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TMF, 2011, Volume 166, Number 3, Pages 443–451 (Mi tmf6621)  

Ultrarelativistic hadrons as cosmic membranes in $TeV$-gravity models

I. Ya. Aref'eva

Steklov Mathematical Institute, Russian Academy of Sciences, Moscow, Russia

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.

Keywords: cosmic membrane, TeV gravity, higher dimension

DOI: https://doi.org/10.4213/tmf6621

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English version:
Theoretical and Mathematical Physics, 2011, 166:3, 385–391

Bibliographic databases:

Document Type: Article
Received: 06.09.2010

Citation: I. Ya. Aref'eva, “Ultrarelativistic hadrons as cosmic membranes in $TeV$-gravity models”, TMF, 166:3 (2011), 443–451; Theoret. and Math. Phys., 166:3 (2011), 385–391

Citation in format AMSBIB
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