Wednesday 2 January 2008

M-theory



John Henry Schwarz (born November 22, 1941) is an American theoretical physicist.Along with Yoichiro Nambu, Holger Bech Nielsen, Joël Scherk, Gabriele Veneziano, Michio Kaku,Michael Green, Leonard Susskind, and Edward Witten, he is regarded as one of the fathers of string theory.


456 Lauritsen Laboratory
Caltech 452-48
Pasadena CA 91125 		jhs@theory.caltech.edu
Phone:(626) 395-6642
Fax:(626) 568-8473

Research Interests

The strong nuclear force that binds quarks together inside protons, neutrons and other hadrons was not yet understood in the 1960s. During that decade, theorists faced the challenge of finding a simple explanation for the wealth of data that the experimentalists were producing with their large accelerators. I was a student in Berkeley, where Professors Geoffrey Chew, Stanley Mandelstam and others were developing ideas such as the "bootstrap hypothesis" and "Regge pole theory". These approaches were not fully successful, but by a remarkable sequence of events they led to superstring theory.

Around 1970 (when I was a postdoc at Princeton), Gabriele Veneziano, Yoichiro Nambu and others developed the "dual resonance model", later interpreted as the theory of a relativistic string. This model incorporates the bootstrap and Regge ideas in a specific mathematical framework and thus was able to describe many qualitative features of hadron physics. In 1971 a second (somewhat better) dual model was discovered by Pierre Ramond, André Neveu and me. Both models shared certain defects, however: They required more than four dimensions for space-time and predicted the existence of massless particles, which do not exist in the hadron spectrum. Various tricks were developed for dealing with the extra dimensions, but no amount of cleverness could get rid of the massless particles.

The final nail was driven into the coffin of string theory in 1973-74, when "quantum chromodynamics" (QCD) emerged as a theory of the strong nuclear force. Its successes were immediate and convincing. String Theory, a very active area of research for almost five years, dried up practically overnight.

In 1972 I moved to Caltech, and in 1974 I arranged a visit by Joël Scherk, a French physicist with whom I had worked earlier in Princeton. We felt strongly that string theory was too beautiful a mathematical structure to be completely irrelevant to nature. We were convinced of the essential correctness of QCD, but still thought that string theory deserved a last look before being abandoned. Soon we realized that its defects could be turned into virtues if it was used for a completely different purpose than that for which it was originally developed.

Massless particles do occur in nature: The quanta of light (photons) and of gravity (gravitons) are examples. These particles are not hadrons, however. Indeed, all consistent versions of the string theories we knew about contained a massless particle with exactly the properties of a graviton. Its interactions at low energy were shown to agree precisely with Einstein's general theory of relativity. (This result was obtained independently by the Japanese physicist Tamiaka Yoneya.) Also, it was known since the work of Kaluza and Klein in the 1920s that extra dimensions of space can play a useful role in gravitation theories, where the geometry of space-time is dynamical.

Since my training was as an elementary particle physicist, gravity was far from my mind in early 1974. Traditionally, elementary particle physicists ignored the gravitational force, which is entirely negligible under ordinary circumstances. For example, the gravitational attraction between an electron and proton in a hydrogen atom is about 1038 times weaker than the electric attraction. General relativists, physicists who specialize in the study of gravity, generally study the largest things in the universe (even the universe itself) and have traditionally had no use for subnuclear physics. They attended different meetings, read different journals, and (until recently) had no need for serious communication with particle physicists, just as particle physicists (until recently) felt they had no need for galaxies, black holes and the early universe in their quest to understand elementary particles.

For these reasons, even when Scherk and I realized that string theory had mathematical features suggestive of gravity, we were not predisposed at first to interpret it as a physical theory of gravity. Fortunately, after a few weeks of intense deliberations, we were ready to take the plunge.

Thus Scherk and I proposed reinterpreting string theory as a candidate for a unified theory of gravity and the other fundamental forces. This was a radical change in viewpoint that required, among other things, supposing that the size of a string is approximately equal to the Planck length 10-33 cm) in order for the gravitational force to have the correct Newtonian strength. This is 20 orders of magnitude smaller than what was envisioned when strings were being used to describe hadrons, whose typical size is 10-13 cm.

In addition to incorporating gravity in a unified theory there was another bonus. All previous attempts to include gravity in the framework of quantum field theory had led to formulas that were plagued by meaningless infinities. We knew that string theories have a much "softer" short-distance behavior, and we were therefore optimistic that this problem would not occur. Recent studies support this conclusion.

Scherk and I were very excited by the possibility that string theory could be the Holy Grail of unified field theory, overcoming the problems that had stymied other approaches. In addition to publishing our work in scholarly journals we gave numerous lectures at conferences and physics departments all over the world. We even submitted a paper to the 1975 essay competition of the Gravity Research Foundation. For the most part our work was politely received --- as far as I know, no one accused us of being crackpots. Yet, for a decade, almost none of the experts took the proposal seriously. I suspect that very few physicists even remember having heard of the proposal in 1974 or 1975.

In 1980, Michael Green and I began collaborating on the further development of superstring theory. Each year we made discoveries that we felt would convince other physicists of the virtue of string theory. This did not happen until after a discovery we made in the summer of 1984 while working at the Aspen Center for Physics, which showed how certain apparent inconsistencies, called anomalies, could be avoided. The subject suddenly became very fashionable and is now one of the most active areas of research in theoretical physics.

Added & Edited
By: Arip Nurahman
Department of Physics, Faculty of Sciences and Mathematics
Indonesia University of Education

and

Follower Open Course Ware at Massachusetts Institute of Technology
Cambridge, USA
Department of Physics
http://web.mit.edu/physics/
http://ocw.mit.edu/OcwWeb/Physics/index.htm
&
Aeronautics and Astronautics Engineering
http://web.mit.edu/aeroastro/www/
http://ocw.mit.edu/OcwWeb/Aeronautics-and-Astronautics/index.htm















In theoretical physics, M-theory is a new limit of string theory in which 11 dimensions of spacetime may be identified. Because the dimensionality exceeds the dimensionality of five superstring theories in 10 dimensions, it was originally believed that the 11-dimensional theory is more fundamental and unifies all string theories (and supersedes them). However, in a more modern understanding, it is another, sixth possible description of physics of the full theory that is still called "string theory." Though a full description of the theory is not yet known, the low-entropy dynamics are known to be supergravity interacting with 2- and 5-dimensional membranes.
This theory is the unique supersymmetric theory in eleven dimensions, with its low-entropy matter content and interactions fully determined, and can be obtained as the strong coupling limit of type IIA string theory because a new dimension of space emerges as the coupling constant increases.

Drawing on the work of a number of string theorists (including Ashoke Sen, Chris Hull, Paul Townsend, Michael Duff and John Schwarz), Edward Witten of the Institute for Advanced Study suggested its existence at a conference at USC in 1995, and used M-theory to explain a number of previously observed dualities, sparking a flurry of new research in string theory called the second superstring revolution.

According to Witten and others, the M in M-theory could stand for master, mathematical, mother, mystery, membrane, magic, or matrix. Witten reluctantly admits the M in M-theory can also stand for murky because the level of understanding of the theory is so primitive. [1] However, originally the letter was taken from membrane, but since Witten was more skeptical to membranes than his colleagues, he just kept the "M". Later, he let the meaning be a matter of taste for the user of the word "M-theory".[2]

In the early 1990s, it was shown that the various superstring theories were related by dualities, which allow physicists to relate the description of an object in one super string theory to the description of a different object in another super string theory. These relationships imply that each of the super string theories is a different aspect of a single underlying theory, proposed by Witten, and named "M-theory".

M-theory is not yet complete; however it can be applied in many situations (usually by exploiting string theoretic dualities). The theory of electromagnetism was also in such a state in the mid-19th century; there were separate theories for electricity and magnetism and, although they were known to be related, the exact relationship was not clear until James Clerk Maxwell published his equations, in his 1864 paper A Dynamical Theory of the Electromagnetic Field. Witten has suggested that a general formulation of M-theory will probably require the development of new mathematical language. However, some scientists have questioned the tangible successes of M-theory given its current incompleteness, and limited predictive power, even after so many years of intense research.

In late 2007, Bagger, Lambert and Gustavsson set off renewed interest in M-theory with the discovery of a candidate Lagrangian description of coincident M2-branes, based on a non-associative generalization of Lie Algebra, Nambu 3-algebra or Filippov 3-algebra. Practitioners hope the Bagger-Lambert-Gustavsson action (BLG action) will provide the long-sought microscopic description of M-theory.

Contents




History and Development

Prior to May 1995

Prior to 1995 there were five (known) consistent superstring theories (here on referred to as string theories), which were given the names Type I string theory, Type IIA string theory, Type IIB string theory, heterotic SO(32) (the HO string) theory, and heterotic E8×E8 (the HE string) theory. The five theories all share essential features that relate them to the name of string theory. Each theory is fundamentally comprised of vibrating, one dimensional strings at approximately the length of the Planck length. Calculations have also shown that each theory requires more than the normal four spacetime dimensions (although all extra dimensions are in fact spatial.) However, when the theories are analyzed in detail, significant differences appear.

Type I string theory and others

 

The Type I string theory has vibrating strings like the rest of the string theories. These strings vibrate both in closed loops, so that the strings have no ends, and as open strings with two loose ends. The open loose strings are what separates the Type I string theory from the other four string theories. This was a feature that the other string theories did not contain (The Type IIA and Type IIB string theories also contain open strings, however these strings are bound to D-branes, that is to say, they are tight).

String vibrational patterns

The calculations of the String Vibrational Patterns show that the list of string vibrational patterns and the way each pattern interacts and influences others vary from one theory to another. These and other differences hindered the development of the string theory as being the theory that united quantum mechanics and general relativity successfully. Attempts by the physics community to eliminate four of the theories, leaving only one string theory, have not been successful.

M-theory




M-theory attempts to unify the five string theories by examining certain identifications and dualities. Thus each of the five string theories becomes a special case of M-theory.
As the names suggest, some of these string theories were thought to be related to each other. In the early 1990s, string theorists discovered that some relations were so strong that they could be thought of as an identification.


Type IIA and Type IIB

 

The Type IIA string theory and the Type IIB string theory were known to be connected by T-duality; this essentially meant that the IIA string theory description of a circle of radius R is exactly the same as the IIB description of a circle of radius 1/R, where distances are measured in units of the Planck length.

This was a profound result. First, this was an intrinsically quantum mechanical result; the identification did not hold in the realm of classical physics. Second, because it is possible to build up any space by gluing circles together in various ways it would seem that any space described by the IIA string theory can also be seen as a different space described by the IIB theory. This implies that the IIA string theory can identify with the IIB string theory: any object which can be described with the IIA theory has an equivalent, although seemingly different, description in terms of the IIB theory. This suggests that the IIA string theory and the IIB string theory are really aspects of the same underlying theory.

Other dualities

There are other dualities between the other string theories. The heterotic SO(32) and the heterotic E8×E8 theories are also related by T-duality; the heterotic SO(32) description of a circle of radius R is exactly the same as the heterotic E8×E8 description of a circle of radius 1/R. This implies that there are really only three superstring theories, which might be called (for discussion) the Type I theory, the Type II theory, and the heterotic theory.

There are still more dualities, however. The Type I string theory is related to the heterotic SO(32) theory by S-duality; this means that the Type I description of weakly interacting particles can also be seen as the heterotic SO(32) description of very strongly interacting particles. This identification is somewhat more subtle, in that it identifies only extreme limits of the respective theories. String theorists have found strong evidence that the two theories are really the same, even away from the extremely strong and extremely weak limits, but they do not yet have a proof strong enough to satisfy mathematicians. However, it has become clear that the two theories are related in some fashion; they appear as different limits of a single underlying theory.

Only two string theories

Given the above commonalities there appear to be only two string theories: the heterotic string theory (which is also the type I string theory) and the type II theory. There are relations between these two theories as well, and these relations are in fact strong enough to allow them to be identified.

Last step

 

This last step is best explained first in a certain limit. In order to describe our world, strings must be extremely tiny objects. So when one studies string theory at low energies, it becomes difficult to see that strings are extended objects — they become effectively zero-dimensional (pointlike). Consequently, the quantum theory describing the low energy limit is a theory that describes the dynamics of these points moving in spacetime, rather than strings. Such theories are called quantum field theories. However, since string theory also describes gravitational interactions, one expects the low-energy theory to describe particles moving in gravitational backgrounds. Finally, since superstring string theories are supersymmetric, one expects to see supersymmetry appearing in the low-energy approximation. These three facts imply that the low-energy approximation to a superstring theory is a supergravity theory.

Supergravity theories

 

 

The possible supergravity theories were classified by Werner Nahm in the 1970s. In 10 dimensions, there are only two supergravity theories, which are denoted Type IIA and Type IIB. This similar denomination is not a coincidence; the Type IIA string theory has the Type IIA supergravity theory as its low-energy limit and the Type IIB string theory gives rise to Type IIB supergravity. The heterotic SO(32) and heterotic E8×E8 string theories also reduce to Type IIA and Type IIB supergravity in the low-energy limit. This suggests that there may indeed be a relation between the heterotic/Type I theories and the Type II theories.

In 1994, Edward Witten outlined the following relationship: The Type IIA supergravity (corresponding to the heterotic SO(32) and Type IIA string theories) can be obtained by dimensional reduction from the single unique eleven-dimensional supergravity theory. This means that if one studied supergravity on an eleven-dimensional spacetime that looks like the product of a ten-dimensional spacetime with another very small one-dimensional manifold, one gets the Type IIA supergravity theory. (And the Type IIB supergravity theory can be obtained by using T-duality.) However, eleven-dimensional supergravity is not consistent on its own — it does not make sense at extremely high energy, and likely requires some form of completion. It seems plausible, then, that there is some quantum theory — which Witten dubbed M-theory — in eleven-dimensions which gives rise at low energies to eleven-dimensional supergravity, and is related to ten-dimensional string theory by dimensional reduction. Dimensional reduction to a circle yields the Type IIA string theory, and dimensional reduction to a line segment yields the heterotic SO(32) string theory.

Same underlying theory

M-theory would implement the notion that all of the different string theories are different special cases and/or different presentations of the same underlying theory (M-theory). Thus the concept of string theory is expanded. Unfortunately little is known about M-theory, but there is a great deal of interest in the concept from the theoretical physics community. Computations in M-theory and string theory in general are extremely complex, so concrete results are very difficult to produce. It may be some time before the full implications of these theories are known.

The promise of M-theory is that all of the different string theories would become different limits of a single underlying theory.

Nomenclature

There are two issues to be dealt with here:
  • When Witten named M-theory, he did not specify what the "M" stood for, presumably because he did not feel he had the right to name a theory which he had not been able to fully describe. According to Witten himself, "'M' stands for "magic," "mystery" , or "matrix", according to taste."[3] According to the BBC/TLC documentary Parallel Universes, the M stands for "membrane". Other suggestions by people such as Michio Kaku, Michael Duff and Neil Turok in that documentary are "mother" (as in "mother of all theories"), and "master" theory.[4]
Cynics have noted that the M might be an upside down "W", standing for Witten. Others have suggested that for now, the "M" in M-theory should stand for Missing or Murky[5]. The various speculations as to what "M" in "M-theory" stands for are explored in the PBS documentary based on Brian Greene's book The Elegant Universe.
  • The name M-theory is slightly ambiguous. It can be used to refer to both the particular eleven-dimensional theory which Witten first proposed, or it can be used to refer to a kind of theory which looks in various limits like the various string theories. Ashoke Sen has suggested that more general theory could go by the name U-theory, which might stand for Ur, Uber, Ultimate, Underlying, or perhaps Unified. (It might also stand for U-duality, which is both a reference to Sen's own work and a kind of particle physics pun.)
M-theory in the following descriptions refers to the more general theory, and will be specified when used in its more limited sense.

M-theory and membranes

 

In the standard string theories, strings are assumed to be the single fundamental constituent of the universe. M-theory adds another fundamental constituent - membranes. Like the tenth spatial dimension, the approximate equations in the original five superstring models proved too weak to reveal membranes.

P-branes

A membrane, or brane, is a multidimensional object, usually called a P-brane, with P referring to the number of dimensions in which it exists. The value of 'P' can range from zero to nine, thus giving branes dimensions from zero (0-brane ≡ point particle) to nine - five more than the world we are accustomed to inhabiting (3 spatial and 1 time). The inclusion of p-branes does not render previous work in string theory wrong on account of not taking note of these P-branes. P-branes are much more massive ("heavier") than strings, and when all higher-dimensional P-branes are much more massive than strings, they can be ignored, as researchers had done unknowingly in the 1970s.

Strings with "loose ends"

Shortly after Witten's breakthrough in 1995, Joseph Polchinski of the University of California, Santa Barbara discovered a fairly obscure feature of string theory. He found that in certain situations the endpoints of strings (strings with "loose ends") would not be able to move with complete freedom as they were attached, or stuck within certain regions of space. Polchinski then reasoned that if the endpoints of open strings are restricted to move within some p-dimensional region of space, then that region of space must be occupied by a p-brane. These type of "sticky" branes are called Dirichlet-P-branes, or D-p-branes. His calculations showed that the newly discovered D-P-branes had exactly the right properties to be the objects that exert a tight grip on the open string endpoints, thus holding down these strings within the p-dimensional region of space they fill.

Strings with closed loops

 

Not all strings are confined to p-branes. Strings with closed loops, like the graviton, are completely free to move from membrane to membrane. Of the four force carrier particles, the graviton is unique in this way. Researchers speculate that this is the reason why investigation through the weak force, the strong force, and the electromagnetic force have not hinted at the possibility of extra dimensions. These force carrier particles are strings with endpoints that confine them to their p-branes. Further testing is needed in order to show that extra spatial dimensions indeed exist through experimentation with gravity.

Membrane Interactions

File:Membrane interactions.JPG
The basic orientable 2-brane interactions
One of the reasons M-theory is so difficult to formulate is that the numbers of different types of membranes in the various dimensions increases exponentially. For example once you get to 3 dimensional surfaces you have to deal with solid objects with knot shaped holes, and then you need the whole of knot theory just to classify them. Since M-theory is thought to operate in 11 dimensions this problem then becomes very difficult. But just like string theory, in order for the theory to satisfy causality, the theory must be local, and so the topology changing must occur at a single point. The basic orientable 2-brane interactions are easy to show. Orientable 2-branes are tori with multiple holes cut out of them.

Matrix theory



The original formulation of M-theory was in terms of a (relatively) low-energy effective field theory, called 11-dimensional Super gravity. Though this formulation provided a key link to the low-energy limits of string theories, it was recognized that a full high-energy formulation (or "UV-completion") of M-theory was needed.

Analogy with water

For an analogy, the Super gravity description is like treating water as a continuous, incompressible fluid. This is effective for describing long-distance effects such as waves and currents, but inadequate to understand short-distance/high-energy phenomena such as evaporation, for which a description of the underlying molecules is needed. What, then, are the underlying degrees of freedom of M-theory?

9 matrices

Banks, Fischler, Shenker and Susskind (BFSS) conjectured that Matrix theory could provide the answer. They demonstrated that a theory of 9 very large matrices, evolving in time, could reproduce the Super gravity description at low energy, but take over for it as it breaks down at high energy. While the Super gravity description assumes a continuous space-time, Matrix theory predicts that, at short distances, non-commutative geometry takes over, somewhat similar to the way the continuum of water breaks down at short distances in favor of the graininess of molecules.

See also

References

  1. ^ Woit, Peter (September 30, 2006). Not Even Wrong: The Failure of String Theory And the Search for Unity in Physical Law. Basic Books. pp. 155. ISBN 0465092756.
  2. ^ Edward Witten, in a radio interview in "Vetandets värld" on Swedish public radio, 2008-06-06, http://www.sr.se/webbradio/?Type=db&Id=1182281
  3. ^ "The Theory Formerly Known As Strings" (page 64)
  4. ^ Parallel Universes; BBC/TLC
  5. ^ String People: Ed Witten

Books

External links

  • The Elegant Universe - A Three-Hour Miniseries with Brian Greene by NOVA (original PBS Broadcast Dates: October 28, 8-10 p.m. and November 4, 8-9 p.m., 2003). Various images, texts, videos and animations explaining string theory and M-theory.
  • Superstringtheory.com - The "Official String Theory Web Site", created by Patricia Schwarz. Excellent references on string theory and M-theory for the layperson and expert.
  • Basics of M-Theory by A. Miemiec and I. Schnakenburg is a lecture note on M-Theory published in Fortsch.Phys.54:5-72,2006.
  • M-Theory-Cambridge
  • M-Theory-Caltech
  • [3] The Science Channel explained String Theory, Super Gravity and M-Theory on Sci-Q Sundays with Dr. Michio Kaku.
Retrieved from "http://en.wikipedia.org/wiki/M-theory"

Diposting oleh Astrophysics Boy di 00:57:00 0 komentar

Subscribe to: Posts (Atom)