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Alcubierre drive

From Wikipedia, the free encyclopedia


The Alcubierre metric, also known as the Alcubierre drive or Warp Drive, is a speculative 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).

In 1994, the Mexican physicist Miguel Alcubierre proposed in the Journal of Classical and Quantum Gravity 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. However, there are no known methods to create such a warp bubble in a region which does not already contain one, or to leave the bubble once inside it, so the Alcubierre drive remains a theoretical concept at this time.

Contents

[edit] 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:

ds^2 = -\left(\alpha^2- \beta_i \beta^i\right)\,dt^2+2 \beta_i \,dx^i\, dt+ \gamma_{ij}\,dx^i\,dx^j

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 (1994) is defined by:

\alpha=1\,
\beta^x=-v_s(t)f\left(r_s(t)\right),
βy = βz = 0
γij = δij

where

v_s(t)=\frac{dx_s(t)}{dt},
r_s(t)=[(x-x_s(t))^2+y^2+z^2]^{\frac{1}{2}}

and

f(r_s)=\frac{\tanh(\sigma (r_s + R))-\tanh(\sigma (r_s - R))}{2 \tanh(\sigma R)}

with R > 0 and σ > 0 arbitrary parameters. 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

-\frac{c^4}{8 \pi G} \frac{v_s^2 (x^2+y^2)}{4 g^2 r_s ^2} \left(\frac{df}{dr_s}\right)^2

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' (Alcubierre, 1994). The existence of exotic matter is not theoretically ruled out and the Casimir effect lends 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 (1999) has shown 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.

[edit] 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. Even more striking, inhabitants of the bubble feel no inertial effects. Travelers making a round trip inside a warp bubble would experience no time dilation of the kind known from the famous twin paradox from special relativity. Most physicists familiar with general relativity consider this metric to be physically unrealizable.

[edit] Mathematical representation

The Alcubierre metric may be written

ds^2 = dx^2 + dy^2 + dz^2 - 2v_s(t)f(r_s(t))\,dx\,dt + \left(v_s(t)^2 f(r_s(t))^2 -1\right)\,dt^2

where

v_s(t)=\frac{dx_s(t)}{dt}

and

r_s(t)=\sqrt{(x-x_s(t))^2+y^2+z^2}.

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.

[edit] 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. Since a ship at the center of the moving volume of the metric is at rest with respect to locally flat space, there are no relativistic mass increase or time dilation effects. The on-board spaceship clock runs at the same speed as the clock of an external observer, and that observer will detect no increase in the mass of the moving ship, even when it travels at FTL speeds. Moreover, 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. Natario has suggested a significantly different kind of warp bubble metric which does not feature expansion.

Whether the Alcubierre metric can be considered physically realistic is questionable. Normally in general relativity, one 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, and even if exotic matter is possible it also 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. Some analyses suggest that 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. Other 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. [1][2]

[edit] The Alcubierre drive and science fiction

Note that faster-than-light travel is often used in science fiction to denote a wide variety of imaginary propulsion methods, most of which have nothing to do with the Alcubierre drive or any other physical theory.

Star Trek fans claim that, in Star Trek, the Alcubierre theory has largely been accepted due to the similarity of the appropriate terms, in order to explain the apparent breaking of the laws of physics in most of the series. In fact, the physics of warp drive in Star Trek have never been defined specifically onscreen and none of the "technical manuals" based on the show has made any reference to Dr. Alcubierre's theory. As a fictional construct, the warp drive in Star Trek is vague in its specifics and changeable to suit the needs of dramatic storytelling.

In a 1978 production memo, Dr. Jesco von Puttkamer, technical advisor for Star Trek: The Motion Picture, proposed a model of warp drive which bears some striking similarities to Dr. Alcubierre's later theory, employing the same principle of a distortion in spacetime moving a ship faster than light inside a pocket of spacetime within it. (The memo is reprinted on pp. 153-4 of the book The Making of Star Trek: The Motion Picture.)

However, later Star Trek technical advisors did not follow this model, and modern Star Trek productions tend to follow a warp-drive model based on the use of "subspace" as an alternate dimensional realm through which a ship may travel at hyperlight speeds, analogous to the use of hyperspace in much science fiction. However, the specifics remain vague enough that some consider it possible to reconcile Star Trek warp drive with the Alcubierre theory (for example, see Aftermath by Christopher L. Bennett in the Starfleet Corps of Engineers Ebook series). Another, more recent book called Warp Speed by Dr. Travis S. Taylor delves more into detail about the Alcubierre theory, as well as using it as the basis for the entire book.

Although it precedes Alcubierre drive, the anime version of Captain Future featured a similar mechanism, called undulating mode.

Alcubierre drive theory is also mentioned in Orbiter, a graphic novel by Warren Ellis.


[edit] Criticisms

  • The pilot inside the bubble is causally disconnected with its walls. Therefore the bubble cannot be used for the first faster-than-light trip to a distant star. In other words, to travel to Vega (which is 26 ly 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.
  • Significant problems with the theoretical potential of this form of propulsion have been noted. Most significantly are the restrictions of quantum inequality (uncertainty principle-type inequalities that place limits on the magnitude and duration of negative energy fluxes due to quantum coherence), noted by Ford and Roman in 1995. Additionally, the rapid accumulation of large energy fluxes would appear to violate the strong, dominant and weak energy conditions.
  • All known warp drive spacetimes violate various energy conditions. It is true that certain experimentally verified quantum phenomena, such as the Casimir effect, when approximated in the context of relativistic classical field theories, lead to stress-energy tensors which also violate the energy conditions. This initially led to hope that Alcubierre type warp drives could perhaps be physically realized by clever engineering taking advantage of such quantum effects. Unfortunately, it turns out that a rather general class of warp drive spacetimes also violates certain quantum inequalities, and such violations are much harder to dismiss. The energy conditions in general relativity were never more than rough rules of thumb, but the quantum inequalities are generalizations of the uncertainty principle and seem to stand on solid ground in quantum field theory. Another problem with a large class of warp drive spacetimes is that even if the violations of the quantum inequalities were acceptable, the energy requirements may be absurdly gigantic, e.g. the mass-energy content of a star might be required to transport a small spaceship across the Milky Way galaxy. Counterarguments to these apparent problems have been offered, but not everyone is convinced they can be overcome: if they could be, it has been suggested that an intense flux of blue shifted starlight would fry any inhabitants of the bubble.
  • Perhaps the most troubling objection of all is that if warp drives were genuinely possible, we would expect to see, even in toy models such as the Alcubierre warp drive, some indication of mass-energy being gathered up, transported, concentrated, reorganized and used to create and operate the warp bubble. But by their very nature, current warp drive metrics seem to have a very different character: the bubble appears (and may eventually disappear) "spontaneously". We can observe a kind of "circulation" of energy-momentum around the bubble, but nothing which suggests a phenomenon which can be created or controlled by physical means.

[edit] Expansion on the work of Alcubierre

  • Chris Van Den Broeck tried to address potential issues in a 1999 paper also published in Classical and Quantum Gravity. By contracting the 3+1 dimensional surface area of the 'bubble' being transported by the drive, while at the same time expanding 3 dimensional the 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[3].
  • Work by González-Díaz resolved the problem of quantum instability for 2 dimensions. In his paper published in Physical Review D, Vol. 62, González-Díaz proposed considering closed, time-like curves. This refinement allows for multiply-connected spaces, closing the geodesic incompleteness and satisfying quantum instability requirements.

[edit] See also

[edit] References

  • Lobo, Francisco S. N.; & Visser, Matt (2004). "Fundamental limitations on 'warp drive' spacetimes". Class. Quant. Grav. 21: 5871-5892.  See also the eprint. arXiv. Retrieved on 23 June, 2005.
  • Natario, Jose (2002). "Warp drive with zero expansion". Class. Quant. Grav. 19: 1157-1166.  See also the eprint. arXiv. Retrieved on 23 June, 2005.
  • Broeck, Chris Van Den (1999). "A `warp drive' with more reasonable total energy requirements". Class. Quant. Grav. 16: 3973-3979.  See also the eprint. arXiv. Retrieved on 23 June, 2005.
  • Low, Robert J. (1999). "Speed Limits in General Relativity". Class. Quant. Grav. 16: 543-549.  See also the eprint version. arXiv. Retrieved on 30 June, 2005.
  • Hiscock, William A. (1997). "Quantum effects in the Alcubierre warp drive spacetime". Class. Quant. Grav. 14: L183-L188.  See also the eprint. arXiv. Retrieved on 23 June, 2005.
  • Pfenning, Michael J.; Ford, L. H. (1997). "The unphysical nature of 'Warp Drive'". Class. Quant. Grav. 14: 1743-1751.  See also the eprint. arXiv. Retrieved on 23 June, 2005.
  • Alcubierre, Miguel (1994). "The warp drive: hyper-fast travel within general relativity". Class. Quant. Grav. 11: L73-L77.  See also the eprint version. arXiv. Retrieved on 23 June, 2005., and also at iop.org
  • Low, Robert (1999). "Speed Limits in General Relativity". Class. Quantum Grav. 16: 543-549.  eprint
  • Berry, Adrian (1999). The Giant Leap: Mankind Heads for the Stars. Headline. ISBN 0-7472-7565-3.  Apparently a popular book by a science writer, on space travel in general.
  • T. S. Taylor, T. C. Powell, "Current Status of Metric Engineering with Implications for the Warp Drive," AIAA-2003-4991 39th AIAA/ASME/SAE/ASEE Joint Propulsion Conference and Exhibit, Huntsville, Alabama, July 20-23, 2003

[edit] External links

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