elko spinors
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2021 ◽  
Author(s):  
Xiang-Nan Zhou ◽  
Yun-Zhi Du ◽  
Zhen-Hua Zhao
Keyword(s):  

Author(s):  
L. C. Duarte ◽  
R. de C. Lima ◽  
R. J. Bueno Rogerio ◽  
C. H. Coronado Villalobos

Author(s):  
Xiang-Nan Zhou ◽  
Yun-Zhi Du ◽  
Zhen-Hua Zhao ◽  
Yu-Xiao Liu

2015 ◽  
Vol 91 (4) ◽  
Author(s):  
I. C. Jardim ◽  
G. Alencar ◽  
R. R. Landim ◽  
R. N. Costa Filho
Keyword(s):  

2014 ◽  
Vol 23 (14) ◽  
pp. 1444008 ◽  
Author(s):  
S. H. Pereira ◽  
A. Pinho S. S.

A brief review is presented about the ELKO spinor field applied to cosmology, with the main results and limitations of the theory. As a simple application, we have analyzed a model involving the interaction of the ELKO spinor field with dark matter in the universe from a dynamical system approach. When the system is rewritten in terms of the deceleration parameter q and under the assumption that such parameter is nearly constant for some different stages of the evolution, stability points were found for different types of interaction between dark matter and ELKO spinors. Within this new analysis several interesting scenarios are possible, depending on the interaction term. For example, if it is assumed that the equation of the state parameter of the ELKO field is of the phantom type, ωϕ < -1, the current acceleration of the universe can be driven by the decay of dark matter particles into ELKO field. Furthermore, even for ωϕ > 0, the inflationary period can be driven by the decay of the inflaton field (described by the ELKO spinor) into dark matter particles.


2012 ◽  
Vol 86 (6) ◽  
Author(s):  
Yu-Xiao Liu ◽  
Xiang-Nan Zhou ◽  
Ke Yang ◽  
Feng-Wei Chen
Keyword(s):  

2009 ◽  
Vol 87 (8) ◽  
pp. 909-916 ◽  
Author(s):  
K. E. Wunderle ◽  
R. Dick

We review the transformation properties of ELKO spinors (Eigenspinoren des Ladungskonjugationsoperators) under charge conjugation, parity, and time reversal. Our calculations confirm that ELKO spinors are not eigenspinors of the helicity operator and satisfy [Formula: see text] which identifies them as a representation of a nonstandard Wigner class. However, we find that ELKO spinors transform symmetrically under parity instead of the previously assumed asymmetry. Furthermore, we demonstrate that ELKO spinors transform asymmetrically under time reversal, which is opposite to the previously reported symmetric behaviour. These changes affect the (anti)commutation relations that are satisfied by the operators acting on ELKO spinors. We are also able to show that ELKO spinors actually satisfy the same (anti)commutation relations as Dirac spinors, even though they belong to two different representations.


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