A Chiral Perturbation Expansion for Gravity
arXiv:hep-th/0511189 · doi:10.1088/1126-6708/2006/02/057
Abstract
A formulation of Einstein gravity, analogous to that for gauge theory arising from the Chalmers-Siegel action, leads to a perturbation theory about an asymmetric weak coupling limit that treats positive and negative helicities differently. We find power counting rules for amplitudes that suggest the theory could find a natural interpretation in terms of a twistor-string theory for gravity with amplitudes supported on holomorphic curves in twistor space.
11 pages, LaTeX, no figures; v2: one reference added
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Cited by in corpus (10)
- Gravity, Twistors and the MHV Formalism
- Actions for Self-dual Higher Spin Gravities
- Twistor Actions for Self-Dual Supergravities
- Chiral approach to massive higher spins
- Superspace formulations of the (super)twistor string
- Gauge independent kinematic algebra of self-dual Yang-Mills theory
- Flat Self-dual Gravity
- Minimal models of field theories: Chiral Higher Spin Gravity
- Einstein Supergravity and New Twistor String Theories
- Minimal models of field theories: SDYM and SDGR