The vacuum structure in QCD and hadron-hadron scattering

1984 ◽  
Vol 24 (3-4) ◽  
pp. 283-296 ◽  
Author(s):  
O. Nachtmann ◽  
A. Reiter
Keyword(s):  
2021 ◽  
Vol 2021 (3) ◽  
Author(s):  
Sebastian Baum ◽  
Marcela Carena ◽  
Nausheen R. Shah ◽  
Carlos E. M. Wagner ◽  
Yikun Wang

Abstract Electroweak baryogenesis is an attractive mechanism to generate the baryon asymmetry of the Universe via a strong first order electroweak phase transition. We compare the phase transition patterns suggested by the vacuum structure at the critical temperatures, at which local minima are degenerate, with those obtained from computing the probability for nucleation via tunneling through the barrier separating local minima. Heuristically, nucleation becomes difficult if the barrier between the local minima is too high, or if the distance (in field space) between the minima is too large. As an example of a model exhibiting such behavior, we study the Next-to-Minimal Supersymmetric Standard Model, whose scalar sector contains two SU(2) doublets and one gauge singlet. We find that the calculation of the nucleation probabilities prefers different regions of parameter space for a strong first order electroweak phase transition than the calculation based solely on the critical temperatures. Our results demonstrate that analyzing only the vacuum structure via the critical temperatures can provide a misleading picture of the phase transition patterns, and, in turn, of the parameter space suitable for electroweak baryogenesis.


1983 ◽  
Vol 27 (8) ◽  
pp. 1852-1868 ◽  
Author(s):  
M. Asorey ◽  
J. G. Esteve ◽  
A. F. Pacheco

1979 ◽  
Vol 16 (2) ◽  
pp. 281-291 ◽  
Author(s):  
D.H. Mayer ◽  
K.S. Viswanathan
Keyword(s):  

2004 ◽  
Vol 597 (2) ◽  
pp. 166-172 ◽  
Author(s):  
Naoyuki Haba ◽  
Toshifumi Yamashita
Keyword(s):  

1995 ◽  
Vol 363 (1-2) ◽  
pp. 85-92 ◽  
Author(s):  
E Abdalla ◽  
K.D Rothe

1997 ◽  
Vol 506 (1-2) ◽  
pp. 521-536 ◽  
Author(s):  
L.D. Paniak ◽  
G.W. Semenoff ◽  
A.R. Zhitnitsky

1986 ◽  
Vol 182 (3-4) ◽  
pp. 221-225 ◽  
Author(s):  
N. Auerbach ◽  
Alfred S. Goldhaber ◽  
Mikkel B. Johnson ◽  
L.Dudley Miller ◽  
A. Picklesimer
Keyword(s):  

2021 ◽  
Vol 81 (3) ◽  
Author(s):  
Marzieh Peyravi ◽  
Nematollah Riazi ◽  
Francisco S. N. Lobo

AbstractIn this work, using two scalar fields ($$\phi $$ ϕ , $$\psi $$ ψ ) coupled to 4 + 1 dimensional gravity, we construct novel topological brane solutions through an explicit U(1) symmetry breaking term. The potential of this model is constructed so that two distinct degenerate vacua in the $$\phi $$ ϕ field exist, in analogy to the $$\phi ^{4}$$ ϕ 4 potential. Therefore, brane solutions appear due to the vacuum structure of the $$\phi $$ ϕ field. However, the topology and vacuum structure in the $$\psi $$ ψ direction depends on the symmetry breaking parameter $$\beta ^{2}$$ β 2 , which leads to different types of branes. As a result, one can interpret the present model as a combination of a $$\phi ^{4}$$ ϕ 4 brane with an auxiliary field, which leads to deviations from the $$\phi ^{4}$$ ϕ 4 system with the brane achieving a richer internal structure. Furthermore, we analyse in detail the behaviour of the superpotentials, the warp factors, the Ricci and Kretschmann scalars and the Einstein tensor components. In addition to this, we explore the stability of the brane in terms of the free parameters of the model. The analysis presented here complements previous work and is sufficiently novel to be interesting.


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