Can the effective string see higher partial waves

The semiclassical cross sections for arbitrary partial waves of ordinary scalars to fall into certain five-dimensional black holes have a form that seems capable of explanation in terms of the effective string model. The kinematics of these processes is analyzed in detail on the effective string and is shown to reproduce the correct functional form of the semiclassical cross sections. But it is necessary to choose a peculiar value of the effective string tension to obtain the correct scaling properties. Furthermore, the assumptions of locality and statistics combine to forbid the effective string from absorbing more than a finite number of partial waves. The relation of this limitation to cosmic censorship is discussed. {copyright} {ital 1997} {ital The American Physical Society}

• Publication year

  1997

• Venue

  Physical Review D

• Publication date

  1997-04-27

• Fields of study

  Physics

• Identifiers
  DOI 10.1103/PhysRevD.56.4984arXiv hep-th/9704195
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  Open on Semantic Scholar

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  Semantic Scholar

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• No concepts are published for this paper.

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