Cosmological particle production in a quantum field simulator as a quantum mechanical scattering problem

The production of quantum field excitations or particles in cosmological spacetimes is a hallmark prediction of curved quantum field theory. The generation of cosmological perturbations from quantum fluctuations in the early Universe constitutes an important application. The problem can be quantum-simulated in terms of structure formation in an interacting Bose-Einstein condensate (BEC) with time-dependent s-wave scattering length. Here, we explore a mapping between cosmological particle production in general ($D+1$)-dimensional spacetimes and scattering problems described by the nonrelativistic stationary Schr"odinger equation in one dimension. Through this mapping, intuitive explanations for emergent spatial structures in both the BEC and the cosmological system can be obtained for analogue cosmological scenarios that range from power-law expansions to periodic modulations. The investigated cosmologies and their scattering analogs are tuned to be implemented in a ($2+1$)-dimensional quantum field simulator.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-12-16
DOI
https://doi.org/10.1103/physrevd.110.123523
Citations
7
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
2.32

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article

Cosmological particle production in a quantum field simulator as a quantum mechanical scattering problem

Markus K. Oberthaler, Nikolas Liebster, Mireia Tolosa-Simeón, Marius Sparn et al.
7 citations
Physical review. D/Physical review. D.
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article

Cosmological particle production in a quantum field simulator as a quantum mechanical scattering problem

Markus K. Oberthaler, Nikolas Liebster, Mireia Tolosa-Simeón, Marius Sparn, Stefan Floerchinger, Elinor Kath, Christian F. Schmidt, Helmut Strobel, Álvaro Parra-López, Jelte Duchene
article en
7 citations

Abstract

The production of quantum field excitations or particles in cosmological spacetimes is a hallmark prediction of curved quantum field theory. The generation of cosmological perturbations from quantum fluctuations in the early Universe constitutes an important application. The problem can be quantum-simulated in terms of structure formation in an interacting Bose-Einstein condensate (BEC) with time-dependent s-wave scattering length. Here, we explore a mapping between cosmological particle production in general ($D+1$)-dimensional spacetimes and scattering problems described by the nonrelativistic stationary Schr\"odinger equation in one dimension. Through this mapping, intuitive explanations for emergent spatial structures in both the BEC and the cosmological system can be obtained for analogue cosmological scenarios that range from power-law expansions to periodic modulations. The investigated cosmologies and their scattering analogs are tuned to be implemented in a ($2+1$)-dimensional quantum field simulator.

Physical review. D/Physical review. D.Vol. 110(12)
Universidad Complutense de Madrid (ES), Heidelberg University (DE), Friedrich Schiller University Jena (DE), Ruhr University Bochum (DE)
European Cooperation in Science and Technology, Deutsche Forschungsgemeinschaft, Studienstiftung des Deutschen Volkes, Ministerio de Ciencia e Innovación
Affordable and clean energy
Openalex Percentile: Top 12%
Cosmology and Gravitation Theories
2.32
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