Interacting Quantum Fields on de Sitter Space
| Autor: | Barata, João C. A., Jäkel, Christian D., Mund, Jens |
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| Rok vydání: | 2016 |
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| Druh dokumentu: | Working Paper |
| Popis: | In 1975 Figari, H{\o}egh-Krohn and Nappi constructed the P(phi)_2 model on the de Sitter space. Here we complement their work with new results, as well as by connecting this model to various areas of mathematics. In particular, i.) we discuss the causal structure of de Sitter space and the induces representations of the Lorentz group. We show that the UIRs of SO_0(1,2) for both the principal and the complementary series can be formulated on Hilbert spaces whose functions are supported on a Cauchy surface, ii.) we describe the free classical dynamical system in both its covariant and canonical form, and present the associated quantum one-particle KMS structures in the sense of Kay, iii.) we discuss the localisation properties of one-particle wave functions and how these properties are inherited by the algebras of local observables. In addition, we describe the relations between the modular objects (in the sense of Tomita-Takesaki theory) associated to wedge algebras and the representations of the Lorentz group, iv.) we connect the representations of SO(1,2) to unitary representations of SO(3) on the Euclidean sphere, and discuss how the P(phi)_2 interaction can be represented by a rotation invariant vector in the Euclidean Fock space. We present a novel Osterwalder-Schrader reconstruction theorem, which shows that physical infrared problems are absent on de Sitter space, v.) we explain how the generators of the boosts and the rotations for the interacting quantum field theory arise arise from the stress-energy tensor. Finally, we show that the interacting quantum fields satisfy the equations of motion in their covariant form. In summary, we argue that the de Sitter P(phi)_2 model is the simplest and most explicit relativistic quantum field theory, which satisfies basic expectations, like covariance, particle creation, stability and finite speed of light. Comment: This work replaces arXiv:1311.2905. The manuscript has been reorganised and some sections are entirely new or are now using different techniques etc. For instance, stochastic processes were an essential ingredient in arXiv:1311.2905, while in the new manuscript they do no appear at all. The version from September 17, 2019, contains corrections on the section dealing with the stress-energy tensor |
| Databáze: | arXiv |
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