Flag-dipole spinor fields in ESK gravities

被引:62
|
作者
da Rocha, Roldao [1 ]
Fabbri, Luca [2 ,3 ,4 ]
Hoff da Silva, J. M. [5 ]
Cavalcanti, R. T. [6 ]
Silva-Neto, J. A. [6 ]
机构
[1] Univ Fed ABC, Ctr Matemat Computacao & Cognicao, BR-09210170 Santo Andre, SP, Brazil
[2] Univ Genoa, DIPTEM, Sez Metodi & Modelli Matemat, I-16129 Genoa, Italy
[3] Univ Bologna, INFN, I-40126 Bologna, Italy
[4] Univ Bologna, Dipartimento Fis, I-40126 Bologna, Italy
[5] UNESP, BR-12516410 Guaratingueta, SP, Brazil
[6] Univ Fed ABC, CCNH, BR-09210170 Santo Andre, SP, Brazil
关键词
F(R) GRAVITY; TORSION; MODEL;
D O I
10.1063/1.4826499
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We consider the Riemann-Cartan geometry as a basis for the Einstein-Sciama-Kibble theory coupled to spinor fields: we focus on f(R) and conformal gravities, regarding the flag-dipole spinor fields, type-(4) spinor fields under the Lounesto classification. We study such theories in specific cases given, for instance, by cosmological scenarios: we find that in such background the Dirac equation admits solutions that are not Dirac spinor fields, but in fact the aforementioned flag-dipoles ones. These solutions are important from a theoretical perspective, as they evince that spinor fields are not necessarily determined by their dynamics, but also a discussion on their structural (algebraic) properties must be carried off. Furthermore, the phenomenological point of view is shown to be also relevant, since for isotropic Universes they circumvent the question whether spinor fields do undergo the Cosmological Principle. (C) 2013 AIP Publishing LLC.
引用
收藏
页数:12
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