From pbranes to Dbranes
A special class of pbranes in string theory
are called D branes. Roughly speaking,
a D brane is a pbrane where the ends of open strings are localized
on the brane.
Dbranes were discovered by investigating Tduality
for open strings. Open strings don't have winding modes around compact
dimensions, so one might think that open strings behave like particles
in the presence of circular dimensions. However, the stringiness of
open strings in the presence of compact dimensions exhibits itself in
a more subtle manner, and the Tdual of an open string theory is anything
but uninteresting.
The normal open string boundary conditions in
the string oscillator expansion comes from the requirement that there
be no momentum exiting or entering through the ends of an open string.
This translates into what are called Neumann
boundary conditions at the ends of the string at (s=0)
and (s=p):
Suppose d1p of the space dimensions are compactified on a torus with
radius R, and p of the space dimensions are left noncompact as before.
In the Tdual of this string theory, the boundary conditions in those
d1p directions are changed from Neumann to Dirichlet boundary conditions
This Tdual theory has strings with ends localized in d1p directions.
So the Tdual of open strings compactified on a torus of radius R is
open strings with their ends fixed to static
pbranes, which we then call Dbranes.
D branes have been very important in understanding
string theory in general (see below) but also of crucial importance
in understanding black holes in string theory, especially in counting
the quantum states that lead to black
hole entropy.
How many dimensions?
Before string theory won the full attention
of the theoretical physics community, the most popular unified theory
was an eleven dimensional theory of supergravity, which is supersymmetry
combined with gravity. The elevendimensional spacetime was to be compactified
on a small 7dimensional sphere, leaving four spacetime dimensions visible
to observers at large distances.
This theory didn't work as a unified theory
of particle physics, because an elevendimensional quantum field theory
theory based on point particles is not renormalizable. Also, chiral
fermions cannot be defined in spacetimes with an odd number of dimensions. But
this eleven dimensional theory would not die. It eventually came back
to life in the strong coupling limit of superstring
theory in ten dimensions.
The theory currently known as M
Technically speaking, M
theory is the unknown elevendimensional theory whose low energy
limit is the supergravity theory in eleven dimensions discussed above.
However, many people have taken to also using M
theory to label the unknown theory believed to be the fundamental
theory from which the known superstring theories emerge as special limits.
We still don't know the fundamental M theory,
but a lot has been learned about the elevendimensional M theory and
how it relates to superstrings in ten spacetime dimensions.
Recall that one of the pbrane spacetimes that
are stabilized by supersymmetry is a twobrane in eleven spacetime dimensions.
This object is called the M2 brane for
short.
Type IIA superstring theory has a stable onebrane
solution called the fundamental string.
If we take M theory with the tenth space dimension compactified into
a circle of radius R, and wrap one of the dimensions of the M2 brane
around that circle, then the result is the fundamental string of the
type IIA theory. When the M2 brane is not around that circle, then the
result is the twodimensional Dbrane, the D2
brane, of the type IIA theory.
If the two theories are identified, the type IIA coupling
constant turns out to be proportional to the radius R of the compactified
tenth dimension in the M theory. So the weakly coupled limit of type
IIA superstring theory, which is the usual tendimensional theory, is
also an expansion around small R. The strong coupling limit of type
IIA theory is where R becomes very large, and the extra dimension of
spacetime is revealed. So type IIA superstring theory lives in ten spacetime
dimensions in the weak coupling limit, but eleven spacetime dimensions
in the strongly coupled limit.
We still don't know
what the fundamental theory behind string theory is, but judging
from all of these relationships, it must be a very interesting and rich
theory, one where distance scales, coupling strengths and even the number
of dimensions in spacetime are not fixed concepts but fluid entities
that shift with our point of view.
