Brandenberger–Vafa Mechanism
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In
string theory In physics, string theory is a theoretical framework in which the point-like particles of particle physics are replaced by one-dimensional objects called strings. String theory describes how these strings propagate through space and intera ...
, the Brandenberger–Vafa mechanism is an argument for why the
observable universe The observable universe is a Ball (mathematics), spherical region of the universe consisting of all matter that can be observation, observed from Earth; the electromagnetic radiation from these astronomical object, objects has had time to reach t ...
has one macroscopic timelike and three macroscopic spacelike dimensions. Its importance stems from the fact that string theory contains additional dimensions rolled up in
Planck scale In particle physics and physical cosmology, Planck units are a system of units of measurement defined exclusively in terms of four universal physical constants: '' c'', '' G'', '' ħ'', and ''k''B (described further below). Expressing one of ...
, as described by Kaluza–Klein compactification. In simple terms, the argument connected with
brane cosmology Brane cosmology refers to several theories in particle physics and cosmology related to string theory, superstring theory and M-theory. Brane and bulk The central idea is that the visible, four-dimensional spacetime is restricted to a brane i ...
claims that strings and branes wrapped around compactified dimensions cause an energy barrier, which permits their unfolding. The Brandenberger–Vafa mechanism is named after Robert Brandenberger and
Cumrun Vafa Cumrun Vafa (, ; born 1 August 1960) is an Iranian-American theoretical physicist and the Hollis Professor of Mathematicks and Natural Philosophy at Harvard University. Early life and education Cumrun Vafa was born in Tehran, Iran on 1 August 1 ...
, who first described it in 1989.


Formulation

On the basis of ten total dimensions in
superstring theory Superstring theory is an attempt to explain all of the particles and fundamental forces of nature in one theory by modeling them as vibrations of tiny supersymmetric strings. 'Superstring theory' is a shorthand for supersymmetric string t ...
, Brandenberger and Vafa argue why four dimensions "decompactify" instead of why six dimensions compactify. They begin by modelling spacelike dimensions topologically as a nine-dimensional
torus In geometry, a torus (: tori or toruses) is a surface of revolution generated by revolving a circle in three-dimensional space one full revolution about an axis that is coplanarity, coplanar with the circle. The main types of toruses inclu ...
T^9=(S^1)^9 so that each dimension can do so separatly.Kim 2006, p. 2 They furthermore assume every dimension to be of same size R, meaning the torus is \mathbb^9/R\mathbb^9 geometrically.Brandenberger & Vafa, p. 396 As remarked later, this size R should be treated quantum theoretically, although they don't do so themselves. In ordinary cosmology, models like the
Friedmann–Lemaître–Robertson–Walker metric The Friedmann–Lemaître–Robertson–Walker metric (FLRW; ) is a metric that describes a homogeneous, isotropic, expanding (or otherwise, contracting) universe that is path-connected, but not necessarily simply connected. The general form o ...
derived from
Einstein's field equations In the general theory of relativity, the Einstein field equations (EFE; also known as Einstein's equations) relate the geometry of spacetime to the distribution of matter within it. The equations were published by Albert Einstein in 1915 in th ...
can be used to get the size R in dependence of the time t (with R\propto t^Brandenberger & Vafa, p. 397) as well as the
temperature Temperature is a physical quantity that quantitatively expresses the attribute of hotness or coldness. Temperature is measurement, measured with a thermometer. It reflects the average kinetic energy of the vibrating and colliding atoms making ...
T in dependence of the size R (with T\propto 1/R). Since there is no known analogy of Einstein's field equations in string theory,Brandenberger & Vafa, p. 399 Brandenberger and Vafa use a different argument to obtain the latter, with the argument having to be modified for small sizes R as the temperature T can then exceed the
Hagedorn temperature The Hagedorn temperature, ''T''H, is the temperature in theoretical physics where hadronic matter (i.e. ordinary matter) is no longer stable, and must either "evaporate" or convert into quark matter; as such, it can be thought of as the "boiling p ...
. This is done using its
T-duality T-duality (short for target-space duality) in theoretical physics is an equivalence of two physical theories, which may be either quantum field theories or string theories. In the simplest example of this relationship, one of the theories descr ...
T(R)=T(1/R) with no physical singularity for R\rightarrow 0.Brandenberger & Easson & Kimberly 2001, Equation (15)


Literature

* * * * * {{cite journal , last=Kim , first=Jin Young , date=2006-08-18 , title=Stabilization of the Extra Dimensions in Brane Gas Cosmology with Bulk Flux , journal=
Physics Letters B Physics is the scientific study of matter, its fundamental constituents, its motion and behavior through space and time, and the related entities of energy and force. "Physical science is that department of knowledge which relates to the or ...
, volume=652 , pages=43–52 , arxiv=hep-th/0608131 , doi=10.1016/S0550-3213(01)00636-8


References


External links

* Brandenberger-Vafa mechanism on ''n''Lab String theory