• Corpus ID: 18238231

6-D model with scalar field condensation at brane and zero 4-D Cosmological Constant

@article{Guendelman20056DMW,
  title={6-D model with scalar field condensation at brane and zero 4-D Cosmological Constant},
  author={Eduardo Guendelman},
  journal={arXiv: High Energy Physics - Theory},
  year={2005}
}
  • E. Guendelman
  • Published 10 July 2005
  • Mathematics, Physics
  • arXiv: High Energy Physics - Theory
In a previous publication we have shown that the gauge theory of relativistic 3-Branes can be formulated in a conformally invariant way if the embedding space is six-dimensional. The implementation of conformal invariance requires the use of a modified measure, independent of the metric in the action. We here generalize the theory to include conformal invariance breaking and a dynamical scalar field with a non-trivial potential. The non conformal invariance contribution can be interpreted as… 

References

SHOWING 1-10 OF 32 REFERENCES
The Cosmological Constant Problems
The old cosmological constant problem is to understand why the vacuum energy is so small; the new problem is to understand why it is comparable to the present mass density. Several approaches to
Lecture Notes on Physics
THE author says in his preface that the book “may be supposed to represent the notes, somewhat expanded, which the teacher would desire the class to take down and learn.” If so, the “notes”before us
Phys
  • Rev., D70: 026003
  • 2004
Rev
  • D47, 2536
  • 1993
Model without branes was considered first in E.I. Guendelman Phys. Lett. B412, 42 (1997); coupling to branes was investigated in E
  • I. Guendelman, Phys. Lett.B
  • 2004
Phys. Rev
  • Phys. Rev
  • 2004
Phys. Rev. Phys. Rev
  • Phys. Rev. Phys. Rev
  • 2004
Guica Sidestepping the Cosmological Constant with Football- Shaped Extra Dimensions, hep-th/0302067; I
  • Navarro JCAP
  • 2003
JHEP Nucl.Phys
  • JHEP Nucl.Phys
  • 2003
Applications to the fermion family problem can be found in E. I. Guendelman and A
  • B. Kaganovich Int. J. Mod. Phys. ibid. Mod. Phys. Lett. A17
  • 2002
...
1
2
3
4
...