In this paper, we study the correspondence between a field theory in de Sitter space in D-dimensions and a dual conformal feld theory in a euclidean space in (D - 1)-dimensions. In particular, we investigate the form in which this correspondence is established for a system of interacting scalar and...
- Autores:
-
Valenzuela Toledo, Cesar Alonso; Departamento de Física, Universidad del Valle, Ciudad Universitaria Meléndez, Santiago de Cali 760032, Colombia
Beltrán Almeida, Juan; Departamento de Física, Universidad Antonio Nariño, Cra 3 Este # 47A-15, Bogotá D.C. 110231, Colombia
Motoa-Manzano, Josue; Departamento de Física, Universidad del Valle, Ciudad Universitaria Meléndez, Santiago de Cali 760032, Colombia.
- Tipo de recurso:
- Article of journal
- Fecha de publicación:
- 2016
- Institución:
- Pontificia Universidad Javeriana
- Repositorio:
- Repositorio Universidad Javeriana
- Idioma:
- eng
- OAI Identifier:
- oai:repository.javeriana.edu.co:10554/31469
- Acceso en línea:
- http://revistas.javeriana.edu.co/index.php/scientarium/article/view/16262
http://hdl.handle.net/10554/31469
- Palabra clave:
- Theoretical Physics; Cosmology
Ination; vector elds; de Sitter symmetries; parity violation.
- Rights
- openAccess
- License
- Atribución-NoComercial-SinDerivadas 4.0 Internacional
Summary: | In this paper, we study the correspondence between a field theory in de Sitter space in D-dimensions and a dual conformal feld theory in a euclidean space in (D - 1)-dimensions. In particular, we investigate the form in which this correspondence is established for a system of interacting scalar and a vector fields propagating in de Sitter space. We analyze some necessary (but not sucient) conditions for which conformal symmetry is preserved in the dual theory in (D - 1)-dimensions, making possible the establishment of the correspondence. The discussion that we address in this paper is framed on the context of inationary cosmology. Thusly, the results obtained here pose some relevant possibilities of application to the calculation of the fields’s correlation functions and of the primordial curvature perturbation \zeta, in inationary models including coupled scalar and vector fields. |
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