Interfacing Friedman and String Cosmologies
نویسنده
چکیده
Compactification and symmetry breaking events in theories of heterotic superstrings implicitly indicate five inflation events. Scales of 10 ly and larger are modeled in terms of these events. The proposed model accounts qualitatively for recent observations (of galactic clusters that lie on ”thin,.. semispherical shells”) and motivates a calculation that accounts (approximately) for the observed number of galaxies. 1. Five Inflation Events Traditionally it was believed that the distribution of mass-energy was homogeneous and isotropic on scales of 10 light years and larger [J. A. Wheeler, 1974]. In recent years however, the homogeneity of the large-scale distribution has been challenged. After surveying more than 5000 galaxies, J. P. Huchra and M. Geller concluded that ”galactic clusters lie on thin, sharply defined semi-spherical shells that surround vast, empty voids.” They compared these phenomena with the ”bubblelike structures that constitute the foam in a kitchen sink” [J.P. Huchra, 1986]. Thus, while the distribution of mass-energy is isotropic (established by observations indicating that the background radiation is isotropic), it is not homogeneous. These observational results have challenged traditional theories, but it is argued here that they can be understood in terms of a supersymmetric gauge theory that indicates multiple symmetry breaking events: i.e. multiple inflation events. In the theory of superstrings, one avoids anomalies and contradictions if the dimension of spacetime is 10. Moreover, one rids the ground state of tachyons and introduces spacetime supersymmetry through GSO projections. Periodic GSO projections involve Ramon boundary conditions, which produce a Type IIA theory, containing spin-1 fields and fermions. Anti-periodic GSO projections involve Nevu-Schwarz boundary conditions, which produce a Type IIB theory, containing scaler fields and fermions. Neither theory is physical. The first is not chiral and the second contains no gauge fields. One can solve this problem however, by combining the two theories into a mixed or ’heterotic’ theory. One approach to this involves compactification of 16 dimensions from the 26 dimensional bosonic theory, which imposes a symmetry E8XE8 onto the 10-spacetime that corresponds to the heterotic theory. One E8 symmetry characterizes the observable sector while the other characterizes the hidden sector (where coupling with gauge fermions in the observable sector is strictly in terms of supergravity). When 10-spacetime is compactified to produce M4XK6, each E8 is broken to yield SU(5)XSU(3). Guth inflation [A. Guth, 1981] is a theoretical device that maintains large scale flatness by compensating (by rapid expansion) for the fattening of the vacuum that is due to a Higgs event (an event in which Higgs scalers are swallowed by other particles, imparting mass to the latter and therefore breaking the initial symmetry). Clearly however, a Guth inflation event is also called for by a compactification that increases mass-energy density;
منابع مشابه
Spatially Homogeneous String Cosmologies
We determine the most general form of the antisymmetric H-field tensor that is admitted by all possible spatially homogeneous cosmological models in 3+1dimensional low-energy bosonic string theory. The maximum number of components of the H field that are left arbitrary is found for each homogeneous cosmology defined by the Bianchi group classification. The relative generality of these string co...
متن کاملConifold Cosmologies in IIA String Theory
We discuss the extension of our recent work on M-theory conifold cosmologies to general conifold transitions and type-IIA string theory.
متن کاملNew Non-separable Diagonal Cosmologies
We find all the perfect fluid G 2 diagonal cosmologies with the property that the quotient of the norms of the two orthogonal Killing vectors is constant along each fluid world-line. We find four different families depending each one on two or three arbitrary parameters which satisfy that the metric coefficients are not separable functions. Some physical properties of these solutions including ...
متن کاملar X iv : h ep - t h / 01 10 26 2 v 1 2 9 O ct 2 00 1 1 Non - Singular String - Cosmologies From Exact Conformal Field Theories
Non-singular two and three dimensional string cosmologies are constructed using the exact conformal field theories corresponding to SO(2,1)/SO(1,1) and SO(2,2)/SO(2,1). All semi-classical curvature singularities are canceled in the exact theories for both of these cosets, but some new quantum curvature singularities emerge. However, considering different patches of the global manifolds, allows ...
متن کاملAnisotropic Null String Cosmologies
We study string propagation in an anisotropic, cosmological background. We solve the equations of motion and the constraints by performing a perturbative expansion of the string coordinates in powers of c, the world-sheet speed of light. To zeroth order the string is approximated by a tensionless string (since c is proportional to the string tension T ). We obtain exact, analytical expressions ...
متن کاملCosmological solutions of supercritical string theory
We study quintessence-driven, spatially flat, expanding FRW cosmologies that arise naturally from string theory formulated in a supercritical number of spacetime dimensions. The treelevel potential of the string theory produces an equation of state at the threshold between accelerating and decelerating cosmologies, and the resulting spacetime is globally conformally equivalent to Minkowski spac...
متن کامل