Cosmic acceleration from M theory on twisted spaces
نویسندگان
چکیده
In a recent paper [I. P. Neupane and D. L. Wiltshire, Phys. Lett. B 619, 201 (2005).] we have found a new class of accelerating cosmologies arising from a time–dependent compactification of classical supergravity on product spaces that include one or more geometric twists along with nontrivial curved internal spaces. With such effects, a scalar potential can have a local minimum with positive vacuum energy. The existence of such a minimum generically predicts a period of accelerated expansion in the four-dimensional Einstein-conformal frame. Here we extend our knowledge of these cosmological solutions by presenting new examples and discuss the properties of the solutions in a more general setting. We also relate the known (asymptotic) solutions for multi-scalar fields with exponential potentials to the accelerating solutions arising from simple (or twisted) product spaces for internal manifolds.
منابع مشابه
Accelerating cosmologies from exponential potentials
It is learnt that exponential potentials of the form V ∼ exp(−2cφ/Mp) arising from the hyperbolic compactification of higher-dimensional theories are of interest for getting short periods of accelerated cosmological expansions. Using such a potential derived for the combined case of hyperbolic-flux compactification, we study a fourdimensional flat (or open) FRW cosmolgy and give analytic (and n...
متن کاملCosmic Acceleration and M-theory
The status of accelerating four-dimensional universes obtained by timedependent compactifications of 10 or 11 dimensional supergravity is reviewed, as is the ‘no-go’ theorem that they evade. All flat cosmologies for a simple exponential potential are found explicitly. It is noted that transient acceleration is generic, and unavoidable for ‘flux’ compactifications. Included is an eternally accel...
متن کاملCosmic Ray Acceleration at Relativistic Shock Waves
Theory of the first-order Fermi acceleration of cosmic ray particles at relativistic shock waves is reviewed. We consider shocks with parallel and oblique, suband super-luminal magnetic field configurations and with finite-amplitude magnetic field perturbations. A role of oblique field configurations and field perturbations in forming the cosmic ray energy spectrum and changing the acceleration...
متن کاملOn the possible reason for non-detection of TeV-protons in SNRs
The theory of shock acceleration predicts the maximum particle energy to be limited only by the acceleration time and the size (geometry) of the shock. This led to optimistic estimates for the galactic cosmic ray energy achievable in the SNR shocks. The estimates imply that the accelerated particles, while making no strong impact on the shock structure (test particle approach) are nevertheless ...
متن کاملON THE POSSIBLE REASON FOR NONDETECTION OF TeV PROTONS IN SUPERNOVA REMNANTS
The theory of shock acceleration predicts the maximum particle energy to be limited only by the acceleration time and the size (geometry) of the shock. This led to optimistic estimates for the galactic cosmic-ray energy achievable in supernova remnant (SNR) shocks. The estimates imply that the accelerated particles, while making no strong impact on the shock structure (test-particle approach), ...
متن کامل