Cosmological Creation of D-branes and anti-D-branes
Mahbub Majumdar, Anne-Christine Davis

TL;DR
This paper proposes a cosmological model where the early universe's space-filling branes undergo phase transitions, leading to the natural formation of D-branes, especially D3-branes, via tachyon dynamics and the Kibble mechanism.
Contribution
It introduces a novel scenario for the cosmological creation of D-branes from an initial brane-antibrane system, emphasizing entropic preferences and phase transition dynamics.
Findings
D-branes are produced during phase transitions at low temperatures.
Lower-dimensional D-branes, especially D3-branes, are exponentially favored.
At least one D-brane per Hubble volume is generated in the process.
Abstract
We argue that the early universe may be described by an initial state of space-filling branes and anti-branes. At high temperature this system is stable. At low temperature tachyons appear and lead to a phase transition, dynamics, and the creation of D-branes. These branes are cosmologically produced in a generic fashion by the Kibble mechanism. From an entropic point of view, the formation of lower dimensional branes is preferred and brane-worlds are exponentially more likely to form than higher dimensional branes. Virtually any brane configuration can be created from such phase transitions by adjusting the tachyon profile. A lower bound on the number defects produced is: one D-brane per Hubble volume.
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