Enviar artigo por via de e-mail About Interaction of the Spinor and Scalar Fields, Removing Contribution of the Scalar Field in the Geometry of the Space-Time
- Autores: Vilca Chaicha MB1, Yuschenko LP1, Shikin GN1
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Afiliações:
- Peoples Friendship University of Russia
- Edição: Nº 2 (2012)
- Páginas: 97-103
- Seção: Articles
- URL: https://journals.rcsi.science/2658-4670/article/view/328700
- ID: 328700
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Resumo
In the static cylindrically symmetric metric and cosmological metric Bianchi I we consider the interacting scalar and spinor fields with the Lagrangian of the interaction Lint = V (φ)S2, where V (φ) is arbitrary function of scalar field φ, S = ψ¯ψ is an invariant of the spinor field ψ. We obtain exact solutions of the Einstein, spinor and scalar equations and one exhibited that function V (φ) is absent in the components of the energy-momentum tensor for the interacting fields. It means that the considered type of the interaction removes the contribution of the scalar field in the geometry of the space-time.
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Sobre autores
M Vilca Chaicha
Peoples Friendship University of Russia
Email: marfon17@mail.ru
Кафедра теоретической физики; Российский университет дружбы народов; Peoples Friendship University of Russia
L Yuschenko
Peoples Friendship University of RussiaКафедра общей физики; Российский университет дружбы народов; Peoples Friendship University of Russia
G Shikin
Peoples Friendship University of RussiaКафедра теоретической физики; Российский университет дружбы народов; Peoples Friendship University of Russia
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