Chiral asymmetry in relativistic matter in a magnetic field

2009 ◽  
Author(s):  
I. A. Shovkovy ◽  
Marvin L. Marshak
2011 ◽  
Vol 83 (8) ◽  
Author(s):  
E. V. Gorbar ◽  
V. A. Miransky ◽  
I. A. Shovkovy

2012 ◽  
Vol 67 (2) ◽  
pp. 547-551 ◽  
Author(s):  
E.V. Gorbar ◽  
V.A. Miransky ◽  
I.A. Shovkovy

2013 ◽  
Vol 88 (2) ◽  
Author(s):  
E. V. Gorbar ◽  
V. A. Miransky ◽  
I. A. Shovkovy ◽  
Xinyang Wang

2011 ◽  
Vol 695 (1-4) ◽  
pp. 354-358 ◽  
Author(s):  
E.V. Gorbar ◽  
V.A. Miransky ◽  
I.A. Shovkovy

2014 ◽  
Vol 90 (8) ◽  
Author(s):  
Lifang Xia ◽  
E. V. Gorbar ◽  
V. A. Miransky ◽  
I. A. Shovkovy

2018 ◽  
Vol 172 ◽  
pp. 08001
Author(s):  
Alejandro Ayala ◽  
L. A. Hernández ◽  
Jordi Salinas

We compute a net electric current during a first order EWPT arising from the asymmetric propagation of fermion chiral modes due to a CP-violating interaction with the Higgs. The interaction is quantified in terms of a CP-violating phase in the bubble wall that separate both phases. We comment on the possibility of this current to generate a seed magnetic field and its implications for primordial magnetogenesis in the early Universe.


2005 ◽  
Vol 20 (06) ◽  
pp. 1095-1102 ◽  
Author(s):  
ROMAN V. BUNIY

For uniform arrangements of magnetic fields, strings, or domain walls (together with the cosmological constant and non-relativistic matter), exact solutions to the Einstein equations are shown to lead to a universe with ellipsoidal expansion. We argue the results can be used to explain some features in the WMAP data. The magnetic field case is the easiest to motivate and has the highest possibility of yielding reliable constraints on observational cosmology.


2010 ◽  
Vol 186 ◽  
pp. 471-478
Author(s):  
Eduard Gorbar ◽  
Vladimir Miransky ◽  
Igor Shovkovy

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