Revision as of 14:53, 18 January 2005 edit155.210.68.89 (talk)No edit summary← Previous edit | Revision as of 19:51, 28 April 2005 edit undo80.221.24.175 (talk)No edit summaryNext edit → | ||
Line 1: | Line 1: | ||
'''Noncommutative quantum field theory''' is a branch of ] | '''Noncommutative quantum field theory''' is a branch of ] | ||
in which the spatial |
in which the spatial coordinates<sup>1</sup> do not commute. One (commonly | ||
studied) version of such theories has the "canonical" commutation | studied) version of such theories has the "canonical" commutation | ||
relation: | relation: | ||
Line 17: | Line 17: | ||
Various lower limits have been claimed for the noncommutative scale, | Various lower limits have been claimed for the noncommutative scale, | ||
(i.e. how accurately positions can be measured) but there is currently no | (i.e. how accurately positions can be measured) but there is currently no | ||
evidence in favour of such theory |
experimental evidence in favour of such theory or grounds for ruling them out. | ||
ruling them out). | |||
One of the novel features of noncommutative field theories is the UV/IR mixing<sup>2</sup> | |||
phenomenon in which the physics at high energies effects the physics at low energies | |||
⚫ | which does not occur in quantum field theories in which the coordinates commute. | ||
Other features include violation of ] due to the preferred direction | |||
of noncommutativity. Relativistic invariance can however be understood in the sense of | |||
] of the theory<sup>3</sup>. ] condition is possibly | |||
modified from that of the commutative theories. | |||
==History and motivation== | |||
The idea of extension of noncommutativity to the coordinates was first | |||
suggested by ] as a possible solution for removing the infinite | |||
quantities of field theories before the ] procedure was developed | |||
and had gained acceptance. | |||
The first paper on the subject was published by ]. The success of | |||
renormalization theory however drained interest from the subject for some time. | |||
In 1980s noncommutative geometry was studied and developed by mathematicians, most | |||
notably ]. The notion of of ] was | |||
generalized to a noncommutative setting. This led to an ] | |||
description of noncommutative space-times and a ] on | |||
a noncommutative ] was developed. | |||
Loosely based on the ] of ], | |||
the recent interest by the particle physics community was driven by a | the recent interest by the particle physics community was driven by a | ||
by ] and ]. |
by ] and ]. They argued that the coordinate | ||
functions of the endpoints of open strings constrained to a D-brane in the presence | |||
feature is the UV/IR mixing<sup>2</sup> in which the physics at high energies | |||
of a constant Neveu-Schwartz B-field, equivalent to a constant magnetic field | |||
has (some limited) effects on physics at low energies which does | |||
on the brane, would satisfy the noncommutative algebra presented above. | |||
⚫ | not occur in quantum field theories in which the |
||
The implication is that a quantum field theory on noncommutative space-time can | |||
be interpreted as a low energy limit of the open string theory. | |||
Another backing up the noncommutativity | |||
of space-time was presented by ], ] and ]. | |||
Their arguments was presented as follows: | |||
According to ], when the energy density grows sufficiently large, | |||
a ] is formed. On the other hand according to the ] a measurement of a space-time separation causes an uncertainty in momentum inversely proportional to | |||
the separation. Thus energy of scale corresponding to the uncertainty in momentum | |||
is localized in the system within a region corresponding to the uncertainty in | |||
position. When the separation is small enough, the ] of the | |||
system is reached and a black hole is formed, preventing any information to escape | |||
the region. Thus a lower limit is introduced for the measurement of length. | |||
A sufficient condition for preventing the gravitational collapse can be expressed | |||
as a form of uncertainty relation for the coordinates. | |||
This relation in turn can be derived from a commutation relation for the coordinates. | |||
There is a of noncommutative | There is a of noncommutative | ||
quantum field theories freely available on the web. | quantum field theories freely available on the web. | ||
It is possible to have a noncommuting time |
It is possible to have a noncommuting time coordinate | ||
but this causes many problems and most research is restricted to | but this causes many problems and most research is restricted to | ||
so-called "space-space" noncommutativity. | so-called "space-space" noncommutativity. | ||
Line 38: | Line 77: | ||
. | . | ||
See . | |||
⚫ | Alain Connes's NCG is a more general framework for geometry. Within it, the process of spontaneous symmetry breaking of QFT was reinterpreted as a usual QFT over non commutative space. | ||
⚫ | Alain Connes's NCG is a more general framework for geometry. Within it, the process of spontaneous symmetry breaking of QFT was reinterpreted as a usual QFT over non commutative space. | ||
] | ] |
Revision as of 19:51, 28 April 2005
Noncommutative quantum field theory is a branch of quantum field theory in which the spatial coordinates do not commute. One (commonly studied) version of such theories has the "canonical" commutation relation:
which means that (with any given set of axes), it is impossible to accurately measure the position of a particle with respect to more than one axis.
Various lower limits have been claimed for the noncommutative scale, (i.e. how accurately positions can be measured) but there is currently no experimental evidence in favour of such theory or grounds for ruling them out.
One of the novel features of noncommutative field theories is the UV/IR mixing phenomenon in which the physics at high energies effects the physics at low energies which does not occur in quantum field theories in which the coordinates commute.
Other features include violation of Lorentz invariance due to the preferred direction of noncommutativity. Relativistic invariance can however be understood in the sense of twist-Poicaré invariance of the theory. Causality condition is possibly modified from that of the commutative theories.
History and motivation
The idea of extension of noncommutativity to the coordinates was first suggested by Heisenberg as a possible solution for removing the infinite quantities of field theories before the renormalization procedure was developed and had gained acceptance. The first paper on the subject was published by Snyder. The success of renormalization theory however drained interest from the subject for some time. In 1980s noncommutative geometry was studied and developed by mathematicians, most notably Alain Connes. The notion of of differential structure was generalized to a noncommutative setting. This led to an operator algebraic description of noncommutative space-times and a Yang-Mills theory on a noncommutative torus was developed.
Loosely based on the noncommutative geometry of Alain Connes, the recent interest by the particle physics community was driven by a paper by Nathan Seiberg and Edward Witten. They argued that the coordinate functions of the endpoints of open strings constrained to a D-brane in the presence of a constant Neveu-Schwartz B-field, equivalent to a constant magnetic field on the brane, would satisfy the noncommutative algebra presented above. The implication is that a quantum field theory on noncommutative space-time can be interpreted as a low energy limit of the open string theory.
Another paper backing up the noncommutativity of space-time was presented by Doplicher, Fredenhagen and Roberts. Their arguments was presented as follows: According to general relativity, when the energy density grows sufficiently large, a black hole is formed. On the other hand according to the Heisenberg uncertainty principle a measurement of a space-time separation causes an uncertainty in momentum inversely proportional to the separation. Thus energy of scale corresponding to the uncertainty in momentum is localized in the system within a region corresponding to the uncertainty in position. When the separation is small enough, the Schwarzschild radius of the system is reached and a black hole is formed, preventing any information to escape the region. Thus a lower limit is introduced for the measurement of length. A sufficient condition for preventing the gravitational collapse can be expressed as a form of uncertainty relation for the coordinates. This relation in turn can be derived from a commutation relation for the coordinates.
There is a good review of noncommutative quantum field theories freely available on the web.
It is possible to have a noncommuting time coordinate but this causes many problems and most research is restricted to so-called "space-space" noncommutativity.
See for example this paper and this paper.
See this paper.
Alain Connes's NCG is a more general framework for geometry. Within it, the process of spontaneous symmetry breaking of QFT was reinterpreted as a usual QFT over non commutative space.
Category: