One residue to rule them all: Electroweak symmetry breaking, inflation and field-space geometry

  1. Karananas, Georgios K.
  2. Michel, Marco
  3. Rubio Peña, Javier 1
  1. 1 Universidad Complutense de Madrid
    info

    Universidad Complutense de Madrid

    Madrid, España

    ROR 02p0gd045

Revista:
Physics Letters B

ISSN: 0370-2693 1873-2445

Año de publicación: 2020

Volumen: 811

Páginas: 135876

Tipo: Artículo

DOI: 10.1016/J.PHYSLETB.2020.135876 GOOGLE SCHOLAR lock_openAcceso abierto editor

Otras publicaciones en: Physics Letters B

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Referencias bibliográficas

  • Senjanović, (2020), Mod. Phys. Lett. A, 35, 10.1142/S0217732320300062
  • Feng, (2013), Annu. Rev. Nucl. Part. Sci., 63, pp. 351, 10.1146/annurev-nucl-102010-130447
  • Bellazzini, (2014), Eur. Phys. J. C, 74, pp. 2766, 10.1140/epjc/s10052-014-2766-x
  • Arkani-Hamed, (1998), Phys. Lett. B, 429, pp. 263, 10.1016/S0370-2693(98)00466-3
  • Dvali, (2004), Phys. Rev. D, 70, 10.1103/PhysRevD.70.063501
  • Dvali, (2006), Phys. Rev. D, 74
  • Dvali
  • Michel, (2020), Phys. Rev. D, 101
  • Graham, (2015), Phys. Rev. Lett., 115, 10.1103/PhysRevLett.115.221801
  • Kaplan, (2016), Phys. Rev. D, 93, 10.1103/PhysRevD.93.085007
  • Vissani, (1998), Phys. Rev. D, 57, pp. 7027, 10.1103/PhysRevD.57.7027
  • Shaposhnikov, (2007)
  • Shaposhnikov, (2009), Phys. Lett. B, 671, pp. 162, 10.1016/j.physletb.2008.11.041
  • Farina, (2013), J. High Energy Phys., 08
  • Karananas, (2017), Phys. Lett. B, 771, pp. 332, 10.1016/j.physletb.2017.05.065
  • Shaposhnikov, (2019), Phys. Rev. D, 99, 10.1103/PhysRevD.99.103528
  • Wetterich, (2012), Phys. Lett. B, 718, pp. 573, 10.1016/j.physletb.2012.11.020
  • Wetterich, (2017), Phys. Lett. B, 770, pp. 268, 10.1016/j.physletb.2017.04.049
  • Dvali
  • Dvali, (2011), Phys. Rev. D, 84, 10.1103/PhysRevD.84.024039
  • Shaposhnikov, (2018), Phys. Lett. B, 783, pp. 253, 10.1016/j.physletb.2018.06.068
  • Shaposhnikov, (2018), J. High Energy Phys., 10
  • Shkerin, (2019), Phys. Rev. D, 99, 10.1103/PhysRevD.99.115018
  • Shaposhnikov
  • Akrami
  • Shaposhnikov, (2020), J. Cosmol. Astropart. Phys., 07
  • Kallosh, (2013), J. Cosmol. Astropart. Phys., 07
  • Galante, (2015), Phys. Rev. Lett., 114, 10.1103/PhysRevLett.114.141302
  • Kallosh, (2015), C. R. Phys., 16, pp. 914, 10.1016/j.crhy.2015.07.004
  • Artymowski, (2016), Phys. Lett. B, 761, pp. 111, 10.1016/j.physletb.2016.08.024
  • Fumagalli, (2017), Phys. Lett. B, 769, pp. 451, 10.1016/j.physletb.2017.04.017
  • Cremmer, (1978), Phys. Lett. B, 74, pp. 61, 10.1016/0370-2693(78)90060-6
  • Bergshoeff, (1981), Nucl. Phys. B, 182, pp. 173, 10.1016/0550-3213(81)90465-X
  • de Roo, (1985), Nucl. Phys. B, 255, pp. 515, 10.1016/0550-3213(85)90151-8
  • Ferrara, (2013), Phys. Rev. D, 87, 10.1103/PhysRevD.87.025004
  • 't Hooft, (1973), Nucl. Phys. B, 61, pp. 455, 10.1016/0550-3213(73)90376-3
  • Weinberg, (1973)
  • Weinberg, (1976), Phys. Rev. Lett., 36, pp. 294, 10.1103/PhysRevLett.36.294
  • Linde, (1977), Phys. Lett. B, 70, pp. 306, 10.1016/0370-2693(77)90664-5
  • Rasanen, (2019), Open J. Astrophys., 2, pp. 1, 10.21105/astro.1811.09514
  • Karananas, (2016), Phys. Lett. B, 761, pp. 223, 10.1016/j.physletb.2016.08.037
  • Karananas, (2016), Phys. Rev. D, 93
  • Casas, (2018), Phys. Rev. D, 97, 10.1103/PhysRevD.97.043520
  • Rubio, (2019), Front. Astron. Space Sci., 5, pp. 50, 10.3389/fspas.2018.00050
  • Garcia-Bellido, (2009), Phys. Rev. D, 79, 10.1103/PhysRevD.79.063531
  • Bezrukov, (2009), J. Cosmol. Astropart. Phys., 06
  • Repond, (2016), J. Cosmol. Astropart. Phys., 07
  • Rubio, (2019), J. Cosmol. Astropart. Phys., 04
  • Bezrukov, (2008), Phys. Lett. B, 659, pp. 703, 10.1016/j.physletb.2007.11.072
  • Bauer, (2008), Phys. Lett. B, 665, pp. 222, 10.1016/j.physletb.2008.06.014
  • Bezrukov, (2018), J. Cosmol. Astropart. Phys., 02
  • Fumagalli, (2016), J. High Energy Phys., 05
  • Rasanen, (2017), J. Cosmol. Astropart. Phys., 11
  • Bezrukov, (2011), J. High Energy Phys., 01
  • Bezrukov, (2015), Phys. Rev. D, 92, 10.1103/PhysRevD.92.083512
  • Shaposhnikov, (2009), Phys. Lett. B, 671, pp. 187, 10.1016/j.physletb.2008.11.054
  • Garcia-Bellido, (2011), Phys. Rev. D, 84, 10.1103/PhysRevD.84.123504
  • Bezrukov, (2013), Phys. Rev. D, 87, 10.1103/PhysRevD.87.096001
  • Garcia-Bellido, (2012), Phys. Lett. B, 718, pp. 507, 10.1016/j.physletb.2012.10.075
  • Rubio, (2014), Phys. Rev. D, 90, 10.1103/PhysRevD.90.027307
  • Casas, (2019), Phys. Rev. D, 99, 10.1103/PhysRevD.99.063512
  • Herrero-Valea, (2019), J. Cosmol. Astropart. Phys., 11
  • Rubio, (2020)
  • Gurdogan, (2016), Phys. Rev. Lett., 117
  • Karananas
  • Englert, (1976), Nucl. Phys. B, 117, pp. 407, 10.1016/0550-3213(76)90406-5
  • Shaposhnikov, (2009), Phys. Lett. B, 675, pp. 403, 10.1016/j.physletb.2009.04.040
  • Armillis, (2013), J. High Energy Phys., 10
  • Gretsch, (2015), Phys. Rev. D, 92, 10.1103/PhysRevD.92.045036
  • Almeida, (2019), J. Cosmol. Astropart. Phys., 1903
  • Blas, (2011), Phys. Rev. D, 84
  • Broy, (2015), J. High Energy Phys., 12