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PhysicsInTheLHCEra.pdf

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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/4131 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/4131 http://eprints.org/relation/ismediumThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/4131 4136 2 11574 document 4136 small.jpg image/png e7a4f6cb3fb17c60cd3f29016feff5ab MD5 1312 2014-02-12 06:06:40 http://eprints.iliauni.edu.ge/968/6/small.jpg 968 6 6 image/png other Thumbnails conversion from text to thumbnail_small ge public

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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/4131 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/4131 http://eprints.org/relation/issmallThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/4131 archive 109 disk0/00/00/09/68 2014-02-12 06:16:46 2015-03-30 08:32:25 2014-02-12 06:16:46 conference_item show Midodashvili Pavle Gogberashvili Merab pub Q1 QC ins14 public paper We introduce the new 5D braneworld with the real scalar field in the bulk. The model represents the brane which bounds collective oscillations of standing gravitational and scalar fields waves in the bulk. These waves are out of phase, i.e. the energy of oscillations passes back and forth between the scalar and gravitational waves. We investigate two limiting cases depending on the values of the width of the brane and of the size of the horizon in extra space. When the amplitude of the standing waves is small these sizes coincide. In the case of large oscillations it is shown that the mass of the lightest KK mode is determined by the smaller scale, which corresponds to the horizon size. So KK modes can be born in accelerators at relatively low energies, what gives a chance to check the present model. 2013-10 published 167-172 Physics in the LHC era Georgia, Tbilisi 14-18 October 2013 conference TRUE