Abstract
We regard an ultrarelativistic hadron moving on a brane embedded in a higher-dimensional space-time as a membrane propagating on a three-brane. For hadron sizes exceeding the compactification radius and characteristic scales of five-dimensional gravitational interaction, this membrane can be regarded as a cosmic membrane in the sense that it extends to the infinities. In the five-dimensional case, a cosmic membrane produces a topological defect similar to the defect produced by a cosmic string in the four-dimensional space-time. This representation allows calculating the effects of the influence of the hadron mass on the gravitational interaction of partons belonging to the colliding hadrons.
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Translated from Teoreticheskaya i Matematicheskaya Fizika, Vol. 166, No. 3, pp. 443–451, March, 2011.
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Aref’eva, I.Y. Ultrarelativistic hadrons as cosmic membranes in TeV-gravity models. Theor Math Phys 166, 385–391 (2011). https://doi.org/10.1007/s11232-011-0030-1
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DOI: https://doi.org/10.1007/s11232-011-0030-1