This article will be permanently flagged as inappropriate and made unaccessible to everyone. Are you certain this article is inappropriate? Excessive Violence Sexual Content Political / Social
Email Address:
Article Id: WHEBN0000260836 Reproduction Date:
In theoretical and mathematical physics, twistor theory maps the geometric objects of conventional 3+1 space-time (Minkowski space) into geometric objects in a 4-dimensional space endowed with a Hermitian form of signature (2,2). This space is called twistor space, and its complex valued coordinates are called "twistors."
Twistor theory was first proposed by Roger Penrose in 1967,^{[1]} as a possible path to a theory of quantum gravity. The twistor approach is especially natural for solving the equations of motion of massless fields of arbitrary spin.
In 2003, Edward Witten^{[2]} proposed uniting twistor and string theory by embedding the topological B model of string theory in twistor space. His objective was to model certain Yang–Mills amplitudes. The resulting model has come to be known as twistor string theory (read below). Simone Speziale and collaborators have also applied it to loop quantum gravity.^{[3]}
Twistor theory is unique to 4D Minkowski space and the (2,2) signature, and does not generalize to other dimensions or signatures. At the heart of twistor theory lies the isomorphism between the conformal group Spin(4,2) and SU(2,2), which is the group of unitary transformations of determinant 1 over a four-dimensional complex vector space that leave invariant a Hermitian form of signature (2,2), see classical group.
\mathbb{M}^c, \mathbb{PT}^+, \mathbb{PN} and \mathbb{PT}^- are all homogeneous spaces of the conformal group.
\mathbb{M}^c admits a conformal metric (i.e., an equivalence class of metric tensors under Weyl rescalings) with signature (+++−). Straight null rays map to straight null rays under a conformal transformation and there is a unique canonical isomorphism between null rays in \mathbb{M}^c and points in \mathbb{PN} respecting the conformal group.
In \mathbb{M}^c, it is the case that positive and negative frequency solutions cannot be locally separated. However, this is possible in twistor space.
\mathbb{PT}^+ \simeq \mathrm{SU}(2,2)/\left[ \mathrm{SU}(2,1) \times \mathrm{U}(1) \right]
For many years after Penrose's foundational 1967 paper, twistor theory progressed slowly, in part because of mathematical challenges. Twistor theory also seemed unrelated to ideas in mainstream physics. While twistor theory appeared to say something about quantum gravity, its potential contributions to understanding the other fundamental interactions and particle physics were less obvious.
Witten (2003) proposed a connection between string theory and twistor geometry, called twistor string theory. Witten (2004)^{[2]} built on this insight to propose a way to do string theory in twistor space, whose dimensionality is necessarily the same as that of 3+1 Minkowski spacetime. Although Witten has said that "I think twistor string theory is something that only partly works," his work has given new life to the twistor research program. For example, twistor string theory may simplify calculating scattering amplitudes from Feynman diagrams by using a geometric structure called an amplituhedron.
Witten's twistor string theory is defined on the supertwistor space \mathbb{CP}^{3|4}. Supertwistors are a supersymmetric extension of twistors introduced by Alan Ferber in 1978.^{[4]} Along with the standard twistor degrees of freedom, a supertwistor contains N fermionic scalars, where N is the number of supersymmetries. The superconformal algebra can be realized on supertwistor space.
String theory, Quantum gravity, Carlo Rovelli, Quantum mechanics, Energy
Mathematics, Twistor theory, Roger Penrose, Quantum Gravity, Complex number
Electromagnetism, Energy, Albert Einstein, ArXiv, Quantum gravity
Electromagnetism, Physics, Quantum mechanics, Lagrangian mechanics, Quantum field theory