Alcubierre Warp Drive
Reaching the Nearest Star in Two
Weeks
An Overview and Comparison by Dr.
David Lewis Anderson
An Alcubierre Warp Drive stretches
spacetime in a wave
causing the fabric of space ahead of a spacecraft to contract and the space
behind it to expand. The ship can ride the wave to accelerate to high speeds
and time travel.
The Alcubierre drive, also known as the Alcubierre metric or Warp Drive, is a mathematical model of a spacetime exhibiting features reminiscent of the fictional "warp drive" from Star Trek, which can travel "faster than light" (although not in a local sense - see below). The key characteristics of the application of Alcubierre warp drives for time control and time travel are presented in the picture below. This is followed by more detail describing the effect below. Alcubierre Warp Drive Description
In
1994, the Mexican physicist Miguel Alcubierre proposed a method of stretching
space in a wave which would in theory cause the fabric of space ahead of a
spacecraft to contract and the space behind it to expand. The ship would ride
this wave inside a region known as a warp bubble of flat space.
Since
the ship is not moving within this bubble, but carried along as the region
itself moves, conventional relativistic effects such as time dilation do not
apply in the way they would in the case of a ship moving at high velocity
through flat spacetime. Also, this method of travel does not actually involve
moving faster than light in a local sense, since a light beam within the
bubble would still always move faster than the ship; it is only "faster
than light" in the sense that, thanks to the contraction of the space in
front of it, the ship could reach its destination faster than a light beam
restricted to travelling outside the warp bubble. Thus, the Alcubierre drive
does not contradict the conventional claim that relativity forbids a
slower-than-light object to accelerate to faster-than-light speeds.
Alcubierre Metric
The Alcubierre Metric defines the so-called
warp drive spacetime.
This is a Lorentzian manifold which, if interpreted in the context of general
relativity, exhibits features reminiscent of the warp drive from Star Trek: a
warp bubble appears in previously flat spacetime and moves off at effectively
superluminal speed. Inhabitants of the bubble feel no inertial effects. The
object(s) within the bubble are not moving (locally) faster than light,
instead, the space around them shifts so that the object(s) arrives at its
destination faster than light would in normal space.
Alcubierre chose a specific form for the function f, but other choices give a simpler spacetime exhibiting the desired "warp drive" effects more clearly and simply. Mathematics of the Alcubierre drive
Using
the 3+1 formalism of general relativity, the spacetime is described by a foliation
of space-like hypersurfaces of constant coordinate time t. The general form
of the Alcubierre metric is:
where α is the lapse function that gives the interval of proper time between nearby hypersurfaces, βI is the shift vector that relates the spatial coordinate systems on different hypersurfaces and γij is a positive definite metric on each of the hypersurfaces. The particular form that Alcubierre studied is defined by: 
where
and
with R > 0 and σ > 0 arbitrary parameters. Alcubierre's specific form of the metric can thus be written; 
With this particular form of the metric, it can be
shown that the energy density measured by observers whose 4-velocity is
normal to the hypersurfaces is given by
where g is the determinant
of the metric tensor. Thus, as the energy density is negative, one needs
exotic matter to travel faster than the speed of light. The existence of
exotic matter is not theoretically ruled out, the Casimir effect and the
accelerating universe both lending support to the proposed existence of such
matter. However, generating enough exotic matter and sustaining it to perform
feats such as faster-than-light travel (and also to keep open the 'throat' of
a wormhole) is thought to be impractical. Low has argued that within the
context of general relativity, it is impossible to construct a warp drive in
the absence of exotic matter. It is generally believed that a consistent
theory of quantum gravity will resolve such issues once and for all.
Physics of the Alcubierre drive
For those familiar
with the effects of special relativity, such as Lorentz contraction and time dilation, the
Alcubierre metric has some apparently peculiar aspects. In particular,
Alcubierre has shown that even when the ship is accelerating, it travels on a
free-fall geodesic. In other words, a ship using the warp to accelerate and
decelerate is always in free fall, and the crew would experience no
accelerational g-forces. Enormous tidal forces would be present near the
edges of the flat-space volume because of the large space curvature there,
but by suitable specification of the metric, these would be made very small
within the volume occupied by the ship.
The original warp drive metric, and simple variants of it, happen to have the ADM form which is often used in discussing the initial value formulation of general relativity. This may explain the widespread misconception that this spacetime is a solution of the field equation of general relativity. Metrics in ADM form are adapted to a certain family of inertial observers, but these observers are not really physically distinguished from other such families. Alcubierre interpreted his "warp bubble" in terms of a contraction of "space" ahead of the bubble and an expansion behind. But this interpretation might be misleading, since the contraction and expansion actually refers to the relative motion of nearby members of the family of ADM observers. In general relativity, one often first specifies a plausible distribution of matter and energy, and then finds the geometry of the spacetime associated with it; but it is also possible to run the Einstein field equations in the other direction, first specifying a metric and then finding the energy-momentum tensor associated with it, and this is what Alcubierre did in building his metric. This practice means that the solution can violate various energy conditions and require exotic matter.
The need for exotic
matter leads to questions about whether it is actually possible to find a way
to distribute the matter in an initial spacetime which lacks a "warp
bubble" in such a way that the bubble will be created at a later time.
Yet another problem is that, according to Serguei Krasnikov, it would be
impossible to generate the bubble without being able to force the exotic
matter to move at locally FTL speeds, which would require the existence of
tachyons. Some methods have been suggested which would avoid the problem of
tachyonic motion, but would probably generate a naked singularity at the
front of the bubble.
Difficulties
Significant problems
with the metric of this form stem from the fact that all known warp
drive spacetimes violate various energy conditions. It is true that certain
experimentally verified quantum phenomena, such as the Casimir effect, when
described in the context of the quantum field theories, lead to stress-energy
tensors which also violate the energy conditions and so one might hope that
Alcubierre type warp drives could perhaps be physically realized by clever
engineering taking advantage of such quantum effects.
However, if certain
quantum inequalities conjectured by Ford and Roman hold, then the energy
requirements for some warp drives may be absurdly gigantic, e.g. the energy
-1067gram equivalent might be required to transport a small
spaceship across the Milky Way galaxy. This is orders of magnitude greater
than the mass of the universe. Counterarguments to these apparent problems
have been offered, but not everyone is convinced they can be overcome.
Chris Van Den Broeck,
in 1999, has tried to address the potential issues. By contracting the 3+1
dimensional surface area of the 'bubble' being transported by the drive,
while at the same time expanding the 3 dimensional volume contained inside,
Van Den Broeck was able to reduce the total energy needed to transport small
atoms to less than 3 solar masses. Later, by slightly modifying the Van Den
Broeck metric, Krasnikov reduced the necessary total amount of negative
energy to a few milligrams.
Krasnikov proposed that, if tachyonic matter could not be found or used, then a solution might be to arrange for masses along the path of the vessel to be set in motion in such a way that the required field was produced. But in this case the Alcubierre Drive vessel is not able to go dashing around the galaxy at will. It is only able to travel routes which, like a railroad, have first been equipped with the necessary infrastructure.
The pilot
inside the bubble is causally disconnected with its walls and cannot carry
out any action outside the bubble. However, it is necessary to place devices
along the route in advance, and since the pilot cannot do this while "in
transit", the bubble cannot be used for the first trip to a distant
star. In other words, to travel to Vega (which is 26 light-years from the
Earth) one first has to arrange everything so that the bubble moving toward
Vega with a superluminal velocity would appear and these arrangements will
always take more than 26 years.
Coule has argued that schemes such as the one proposed by Alcubierre are not feasible because the matter to be placed on the road beforehand has to be placed at superluminal speed. Thus, according to Coule, an Alcubierre Drive is required in order to build an Alcubierre Drive. Since none have been proven to exist already then the drive is impossible to construct, even if the metric is physically meaningful. Coule argues that an analogous objection will apply to any proposed method of constructing an Alcubierre Drive. |
From The Anderson
Institute @ http://www.andersoninstitute.com/alcubierre-warp-drive.html
For more information about superluminal travel see http://nexusilluminati.blogspot.com/search/label/faster%20than$20light
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