Holographic Space-Time: The Takeaway
arXiv:1109.2435
Abstract
The theory of holographic space-time (HST) generalizes both string theory and quantum field theory. It provides a geometric rationale for supersymmetry (SUSY) and a formalism in which super-Poincare invariance follows from Poincare invariance. HST unifies particles and black holes, realizing both as excitations of non-commutative geometrical variables on a holographic screen. Compact extra dimensions are interpreted as finite dimensional unitary representations of super-algebras, and have no moduli. Full field theoretic Fock spaces, and continuous moduli are both emergent phenomena of super-Poincare invariant limits in which the number of holographic degrees of freedom goes to infinity. Finite radius de Sitter (dS) spaces have no moduli, and break SUSY with a gravitino mass scaling like . We present a holographic theory of inflation and fluctuations. The inflaton field is an emergent concept, describing the geometry of an underlying HST model, rather than "a field associated with a microscopic string theory". We argue that the phrase in quotes is meaningless in the HST formalism.
19 pages, LaTeX
References in corpus (6)
- Local bulk S-matrix elements and CFT singularities
- Towards a quantum theory of de Sitter space
- Lessons from Classical Gravity about the Quantum Structure of Spacetime
- Entropy density of spacetime and the Navier-Stokes fluid dynamics of null surfaces
- Some Thoughts on the Quantum Theory of Stable de Sitter Space
- Entropy density of spacetime and thermodynamic interpretation of field equations of gravity in any diffeomorphism invariant theory
Cited by in corpus (36)
- Emergent Gravity and the Dark Universe
- Space from Hilbert Space: Recovering Geometry from Bulk Entanglement
- Black holes, quantum information, and unitary evolution
- Complementarity Is Not Enough
- Nonviolent nonlocality
- Nonviolent information transfer from black holes: a field theory parameterization
- Quantum Mereology: Factorizing Hilbert Space into Subsystems with Quasi-Classical Dynamics
- Quantum information transfer and models for black hole mechanics
- The Holographic Space-Time Model of Cosmology
- Modulated Hawking radiation and a nonviolent channel for information release
- Fluctuation and dissipation in de Sitter space
- Holographic Space-Time Does Not Predict Firewalls
- Effective field theory models for nonviolent information transfer from black holes
- Interferometric Tests of Planckian Quantum Geometry Models
- Modular discretization of the AdS2/CFT1 Holography
- Holographic Space-time and Black Holes: Mirages As Alternate Reality
- Holographic Theory of Accelerated Observers, the S-matrix, and the Emergence of Effective Field Theory
- Holographic Theories of Inflation and Fluctuations
- Holographic Space-time and Newton's Law
- Supersymmetry Breaking and the Cosmological Constant
- Instantons, Twistors, and Emergent Gravity
- Holographic Space-time, Newton's Law and the Dynamics of Black Holes
- Holographic Fluctuations from Unitary de Sitter Invariant Field Theory
- Complementarity, not Firewalls
- Statistical Measures of Planck Scale Signal Correlations in Interferometers
- Emergent Gravity in a Holographic Universe
- Angular correlations of causally-coherent primordial quantum perturbations
- Holographic Space-time Models in Dimensions
- Microscopic Models of Linear Dilaton Gravity and Their Semi-classical Approximations
- Why The Cosmological Constant is a Boundary Condition
- Holographic Space-time Models of Anti-deSitter Space-times
- Soft Gravitons and the Flat Space Limit of Anti-deSitter Space
- Update on the Pyramid Scheme
- Deformed Bubbles and Lorentz Invariance in Vacuum Decay
- Note on Localized Objects as Constrained States of Holographic Variables
- The Gravitational Memory of a Galaxy