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Warp drive aerodynamics
by
Martín-Martínez, Eduardo
, Barceló, Carlos
, Garay, Luis J.
, Boyanov, Valentin
, Sánchez Velázquez, Jose M.
in
Black Holes
/ Classical and Quantum Gravitation
/ Classical Theories of Gravity
/ Elementary Particles
/ Energy
/ Geodesy
/ High energy physics
/ Models of Quantum Gravity
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ Renormalization and Regularization
/ Science fiction & fantasy
/ Spacetime
/ String Theory
/ Warp drives
2022
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Warp drive aerodynamics
by
Martín-Martínez, Eduardo
, Barceló, Carlos
, Garay, Luis J.
, Boyanov, Valentin
, Sánchez Velázquez, Jose M.
in
Black Holes
/ Classical and Quantum Gravitation
/ Classical Theories of Gravity
/ Elementary Particles
/ Energy
/ Geodesy
/ High energy physics
/ Models of Quantum Gravity
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ Renormalization and Regularization
/ Science fiction & fantasy
/ Spacetime
/ String Theory
/ Warp drives
2022
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Warp drive aerodynamics
by
Martín-Martínez, Eduardo
, Barceló, Carlos
, Garay, Luis J.
, Boyanov, Valentin
, Sánchez Velázquez, Jose M.
in
Black Holes
/ Classical and Quantum Gravitation
/ Classical Theories of Gravity
/ Elementary Particles
/ Energy
/ Geodesy
/ High energy physics
/ Models of Quantum Gravity
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ Renormalization and Regularization
/ Science fiction & fantasy
/ Spacetime
/ String Theory
/ Warp drives
2022
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Journal Article
Warp drive aerodynamics
2022
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Overview
A
bstract
In this work we analyse the potential for a warp drive spacetime to develop instabilities due to the presence of quantum matter. Particularly, we look for points of infinite blueshift (which are analogous to points of a black hole inner horizon, known for its semiclassical instability), and categorise them through the behaviour of geodesics in their vicinity. We find that warp-drive bubbles in dimension 2+1 or higher are in fact likely to be stable, as they generally contain only isolated points where divergences are approached, leading to a finite limit for the overall accumulation of destabilising energy. Furthermore, any semiclassical instabilities in the warp drive due to energy-density buildups can be further diminished with particular, more “aerodynamic” shapes and trajectories for the drive.
Publisher
Springer Berlin Heidelberg,Springer Nature B.V,SpringerOpen
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