
Introducing Physical Warp Drives 3
the metric in Equation (1) with time-variable v
s
= v
s
(t) corresponds to a time-variable
stress-energy tensor which does not satisfy continuity equations. Alternatively, such
solutions may be said to require an implicit dynamical field to effectively provide
propulsion for the object, e.g. (Bassett et al. 2000). Generally, there are no self-
consistent warp drive solutions proposed in the literature which can self-accelerate at
all from zero velocities, not to mention gain superluminal speeds.
Despite the rather extensive work on the properties of the Alcubierre drive
solution, it remains unclear which of the above issues are features of the Alcubierre
solution specifically or more fundamental properties of warp drives as such. New warp
drive solutions have been introduced only in very few studies. (Van Den Broeck 1999)
reduced the energy requirements of the Alcubierre drive to about the mass of the
Sun while satisfying the vacuum energy inequalities. The reduction was realized
by decreasing the externally measured size of the warp bubble down to 10
−15
m
while keeping the internal volume constant. This solution satisfies the weak energy
conditions, although it requires that classical gravity remains applicable down to such
small scales, at which it was never tested. However, as we show in Appendix A through
a coordinate transformation, this solution is equivalent to the Alcubierre solution.
(Nat´ario 2002) constructed a warp drive solution without space contraction or
expansion, contrary to the earlier assumption that it facilitated the movement of
warp drives. (Nat´ario 2006) constructed a new subluminal warp drive solution in the
weak-field regime, which required negative energies. (Loup et al. 2001) had previously
introduced a modified version of the Alcubierre drive intended to alter the rate of
time for the observers inside the bubble. However, their modification reduces to the
original Alcubierre metric, as we also show in Appendix A. Finally, (Lentz 2020)
has recently proposed a warp drive metric claiming to have purely positive energy
everywhere in both subluminal and superluminal regimes, although without providing
means to reproduce the study.
The works above, to our knowledge, summarize all the modifications of the
Alcubierre drive available in the literature. Superluminal travel had also been studied
by (Krasnikov 1998) and (Everett & Roman 1997). In these studies, the authors
introduced Krasnikov tubes. Krasnikov tubes are ‘spacetime tunnels’ which allow for
superluminal travel without violating causality, but only for round trips and with
much larger energy requirements than the Alcubierre drive. Superluminal travel has
also been discussed in the context of wormholes, e.g. (Garattini & Lobo 2007), and
time-machine metrics, e.g. (Fermi & Pizzocchero 2018), in all cases requiring negative
energies. Finally, modified gravity theories may provide some desirable properties
for the Alcubierre drive. For instance, conformal gravity allows for construction of
Alcubierre solutions with positive energy only (Varieschi & Burstein 2013), while
extra-dimensional theories of gravity may reduce the energy requirements of the drive
(White 2013).
In this study, we show that the properties of the Alcubierre metric – in particular,
its negative energy density and the accompanying immense energy requirements – are
not a necessary feature of warp drive spacetimes. In Section 2, we discuss that any
general warp drive, including the Alcubierre metric, may be thought of as a shell of
positive- or negative-energy density material which modifies the state of spacetime in
the flat vacuum region inside it. In Section 3, we introduce, for the first time, the most
general spherically symmetric warp drives. We show that the reason for the negative
energy requirements of the Alcubierre metric and all the warp drives introduced in
the literature is, likely, the truncation of the gravitational field outside of the metric,