Export citation

Export citation

Choose format for download:

Download Citation
  • Access by Xinjiang University

Warped gravitons at the CERN LHC and beyond

Kaustubh Agashe1, Hooman Davoudiasl3, Gilad Perez2, and Amarjit Soni3

  • 1Department of Physics, Syracuse University, Syracuse, New York 13244, USA
  • 2C. N. Yang Institute for Theoretical Physics, State University of New York, Stony Brook, New York 11794-3840, USA
  • 3Brookhaven National Laboratory, Upton, New York 11973, USA

Phys. Rev. D 76, 036006 – Published 31 August, 2007

DOI: https://doi.org/10.1103/PhysRevD.76.036006

Abstract

We study the production and decay of Kaluza-Klein (KK) gravitons at the CERN Large Hadron Collider (LHC), in the framework of a warped extra dimension in which the standard model (SM) fields propagate. Such a scenario can provide solutions to both the Planck-weak hierarchy problem and the flavor puzzle of the SM. In this scenario, the production via qq¯ annihilation and decays to the conventional photon and lepton channels are highly suppressed. However, we show that graviton production via gluon fusion followed by decay to longitudinal Z/W can be significant; vector boson fusion is found to be a subdominant production mode. In particular, the golden ZZ decay mode offers a distinctive 4-lepton signal that could lead to the observation at the LHC with 300fb1 (SLHC with 3ab1) of a KK graviton with a mass up to 2 (3) TeV for the ratio of the AdS5 curvature to the Planck scale modestly above unity. We argue that (contrary to the lore) such a size of the curvature scale can still be within the regime of validity of the framework. Upgrades beyond the SLHC luminosity are required to discover gravitons heavier than 4TeV, as favored by the electroweak and flavor precision tests in the simplest such models.

Article Text

References (31)

  1. L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 3370 (1999).
  2. N. Arkani-Hamed, S. Dimopoulos, and G. R. Dvali, Phys. Lett. B 429, 263 (1998); I. Antoniadis, N. Arkani-Hamed, S. Dimopoulos, and G. R. Dvali, 436, 257 (1998); N. Arkani-Hamed, S. Dimopoulos, and G. R. Dvali, Phys. Rev. D 59, 086004 (1999).
  3. J. M. Maldacena, Adv. Theor. Math. Phys. 2, 231 (1998); Int. J. Theor. Phys. 38, 1113 (1999); S. S. Gubser, I. R. Klebanov, and A. M. Polyakov, Phys. Lett. B 428, 105 (1998); E. Witten, Adv. Theor. Math. Phys. 2, 253 (1998).
  4. N. Arkani-Hamed, M. Porrati, and L. Randall, J. High Energy Phys. 08 (2001) 017; R. Rattazzi and A. Zaffaroni, 04 (2001) 021.
  5. R. Contino, Y. Nomura, and A. Pomarol, Nucl. Phys. B671, 148 (2003); K. Agashe, R. Contino, and A. Pomarol, B719, 165 (2005).
  6. H. Davoudiasl, J. L. Hewett, and T. G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000).
  7. H. Davoudiasl, J. L. Hewett, and T. G. Rizzo, Phys. Lett. B 473, 43 (2000); A. Pomarol, 486, 153 (2000).
  8. Y. Grossman and M. Neubert, Phys. Lett. B 474, 361 (2000).
  9. S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, Phys. Rev. D 62, 084025 (2000).
  10. T. Gherghetta and A. Pomarol, Nucl. Phys. B586, 141 (2000).
  11. S. J. Huber and Q. Shafi, Phys. Lett. B 498, 256 (2001).
  12. H. Davoudiasl, J. L. Hewett, and T. G. Rizzo, Phys. Rev. D 63, 075004 (2001).
  13. H. Davoudiasl T. G. Rizzoand , Phys. Lett. B 512, 100 (2001).
  14. H. Davoudiasl, J. L. Hewett, B. Lillie, and T. G. Rizzo, Phys. Rev. D 70, 015006 (2004).
  15. K. Agashe, G. Perez, and A. Soni, Phys. Rev. Lett. 93, 201804 (2004); Phys. Rev. D 71, 016002 (2005).
  16. K. Agashe et al., J. High Energy Phys. 08 (2003) 050.
  17. K. Agashe, M. Papucci, G. Perez, and D. Pirjol, arXiv:hep-ph/0509117; Z. Ligeti, M. Papucci, and G. Perez, Phys. Rev. Lett. 97, 101801 (2006).
  18. K. Agashe et al., Phys. Lett. B 641, 62 (2006).
  19. M. Carena, E. Ponton, J. Santiago, and C. E. M. Wagner, Nucl. Phys. B759, 202 (2006); arXiv:hep-ph/0701055.
  20. T. Han, J. D. Lykken, and R. J. Zhang, Phys. Rev. D 59, 105006 (1999).
  21. S. C. Park, H. S. Song, and J. H. Song, Phys. Rev. D 65, 075008 (2002).
  22. See, for example, T. Han, arXiv:hep-ph/0508097 and references therein.
  23. See for example E. Eichten, I. Hinchliffe, K. D. Lane, and C. Quigg, Rev. Mod. Phys. 56, 579 (1984); 58, 1065(A) (1986) and references therein.
  24. J. E. Huth et al., Proceedings of Research Directions For The Decade: Snowmass Accord, 1990, edited by E. L. Berger (World Scientific, Singapore, 1992).
  25. Z. Chacko, M. A. Luty, and E. Ponton, J. High Energy Phys. 07 (2000) 036.
  26. K. Agashe, A. Belyaev, T. Krupovnickas, G. Perez, and J. Virzi, arXiv:hep-ph/0612015.
  27. F. Hubaut, E. Monnier, P. Pralavorio, K. Smolek, and V. Simak, Eur. Phys. J. C 44S2, 13 (2005); M. Baarmand, H. Mermerkaya, and I. Vodopianov, Report No. CERN-CMS-NOTE-2006-111.
  28. F. Gianotti et al., Eur. Phys. J. C 39, 293 (2005).
  29. O. Bruning et al., Report No. CERN-LHC-PROJECT-REPORT-626.
  30. J. Hirn and V. Sanz, Phys. Rev. Lett. 97, 121803 (2006); J. High Energy Phys. 03 (2007) 100.
  31. A. L. Fitzpatrick, J. Kaplan, L. Randall, and L. T. Wang, arXiv:hep-ph/0701150.

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation