Spherical membranes in Matrix theory

dc.creatorKabat, Daniel
dc.creatorTaylor, Washington
dc.date1997-11-11
dc.date1998-01-31
dc.date.accessioned2026-07-07T11:36:08Z
dc.date.available2026-07-07T11:36:08Z
dc.descriptionWe consider membranes of spherical topology in uncompactified Matrix theory. In general for large membranes Matrix theory reproduces the classical membrane dynamics up to 1/N corrections; for certain simple membrane configurations, the equations of motion agree exactly at finite N. We derive a general formula for the one-loop Matrix potential between two finite-sized objects at large separations. Applied to a graviton interacting with a round spherical membrane, we show that the Matrix potential agrees with the naive supergravity potential for large N, but differs at subleading orders in N. The result is quite general: we prove a pair of theorems showing that for large N, after removing the effects of gravitational radiation, the one-loop potential between classical Matrix configurations agrees with the long-distance potential expected from supergravity. As a spherical membrane shrinks, it eventually becomes a black hole. This provides a natural framework to study Schwarzschild black holes in Matrix theory.
dc.description21 pages LaTeX. V2: references added; V3: reference added, minor corrections
dc.identifierhttps://arxiv.org/abs/hep-th/9711078
dc.identifierhttp://arxiv.org/abs/hep-th/9711078
dc.identifierAdv.Theor.Math.Phys.2:181-206,1998
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198819
dc.subjectHigh Energy Physics - Theory
dc.titleSpherical membranes in Matrix theory
dc.typetext

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