably those related to the low-energy limit of superstring theory andM-theory), to be connec...
متن کاملSUSY Breaking, Cosmology, Vacuum Selection and the Cosmological Constant in String Theory
This is a summary of a loosely connected collection of results on supersymmetry (SUSY) breaking and cosmology in the context of superstring theory. The requirement of a satisfactory inflationary cosmology puts strong constraints on the superstring vacuum state. Some of these are phenomenological, i.e. certain things must be true if the theory is to reproduce observations of the Cosmic Microwave...
متن کاملSome Reflections on Moduli, Their Stabilization and Cosmology
We review some aspects of moduli in string theory. We argue that one should focus on approximate moduli spaces, and that there is evidence that such spaces exist nonperturbatively. We ask what it would mean for string theory to predict low energy supersymmetry. Aspects of two proposed mechanisms for fixing the moduli are discussed, and solutions to certain cosmological problems associated with ...
متن کامل