D-brane worlds and the cosmological constant
P. Gusin, J. Warczewski

TL;DR
This paper investigates the cosmological constant on a D-brane within p-brane backgrounds, deriving the energy-momentum tensor and analyzing the properties of the resulting perfect fluid, including its energy density, pressure, and sound speed.
Contribution
It provides a detailed derivation of the cosmological constant and energy-momentum tensor for a D-brane in p-brane backgrounds, interpreting it as a perfect fluid with specific properties.
Findings
Negative pressure on the D-brane fluid
Real speed of sound despite negative pressure
Explicit form of the energy-momentum tensor
Abstract
The cosmological constant on a D-brane is analyzed. This D-brane is in the background produced by the p-brane solutions. The energy-momentum tensor in this model has been found and the form of the cosmological constant has been derived. This energy-momentum tensor is interpreted as an energy-momentum tensor for a perfect fluid on the D-brane. The energy density and the pressure for this fluid have been derived. As it turned out the pressure is negative but the speed of sound is real.
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