Dynamics of Electroweak Phase Transition in the 3-3-1-1 Model
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https://doi.org/10.15625/0868-3166/30/1/14467Keywords:
electroweak phase transition, inflationary model, 3-3-1-1 modelAbstract
The bubble nucleation in the framework of 3-3-1-1 model is studied. Previous studies show that first order electroweak phase transition occurs in two periods. In this paper we evaluate the bubble nucleation temperature throughout the parameter space. Using the stringent condition for bubble nucleation formation we find that in the first period, symmetry breaking from \(SU(3)\rightarrow SU(2)\), the bubble is formed at the nucleation temperature $T=150$ GeV and the lower bound of the scalar mass is 600 GeV. In the second period, symmetry breaking from \((SU(2)\rightarrow U(1)\), only subcritical bubbles are formed. This constraint eliminates the electroweak baryon genesis in the second period of the model.Downloads
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C. Patrignani et al. (Particle Data Group), Chin. Phys. C 40 (2016) 100001.
E. W. Kolb and M.S. Turner, The Early Universe, Frontiers in Physics, Westview, Boulder, CO, 1994.
V. A. Kuzmin, V. A. Rubakov, and M. E. Shaposhnikov, Phys. Lett. B 155 (1985) 36.
D. E. Morrissey and M. J. Ramsey-Musolf, New J. Phys. 14 (2012) 125003.
Y. Aoki, F. Csikor, Z. Fodor and A. Ukawa, Phys. Rev. D 60 (1999) 013001, hep-lat/9901021.
F. Csikor, Z. Fodor and J. Heitger, Phys. Rev. Lett. 82 (1999) 21, hep-ph/9809291.
M. Laine and K. Rummukainen, Nucl. Phys. Proc. Suppl. 73 (1999) 180, hep-lat/9809045.
M. Gurtler, E.-M. Ilgenfritz and A. Schiller, Phys. Rev. D 56 (1997) 3888, hep-lat/9704013.
P. V. Dong, H. T. Hung and T. D. Tham, Phys. Rev. D 87 (2013) 115003.
P. V. Dong, D. T. Huong, Farinaldo S. Queiroz and N. T. Thuy, Phys. Rev. D 90 (2014) 075021.
D. T. Huong, P. V. Dong, C. S. Kim and N. T. Thuy, Phys. Rev. D 91 (2015) 055023.
P. V. Dong, Phys. Rev. D 92, 055026 (2015);P. V. Dong and D. T. Si, Phys. Rev. D 93 (2016) 115003.
D. T. Huong and P. V. Dong, Eur. Phys. J. C 77 (2017) 204.
P. V. Dong, D. T. Huong, D. A. Camargo, F. S. Queiroz and J. W. F. Valle, Asymmetric Dark Matter, Inflation
and Leptogenesis from B-L Symmetry Breaking, arXiv:1805.08251 [hep-ph] (2018).
V. Q. Phong, N. T. Tuong, N. C. Thao, and H. N. Long, Phys. Rev. D 99 (2019) 015035, arXiv:1805.09610[hepph].
D. Chang and H. N. Long, Phys. Rev. D 73 (2006) 053006.
I. Affleck, Phys. Rev. Lett. 46 (1981) 388; A. D. Linde, Nucl. Phys. B 216 (1983) 421 [Erratum-ibid. B 223
(1983) 544]; Phys. Lett. B 100 (1981) 37.
L. Dolan and R. Jackiw, Phys. Rev. D 9 (1974) 3320.
S. Weinberg, Phys. Rev. D 9 (1974) 3357.
C. L. Wainwright, Comput. Phys. Commun. 183 (2012) 2006.
M. Dine, R. G. Leigh, P. Y. Huet, A. D. Linde and D. A. Linde, Phys. Rev. D 46 (1992) 550, hep-ph/9203203.
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Accepted 13-01-2020
Published 05-03-2020