Perfect fluid warp drive solutions with the cosmological constant
Osvaldo L. Santos-Pereira, Everton M. C. Abreu, Marcelo B. Ribeiro

TL;DR
This paper explores solutions to Einstein's equations with a cosmological constant for the Alcubierre warp drive, revealing complex energy-matter configurations needed for superluminal travel and questioning the necessity of negative matter.
Contribution
It extends warp drive solutions to include the cosmological constant and perfect fluids, analyzing energy conditions and the complexity of matter required for superluminal speeds.
Findings
Off-diagonal energy-momentum components are necessary for warp bubble motion.
Superluminal speeds may not require negative matter.
More complex matter distributions are needed for stable warp drive solutions.
Abstract
The Alcubierre metric describes a spacetime geometry that allows a massive particle inside a spacetime distortion, called warp bubble, to travel with superluminal global velocities. In this work we advance solutions of the Einstein equations with the cosmological constant for the Alcubierre warp drive metric having the perfect fluid as source. We also consider the particular dust case with the cosmological constant, which generalizes our previous dust solution (arXiv:2008.06560) and led to vacuum solutions connecting the warp drive with shock waves via the Burgers equation, as well as our perfect fluid solution without the cosmological constant (arXiv:2101.11467). All energy conditions are also analyzed. The results show that the shift vector in the direction of the warp bubble motion creates a coupling in the Einstein equations that requires off-diagonal terms in the energy-momentum…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
