Published November 15, 2006 | Version v1
Journal article

Higher-dimensional bulk wormholes and their manifestations in brane worlds

  • 1. Department of General Studies, Charles Drew University, Los Angeles, California 90059 (United States)

Description

There is nothing to prevent a higher-dimensional anti-de Sitter bulk spacetime from containing various other branes in addition to hosting our universe, presumed to be a positive-tension 3-brane. In particular, it could contain closed, microscopic branes that form the boundary surfaces of void bubbles and thus violate the null energy condition in the bulk. The possible existence of such micro branes can be investigated by considering the properties of the ground state of a pseudo-Wheeler-DeWitt equation describing brane quantum dynamics in minisuperspace. If they exist, a concentration of these micro branes could act as a fluid of exotic matter able to support macroscopic wormholes connecting otherwise-distant regions of the bulk. Were the brane constituting our universe to expand into a region of the bulk containing such higher-dimensional macroscopic wormholes, they would likely manifest themselves in our brane as wormholes of normal dimensionality, whose spontaneous appearance and general dynamics would seem inexplicably peculiar. This encounter could also result in the formation of baby universes of a particular type

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
74
Journal Issue
10
Journal Page Range
p. 104025-104025.11
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
38032703
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Descriptors DEI
COSMOLOGY; DE SITTER GROUP; FIELD EQUATIONS; GROUND STATES; MEMBRANES; QUANTUM FIELD THEORY; SPACE-TIME; UNIVERSE
Descriptors DEC
ENERGY LEVELS; EQUATIONS; FIELD THEORIES; LIE GROUPS; SYMMETRY GROUPS

Optional Information

Notes
(c) 2006 The American Physical Society