TY - JOUR
T1 - Spherically symmetric and rotating wormholes produced by lightlike branes
AU - Guendelman, Eduardo
AU - Kaganovich, Alexander
AU - Nissimov, Emil
AU - Pacheva, Svetlana
N1 - Funding Information:
We are very grateful to Werner Israel and Eric Poisson for useful and illuminating correspondence. E. Nissimov and S. Pacheva are supported by Bulgarian NSF grant DO 02-257. Also, all of us acknowledge support of our collaboration through the exchange agreement between the Ben-Gurion University of the Negev (Beer-Sheva, Israel) and the Bulgarian Academy of Sciences.
PY - 2010/3/20
Y1 - 2010/3/20
N2 - Lightlike p-branes (LL-branes) with dynamical (variable) tension allow simple and elegant Polyakov-type and dual to it NambuGoto-like worldvolume action formulations. Here we first briefly describe the dynamics of LL-branes as test objects in various physically interesting gravitational backgrounds of black hole type, including rotating ones. Next we show that LL-branes are the appropriate gravitational sources that provide proper matter energymomentum tensors in the Einstein equations of motion needed to generate traversable wormhole solutions, in particular, self-consistent cylindrical rotating wormholes, with the LL-branes occupying their throats. Here a major role is being played by the dynamical LL-brane tension which turns out to be negative but may be of arbitrary small magnitude. As a particular solution we obtain traversable wormhole with Schwarzschild geometry generated by a LL-brane positioned at the wormhole throat, which represents the correct consistent realization of the original EinsteinRosen "bridge" manifold.
AB - Lightlike p-branes (LL-branes) with dynamical (variable) tension allow simple and elegant Polyakov-type and dual to it NambuGoto-like worldvolume action formulations. Here we first briefly describe the dynamics of LL-branes as test objects in various physically interesting gravitational backgrounds of black hole type, including rotating ones. Next we show that LL-branes are the appropriate gravitational sources that provide proper matter energymomentum tensors in the Einstein equations of motion needed to generate traversable wormhole solutions, in particular, self-consistent cylindrical rotating wormholes, with the LL-branes occupying their throats. Here a major role is being played by the dynamical LL-brane tension which turns out to be negative but may be of arbitrary small magnitude. As a particular solution we obtain traversable wormhole with Schwarzschild geometry generated by a LL-brane positioned at the wormhole throat, which represents the correct consistent realization of the original EinsteinRosen "bridge" manifold.
KW - Black hole's horizon "straddling"
KW - Dynamical brane tension
KW - Non-NambuGoto lightlike branes
KW - Traversable wormholes
UR - http://www.scopus.com/inward/record.url?scp=77951669063&partnerID=8YFLogxK
U2 - 10.1142/S0217751X10047762
DO - 10.1142/S0217751X10047762
M3 - Article
AN - SCOPUS:77951669063
SN - 0217-751X
VL - 25
SP - 1405
EP - 1428
JO - International Journal of Modern Physics A
JF - International Journal of Modern Physics A
IS - 7
ER -