Dynamical Topology Change, Compactification and Waves in String Cosmology
E. Kiritsis, C. Kounnas
Abstract
Exact string solutions are presented, where moduli fields are varying with time. They provide examples where a dynamical change of the topology of space is occurring. Some other solutions give cosmological examples where some dimensions are compactified dynamically or simulate pre-big bang type scenarios. Some lessons are drawn concerning the region of validity of effective theories and how they can be glued together, using stringy information in the region where the geometry and topology are not well defined from the low energy point of view. Other time dependent solutions are presented where a hierarchy of scales is absent. Such solutions have dynamics which is qualitatively different and resemble plane gravitational waves. (Talk given at the Trieste Spring School and Workshop, 1994.)
Create a lesson
Related papers
Scale-Dependent Weak-Field Dynamics in Horndeski Theory: Galaxy Rotation Curves and Turnaround Scales
Hatice Özer
Mixed-Order Parity-Violating Corrections to Rotating Black Holes in Combined Scalar Gauss-Bonnet and Dynamical Chern-Simons Gravity
Abhishek Rout, Brett Altschul
On the Motion of a Point Electric Charge in the Field of Wu-Yang Monopoles in Bertotti-Robinson Spacetimes
Tekin Dereli, Yorgo Senikoglu
Particle dynamics in rotating charged Bumblebee black holes: An analytical correspondence with Kerr-Newman
Deyou Chen, Chuang Yang
A Unified AI Framework for Rapid and Accurate Waveform Generation of Compact Binary Coalescences
Mengfei Sun, Jin Li, Yuanhong Zhong et al.
Final state of superradiant instability in Einstein-Maxwell-dilaton black hole
Afsaneh Rahmani, Samaneh Oghbaiee