We present a study of Dirac quantum fields in a four-dimensional de Sitter spacetime. The theory is based on the requirement of precise analyticity properties of the waves and the correlation functions in the complexification of the de Sitter manifold. Holomorphic de Sitter spinorial plane waves are introduced in this way and used to construct the two-point functions, whose properties are fully characterized. The physical interpretation of the analyticity properties of Wightman's functions in terms of a KMS-type thermal condition is also given.

Dirac fields and thermal effects in the de Sitter universe / P. Bartesaghi, J.-. Gazeau, U. Moschella, M.V. Takook. - In: CLASSICAL AND QUANTUM GRAVITY. - ISSN 0264-9381. - 18:21(2001 Nov 07), pp. 4373-4394. [10.1088/0264-9381/18/21/302]

Dirac fields and thermal effects in the de Sitter universe

P. Bartesaghi
Primo
Membro del Collaboration Group
;
2001

Abstract

We present a study of Dirac quantum fields in a four-dimensional de Sitter spacetime. The theory is based on the requirement of precise analyticity properties of the waves and the correlation functions in the complexification of the de Sitter manifold. Holomorphic de Sitter spinorial plane waves are introduced in this way and used to construct the two-point functions, whose properties are fully characterized. The physical interpretation of the analyticity properties of Wightman's functions in terms of a KMS-type thermal condition is also given.
Quantum Field Theory; Quantum Gravity; de Sitter Universe:
Settore PHYS-02/A - Fisica teorica delle interazioni fondamentali, modelli, metodi matematici e applicazioni
7-nov-2001
22-ott-2001
https://iopscience.iop.org/article/10.1088/0264-9381/18/21/302
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/1122308
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