scholarly journals Probing the QCD vacuum with an Abelian chromomagnetic field: A study within an effective model

2009 ◽  
Vol 80 (3) ◽  
Author(s):  
L. Campanelli ◽  
M. Ruggieri
2015 ◽  
Vol 30 (02) ◽  
pp. 1550009
Author(s):  
Mahary Vasihoun ◽  
Eduardo Guendelman

As it is well known, one can lower the energy of the trivial perturbation QCD vacuum by introducing a nonvanishing chromomagnetic field strength. This happens because radiative corrections produce an effective action of the form [Formula: see text] with f′(y0) = 0 for some y0≠0. However, a vacuum with a nonzero field strength is not consistent with Poincaré Invariance (PI). Generalizing this type of effective action by introducing, in the simplest way, a four-index field strength ∂[μAναβ], which can have an expectation value without violating PI, we are lead to an effective action that can describe both a confinement phase and a perturbative phase of the theory. In the unconfined phase, the four-index field strength does not introduce new degrees of freedom, while in the confined phase both four-index field strength and ordinary gauge fields are not true degrees of freedom. The matching of these phases through membranes that couple minimally to the three-index potentials from which the four-index field strength derive, leads automatically to the MIT bag boundary conditions for the gauge fields living inside the bubble containing the perturbative phase.


Author(s):  
Li DING ◽  
Zhangcai HUANG ◽  
Atsushi KUROKAWA ◽  
Jing WANG ◽  
Yasuaki INOUE

Author(s):  
Mobeen Ur Rehman ◽  
Muhammad Adnan ◽  
Mouazma Batool ◽  
Liaqat Ali Khan ◽  
Ammar Masood

2020 ◽  
Author(s):  
John Buyungo ◽  
Mohammed Kamil Quraishi ◽  
Natasha Ewen ◽  
Steve Garnett
Keyword(s):  

2011 ◽  
Vol 20 (supp02) ◽  
pp. 133-139
Author(s):  
ALEXANDRE MESQUITA ◽  
MOISÉS RAZEIRA ◽  
DIMITER HADJIMICHEF ◽  
CÉSAR A. Z. VASCONCELLOS ◽  
ROSANA O. GOMES ◽  
...  

We study the effects of antikaon condensates in neutron stars in the framework of a relativistic effective model with derivative couplings which includes genuine many-body forces simulated by nonlinear interaction terms involving scalar-isoscalar (σ, σ*), vector-isoscalar (ω, ɸ), vector-isovector (ϱ), scalar-isovector (δ) mesons. The effective model presented in this work has a philosophy quite similar to the original version of the model with parameterized couplings. But unlike that, in which the parametrization is directly inserted in the coupling constants of the Glendenning model, we present here a method for the derivation of the parametric dependence of the coupling terms, in a way that allows in one side to consistently justify this parametrization and in the other to extend in a coherent way the range of possibilities of parameterizations in effective models with derivative couplings. The extended model is then applied to the description of the mass of neutron stars.


2015 ◽  
Vol 40 (2) ◽  
pp. 272 ◽  
Author(s):  
Meng Qiu ◽  
Shiyi Xiao ◽  
Qiong He ◽  
Shulin Sun ◽  
Lei Zhou
Keyword(s):  

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