Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Chern–Simons theory
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==Relationships with other theories== ===Topological string theories=== {{further|Topological string theory}} In the context of [[string theory]], a ''U''(''N'') Chern–Simons theory on an oriented Lagrangian 3-submanifold M of a 6-manifold ''X'' arises as the [[string field theory]] of open strings ending on a [[D-brane]] wrapping ''X'' in the [[topological string theory#A-model|A-model]] topological string theory on ''X''. The [[topological string theory#B-model|B-model]] topological open string field theory on the spacefilling worldvolume of a stack of D5-branes is a 6-dimensional variant of Chern–Simons theory known as holomorphic Chern–Simons theory. ===WZW and matrix models=== Chern–Simons theories are related to many other field theories. For example, if one considers a Chern–Simons theory with gauge group G on a manifold with boundary then all of the 3-dimensional propagating degrees of freedom may be gauged away, leaving a [[two-dimensional conformal field theory]] known as a G [[Wess–Zumino–Witten model]] on the boundary. In addition the ''U''(''N'') and SO(''N'') Chern–Simons theories at large ''N'' are well approximated by [[matrix theory (physics)|matrix models]]. ===Chern–Simons gravity theory=== {{See also|(2+1)-dimensional topological gravity}} In 1982, [[Stanley Deser|S. Deser]], [[Roman Jackiw|R. Jackiw]] and S. Templeton proposed the Chern–Simons gravity theory in three dimensions, in which the [[Einstein–Hilbert action]] in gravity theory is modified by adding the Chern–Simons term. ({{harvtxt|Deser|Jackiw|Templeton|1982}}) In 2003, R. Jackiw and S. Y. Pi extended this theory to four dimensions ({{harvtxt|Jackiw|Pi|2003}}) and Chern–Simons gravity theory has some considerable effects not only to fundamental physics but also condensed matter theory and astronomy. The four-dimensional case is very analogous to the three-dimensional case. In three dimensions, the gravitational Chern–Simons term is :<math>\operatorname{CS}(\Gamma)=\frac{1}{2\pi^2}\int d^3x\varepsilon^{ijk}\biggl(\Gamma^p_{iq}\partial_j\Gamma^q_{kp}+\frac{2}{3}\Gamma^p_{iq}\Gamma^q_{jr}\Gamma^r_{kp}\biggr).</math> This variation gives the [[Cotton tensor]] :<math>=-\frac{1}{2\sqrt{g}}\bigl(\varepsilon^{mij}D_i R^n_j+\varepsilon^{nij}D_i R^m_j).</math> Then, Chern–Simons modification of three-dimensional gravity is made by adding the above Cotton tensor to the field equation, which can be obtained as the vacuum solution by varying the Einstein–Hilbert action. ===Chern–Simons matter theories=== In 2013 Kenneth A. Intriligator and [[Nathan Seiberg]] solved these 3d Chern–Simons gauge theories and their phases using [[Seiberg-Witten monopole|monopole]]s carrying extra degrees of freedom. The [[Witten index]] of the many [[vacuum state|vacua]] discovered was computed by compactifying the space by turning on mass parameters and then computing the index. In some vacua, [[supersymmetry]] was computed to be broken. These monopoles were related to [[condensed matter physics|condensed matter]] [[quantum vortex|vortices]]. ({{harvtxt|Intriligator|Seiberg|2013}}) The ''N'' = 6 Chern–Simons matter theory is the [[AdS/CFT correspondence|holographic dual]] of M-theory on <math>AdS_4\times S_7</math>. ===Four-dimensional Chern–Simons theory=== {{See also|Four-dimensional Chern–Simons theory}} In 2013 [[Kevin Costello]] defined a closely related theory defined on a four-dimensional manifold consisting of the product of a two-dimensional 'topological plane' and a two-dimensional (or one complex dimensional) complex curve.<ref>{{cite arXiv |last1=Costello |first1=Kevin |title=Supersymmetric gauge theory and the Yangian |date=2013 |class=hep-th |eprint=1303.2632 }}</ref> He later studied the theory in more detail together with Witten and Masahito Yamazaki,<ref name="CWY1">{{cite journal |last1=Costello |first1=Kevin |last2=Witten |first2=Edward |last3=Yamazaki |first3=Masahito |title=Gauge Theory And Integrability, I |journal=Notices of the International Congress of Chinese Mathematicians |date=2018 |volume=6 |issue=1 |pages=46–119 |doi=10.4310/ICCM.2018.v6.n1.a6 |arxiv=1709.09993 }}</ref><ref name="CWY2">{{cite journal |last1=Costello |first1=Kevin |last2=Witten |first2=Edward |last3=Yamazaki |first3=Masahito |title=Gauge Theory And Integrability, II |journal=Notices of the International Congress of Chinese Mathematicians |date=2018 |volume=6 |issue=1 |pages=120–146 |doi=10.4310/ICCM.2018.v6.n1.a7 |arxiv=1802.01579 |s2cid=119592177 }}</ref><ref name="CY">{{cite arXiv|last1=Costello |first1=Kevin |last2=Yamazaki |first2=Masahito |title=Gauge Theory And Integrability, III |date=2019 |class=hep-th |eprint=1908.02289 }}</ref> demonstrating how the gauge theory could be related to many notions in [[integrable system]]s theory, including exactly solvable lattice models (like the [[six-vertex model]] or the [[Quantum Heisenberg model|XXZ spin chain]]), integrable quantum field theories (such as the [[Gross–Neveu model]], [[Chiral model|principal chiral model]] and symmetric space coset [[sigma model]]s), the [[Yang–Baxter equation]] and [[quantum groups]] such as the [[Yangian]] which describe symmetries underpinning the integrability of the aforementioned systems. The action on the 4-manifold <math>M = \Sigma \times C</math> where <math>\Sigma</math> is a two-dimensional manifold and <math>C</math> is a complex curve is <math display = block>S = \int_M \omega \wedge CS(A)</math> where <math>\omega</math> is a [[meromorphic]] [[one-form]] on <math>C</math>.
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)