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Higgs inflation on braneworld. (English) Zbl 1284.83220

Summary: We discuss a Higgs inflation model in the warped DGP braneworld background. It generates reasonable primordial perturbations. At the same time, with enhanced nonminimal coupling, it overcomes the severe problem in the Higgs inflation in four dimensions, which says that the effective field theory becomes invalid at an energy scale far below the energy scale for inflation exit. Furthermore, we present the constraints for the parameters confronted to PLANCK and related observations. PLANCK low-l data almost fixes the inflation energy scale in this Higgs inflation model with specific brane parameters.

MSC:

83F05 Relativistic cosmology
81T30 String and superstring theories; other extended objects (e.g., branes) in quantum field theory
81V22 Unified quantum theories

References:

[1] DOI: 10.1016/j.physletb.2012.08.020 · doi:10.1016/j.physletb.2012.08.020
[2] DOI: 10.1016/j.physletb.2012.08.021 · doi:10.1016/j.physletb.2012.08.021
[3] DOI: 10.1016/j.physletb.2007.11.072 · doi:10.1016/j.physletb.2007.11.072
[4] DOI: 10.1088/1475-7516/2008/11/021 · doi:10.1088/1475-7516/2008/11/021
[5] DOI: 10.1016/j.physletb.2009.05.054 · doi:10.1016/j.physletb.2009.05.054
[6] DOI: 10.1088/0264-9381/30/21/214001 · Zbl 1277.83003 · doi:10.1088/0264-9381/30/21/214001
[7] DOI: 10.1007/JHEP01(2011)016 · Zbl 1214.83051 · doi:10.1007/JHEP01(2011)016
[8] DOI: 10.1088/1126-6708/2009/09/103 · doi:10.1088/1126-6708/2009/09/103
[9] DOI: 10.1103/PhysRevD.79.081302 · doi:10.1103/PhysRevD.79.081302
[10] DOI: 10.1007/JHEP07(2010)007 · Zbl 1290.81198 · doi:10.1007/JHEP07(2010)007
[11] DOI: 10.1007/JHEP11(2010)023 · Zbl 1294.81348 · doi:10.1007/JHEP11(2010)023
[12] DOI: 10.1016/j.physletb.2011.01.028 · doi:10.1016/j.physletb.2011.01.028
[13] DOI: 10.1016/0550-3213(95)00621-4 · Zbl 1004.81525 · doi:10.1016/0550-3213(95)00621-4
[14] DOI: 10.1103/PhysRevD.63.065007 · doi:10.1103/PhysRevD.63.065007
[15] DOI: 10.1016/S0370-2693(01)00160-5 · Zbl 0977.83103 · doi:10.1016/S0370-2693(01)00160-5
[16] DOI: 10.1103/PhysRevD.65.044023 · doi:10.1103/PhysRevD.65.044023
[17] DOI: 10.1103/PhysRevD.66.024019 · doi:10.1103/PhysRevD.66.024019
[18] DOI: 10.1103/PhysRevD.66.024019 · doi:10.1103/PhysRevD.66.024019
[19] DOI: 10.1016/S0370-2693(01)00236-2 · Zbl 0977.83110 · doi:10.1016/S0370-2693(01)00236-2
[20] DOI: 10.1088/1126-6708/2004/03/038 · doi:10.1088/1126-6708/2004/03/038
[21] DOI: 10.1088/1475-7516/2004/08/017 · doi:10.1088/1475-7516/2004/08/017
[22] DOI: 10.1016/j.physletb.2006.07.055 · Zbl 1248.83125 · doi:10.1016/j.physletb.2006.07.055
[23] DOI: 10.1103/PhysRevD.86.043505 · doi:10.1103/PhysRevD.86.043505
[24] DOI: 10.1007/s10509-012-0980-2 · Zbl 1255.83162 · doi:10.1007/s10509-012-0980-2
[25] DOI: 10.1088/1475-7516/2007/11/006 · doi:10.1088/1475-7516/2007/11/006
[26] DOI: 10.1007/JHEP05(2012)108 · Zbl 1348.81377 · doi:10.1007/JHEP05(2012)108
[27] DOI: 10.1142/S0217732399001103 · doi:10.1142/S0217732399001103
[28] DOI: 10.1007/JHEP06(2011)043 · Zbl 1298.83023 · doi:10.1007/JHEP06(2011)043
[29] DOI: 10.1088/0264-9381/21/15/N02 · Zbl 1070.83023 · doi:10.1088/0264-9381/21/15/N02
[30] DOI: 10.1103/PhysRevD.71.063536 · doi:10.1103/PhysRevD.71.063536
[31] DOI: 10.1016/S0370-2693(99)00051-9 · doi:10.1016/S0370-2693(99)00051-9
[32] van der Bij J. J., Acta Phys. Pol. B 25 pp 827– (1994)
[33] DOI: 10.1016/0550-3213(95)00128-X · doi:10.1016/0550-3213(95)00128-X
[34] van der Bij J. J., Int. J. Phys. 1 pp 63– (1995)
[35] DOI: 10.1016/0370-2693(94)91292-0 · doi:10.1016/0370-2693(94)91292-0
[36] DOI: 10.1103/PhysRevD.52.4295 · doi:10.1103/PhysRevD.52.4295
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