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Anisotropic type I string compactification, winding modes and large extra dimensions. (English) Zbl 0947.81565

Summary: We discuss the structure of general anisotropic compactification in type I \(D=4, N=1\) string theory. It is emphasized that, in this context, a possible interpretation of \(M_{\text{Planck}}\) as “dual” to (at least) one of the Kaluza-Klein or windings modes could provide interesting interpretations of the “physical scales” and the GUT coupling. Some of the scenarios presented here are strictly connected with the phenomenological proposal of TeV-scale gravity (i.e. millimeter compactification). We show that in this scenario new and probably dominant effects should arise from the presence of “low-energy” winding modes of usual SM particles. Stringent bounds on the Planck mass in \(4+n\) dimensions are derived from the existing experimental limits on massive replicas of SM gauge bosons. Non-observation of winding modes at the planned accelerators could provide stronger bounds on the \(4+n\)-dimensional Planck mass than those from graviton emission into the bulk. Some comments on other possible phenomenological interesting scenarios are addressed.

MSC:

81V22 Unified quantum theories
81T13 Yang-Mills and other gauge theories in quantum field theory
81V17 Gravitational interaction in quantum theory

References:

[1] Dienes, K., Phys. Rep., 287, 447 (1997)
[2] Witten, E., Nucl. Phys. B, 471, 135 (1996) · Zbl 1003.81536
[3] Polchinski, J.; Witten, E., Nucl. Phys. B, 460, 525 (1996) · Zbl 1004.81526
[4] Horawa, P.; Witten, E., Nucl. Phys. B, 460, 506 (1996) · Zbl 1004.81525
[5] C. Burgess, L. Ibáñez and F. Quevedo, hep-ph/9810535.; C. Burgess, L. Ibáñez and F. Quevedo, hep-ph/9810535.
[6] Lykken, J. D., Phys. Rev. D, 54, 3693 (1996)
[7] Arkani-Hamed, N.; Dimopoulos, S.; Dvali, G., Phys. Lett. B, 429, 263 (1998) · Zbl 1355.81103
[8] N. Arkani-Hamed, S. Dimopoulos and G. Dvali, hep-ph/9807344.; N. Arkani-Hamed, S. Dimopoulos and G. Dvali, hep-ph/9807344.
[9] Shiu, G.; Tye, S.-H. H., Phys. Rev. D, 58, 106007 (1998)
[10] G. Giudice, R. Rattazzi and J. Wells, hep-ph/9811291; E.A. Mirabelli, M. Perelstein and M.E. Peskin, hep-ph/9811337; T. Han, J.D. Lykken and R.J. Zhang, hep-ph/9811350.; G. Giudice, R. Rattazzi and J. Wells, hep-ph/9811291; E.A. Mirabelli, M. Perelstein and M.E. Peskin, hep-ph/9811337; T. Han, J.D. Lykken and R.J. Zhang, hep-ph/9811350.
[11] For a review see J. Polchinski, hep-th/9611050; C.P. Bachas, hep-th/9806199.; For a review see J. Polchinski, hep-th/9611050; C.P. Bachas, hep-th/9806199.
[12] Lykken, J., (Nucl. Phys. B (Proc. Suppl.), 52 A (1997)), 271 · Zbl 0957.81618
[13] Z. Kakushadze and S.-H.H. Tye, hep-th/9512155; G. Aldazabal, hep-th/9507162; L. Ibáñez, hep-th/9505098.; Z. Kakushadze and S.-H.H. Tye, hep-th/9512155; G. Aldazabal, hep-th/9507162; L. Ibáñez, hep-th/9505098.
[14] L. Ibáñez, C. Muñoz and S. Rigolin, hep-th/9812397.; L. Ibáñez, C. Muñoz and S. Rigolin, hep-th/9812397.
[15] N. Arkani-Hamed, S. Dimopoulos and J. March-Russell, hep-th/9809124; K.R. Dienes, E. Dudas, A. Ghorghetta and A. Riotto, hep-ph/9809406; D. Lyth, hep-ph/9810320; N. Kaloper and A. Linde, hep-th/9811141; G. Dvali and S.-H.H. Tye, hep-ph/9812483.; N. Arkani-Hamed, S. Dimopoulos and J. March-Russell, hep-th/9809124; K.R. Dienes, E. Dudas, A. Ghorghetta and A. Riotto, hep-ph/9809406; D. Lyth, hep-ph/9810320; N. Kaloper and A. Linde, hep-th/9811141; G. Dvali and S.-H.H. Tye, hep-ph/9812483.
[16] Z. Kakushadze and S.-H.H. Tye, hep-th/9809147; K. Benakli, hep-ph/9809582; M. Maggiore and A. Riotto, hep-th/9811089; S. Nussinov and R. Shrock, hep-ph/9811323; N. Arkani-Hamed and S. Dimopoulos, hep-ph/9811353; J. Hewett, hep-ph/9811356; Z. Berezhiani and G. Dvali, hep-ph/9811378; K.R. Dienes, E. Dudas and A. Gherghetta, hep-ph/9811428; N. Arkani-Hamed, S. Dimopoulos and J. March-Russell, hep-ph/9811448; P. Mathews, S. Raychaudhuri and K. Sridhar, hep-ph/9811501; hep-ph/9812486; Z. Kakushadze, hep-th/9812163; A.E. Faraggi and M. Pospelov, hep-ph/9901299.; Z. Kakushadze and S.-H.H. Tye, hep-th/9809147; K. Benakli, hep-ph/9809582; M. Maggiore and A. Riotto, hep-th/9811089; S. Nussinov and R. Shrock, hep-ph/9811323; N. Arkani-Hamed and S. Dimopoulos, hep-ph/9811353; J. Hewett, hep-ph/9811356; Z. Berezhiani and G. Dvali, hep-ph/9811378; K.R. Dienes, E. Dudas and A. Gherghetta, hep-ph/9811428; N. Arkani-Hamed, S. Dimopoulos and J. March-Russell, hep-ph/9811448; P. Mathews, S. Raychaudhuri and K. Sridhar, hep-ph/9811501; hep-ph/9812486; Z. Kakushadze, hep-th/9812163; A.E. Faraggi and M. Pospelov, hep-ph/9901299.
[17] Caceres, E.; Kaplunovsky, V. S.; Mandelberg, I. M., Nucl. Phys. B, 493, 73 (1997) · Zbl 1004.81546
[18] Dienes, K. R.; Dudas, E.; Gherghetta, A., Nucl. Phys. B, 537, 47 (1999) · Zbl 0948.81660
[19] S. Abel and S. King, hep-ph/9809467.; S. Abel and S. King, hep-ph/9809467.
[20] Ghilencea, G.; Ross, G. G., Phys. Lett. B, 442, 165 (1998) · Zbl 1002.81568
[21] T. Kobayashi, J. Kubo, M. Mondragon and G. Zoupanos, hep-ph/9812221.; T. Kobayashi, J. Kubo, M. Mondragon and G. Zoupanos, hep-ph/9812221.
[22] Brignole, A.; Feruglio, F.; Zwirner, F., Phys. Lett. B, 438, 89 (1998)
[23] I. Antoniadis, S. Dimopoulos, A. Pomarol and M. Quirós, hep-ph/9810410; A. Delgado, A. Pomarol and M. Quirós, hep-ph/9812489.; I. Antoniadis, S. Dimopoulos, A. Pomarol and M. Quirós, hep-ph/9810410; A. Delgado, A. Pomarol and M. Quirós, hep-ph/9812489.
[24] Antoniadis, I.; Benakli, K.; Quirós, M., Phys. Lett. B, 331, 313 (1994)
[25] Long, J. C.; Chan, H. W.; Price, J. C., Nucl. Phys. B, 539, 23 (1999)
[26] Abe, F., Phys. Rev. Lett., 79, 2192 (1997)
[27] Leike, A.; Riemann, S., Z. Phys. C, 75, 341 (1997), See, for example
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