Moduli stabilization with F-term uplifting in heterotic string theory

@article{Jeong2008ModuliSW,
  title={Moduli stabilization with F-term uplifting in heterotic string theory},
  author={Kwang Sik Jeong and Seodong Shin},
  journal={Physical Review D},
  year={2008},
  volume={79},
  pages={046001}
}
We discuss the role of F-term uplifting in stabilizing moduli within the framework of heterotic string theory. It turns out that the uplifting sector plays an important role in fixing the volume modulus at one of the self-dual points of a modular invariant potential. For the volume modulus stabilized at a self-dual point, the F-term uplifting leads to the dilation stabilization which can naturally yield the mirage mediation pattern of soft supersymmetry breaking terms. Generalizing to the case… 

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References

SHOWING 1-10 OF 13 REFERENCES

Phys

  • Rev. D 77, 106007
  • 2008

JHEP 0608

  • 007
  • 2006

JHEP 0411

  • 076 (2004) [arXiv:hep-th/0411066]; K. Choi, A. Falkowski, H. P. Nilles and M. Olechowski, Nucl. Phys. B 718, 113
  • 2005

Phys

  • Lett. B 642, 404 (2006) [arXiv:hep-th/0606104]; H. Abe, T. Higaki and T. Kobayashi, Phys. Rev. D 76, 105003 (2007) [arXiv:0707.2671 [hep-th]]; K. S. Jeong, Mod. Phys. Lett. A 23, 1981
  • 2008

Nucl

  • Phys. B 382, 305 (1992) [arXiv:hep-th/9202046]; M. K. Gaillard and B. D. Nelson, Int. J. Mod. Phys. A 22, 1451
  • 2007

Phys

  • Lett. B 245, 401
  • 1990

Phys

  • Lett. B 193, 37 (1987); J. A. Casas, Z. Lalak, C. Munoz and G. G. Ross, Nucl. Phys. B 347, 243
  • 1990

Phys

  • Lett. B 225, 363 (1989); S. Ferrara, D. Lust and S. Theisen, Phys. Lett. B 233, 147
  • 1989

Nucl

  • Phys. B 557, 79 (1999) [arXiv:hep-th/9810155]; G. F. Giudice, M. A. Luty, H. Murayama and R. Rattazzi, JHEP 9812, 027
  • 1998

JHEP 0704

  • 006
  • 2007