Low energy description of quantum gravity and complementarity
Autor: | Jaime Varela, Sean J. Weinberg, Yasunori Nomura |
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Přispěvatelé: | Massachusetts Institute of Technology. Center for Theoretical Physics, Massachusetts Institute of Technology. Department of Physics, Massachusetts Institute of Technology. Laboratory for Nuclear Science, Nomura, Yasunori, Varela, Jaime, Weinberg, Sean Jason |
Rok vydání: | 2014 |
Předmět: |
High Energy Physics - Theory
Centers of gravity in non-uniform fields Nuclear and High Energy Physics Observer (quantum physics) FOS: Physical sciences General Relativity and Quantum Cosmology (gr-qc) 01 natural sciences Atomic General Relativity and Quantum Cosmology Gravitation Particle and Plasma Physics Affordable and Clean Energy 0103 physical sciences Nuclear 010306 general physics Mathematical Physics Physics Spacetime 010308 nuclear & particles physics Molecular Nuclear & Particles Physics Classical mechanics High Energy Physics - Theory (hep-th) Gravity well Quantum gravity Proper acceleration Astronomical and Space Sciences Black hole complementarity |
Zdroj: | Nomura, Y; Varela, J; & Weinberg, SJ. (2014). Low energy description of quantum gravity and complementarity. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 733, 126-133. doi: 10.1016/j.physletb.2014.04.027. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/1br3t2d8 Physics Letters B Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, vol 733 TopicHub SCOAP3 |
ISSN: | 0370-2693 |
DOI: | 10.1016/j.physletb.2014.04.027 |
Popis: | We consider a framework in which low energy dynamics of quantum gravity is described preserving locality, and yet taking into account the effects that are not captured by the naive global spacetime picture, e.g. those associated with black hole complementarity. Our framework employs a “special relativistic” description of gravity; specifically, gravity is treated as a force measured by the observer tied to the coordinate system associated with a freely falling local Lorentz frame. We identify, in simple cases, regions of spacetime in which low energy local descriptions are applicable as viewed from the freely falling frame; in particular, we identify a surface called the gravitational observer horizon on which the local proper acceleration measured in the observer's coordinates becomes the cutoff (string) scale. This allows for separating between the “low-energy” local physics and “trans-Planckian” intrinsically quantum gravitational (stringy) physics, and allows for developing physical pictures of the origins of various effects. We explore the structure of the Hilbert space in which the proposed scheme is realized in a simple manner, and classify its elements according to certain horizons they possess. We also discuss implications of our framework on the firewall problem. We conjecture that the complementarity picture may persist due to properties of trans-Planckian physics. United States. Dept. of Energy. Office of High Energy and Nuclear Physics (Contract DE-FG02-05ER41360) United States. Dept. of Energy. Office of High Energy and Nuclear Physics (Contract DE-AC02-05CH11231) National Science Foundation (U.S.) (NSF Grant No. PHY-0855653) National Science Foundation (U.S.) (NSF Grant No. DGE-1106400) Simons Foundation (Grant 230224) |
Databáze: | OpenAIRE |
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