String Theory at Short Distance and the Principle of Equivalence

Point particles fall freely along geodesics; strings do not. In string theory all probes of spacetime structure, including photons, are extended objects and therefore always subject to tidal forces. We illustrate how string theory modifies the behavior of light in weak gravitational fields and limit...

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description Point particles fall freely along geodesics; strings do not. In string theory all probes of spacetime structure, including photons, are extended objects and therefore always subject to tidal forces. We illustrate how string theory modifies the behavior of light in weak gravitational fields and limits the applicability of the principle of equivalence. This gives in principle a window on the short-distance structure of geometry in quantum gravity where one can see in a model-independent way how some of its predictions differ from those of classical gravity. We compare this with the lessons of high-energy string scattering.
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subjects Physics - Astrophysics of Galaxies
Physics - Cosmology and Nongalactic Astrophysics
Physics - Earth and Planetary Astrophysics
Physics - General Relativity and Quantum Cosmology
Physics - High Energy Astrophysical Phenomena
Physics - High Energy Physics - Theory
Physics - Instrumentation and Methods for Astrophysics
Physics - Solar and Stellar Astrophysics
title String Theory at Short Distance and the Principle of Equivalence
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