Schwinger-Keldysh superspace in quantum mechanics
Abstract
We examine, in a quantum mechanical setting, the Hilbert space representation of the Becchi, Rouet, Stora, and Tyutin (BRST) symmetry associated with Schwinger-Keldysh path integrals. This structure had been postulated to encode important constraints on influence functionals in coarse-grained systems with dissipation, or in open quantum systems. Operationally, this entails uplifting the standard Schwinger-Keldysh two-copy formalism into superspace by appending BRST ghost degrees of freedom. These statements were previously argued at the level of the correlation functions. We provide herein a complementary perspective by working out the Hilbert space structure explicitly. Our analysis clarifies two crucial issues not evident in earlier works: first, certain background ghost insertions necessary to reproduce the correct Schwinger-Keldysh correlators arise naturally, and, second, the Schwinger-Keldysh difference operators are systematically dressed by the ghost bilinears, which turn out to be necessary to give rise to a consistent operator algebra. We also elaborate on the structure of the final state (which is BRST closed) and the future boundary condition of the ghost fields.
- Authors:
- Publication Date:
- Research Org.:
- Univ. of California, Davis, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1439370
- Alternate Identifier(s):
- OSTI ID: 1498876
- Grant/Contract Number:
- SC0009999
- Resource Type:
- Published Article
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Name: Physical Review D Journal Volume: 97 Journal Issue: 10; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; quantum field theory (low energy); topological field theories; many-body techniques
Citation Formats
Geracie, Michael, Haehl, Felix M., Loganayagam, R., Narayan, Prithvi, Ramirez, David M., and Rangamani, Mukund. Schwinger-Keldysh superspace in quantum mechanics. United States: N. p., 2018.
Web. doi:10.1103/PhysRevD.97.105023.
Geracie, Michael, Haehl, Felix M., Loganayagam, R., Narayan, Prithvi, Ramirez, David M., & Rangamani, Mukund. Schwinger-Keldysh superspace in quantum mechanics. United States. https://doi.org/10.1103/PhysRevD.97.105023
Geracie, Michael, Haehl, Felix M., Loganayagam, R., Narayan, Prithvi, Ramirez, David M., and Rangamani, Mukund. Tue .
"Schwinger-Keldysh superspace in quantum mechanics". United States. https://doi.org/10.1103/PhysRevD.97.105023.
@article{osti_1439370,
title = {Schwinger-Keldysh superspace in quantum mechanics},
author = {Geracie, Michael and Haehl, Felix M. and Loganayagam, R. and Narayan, Prithvi and Ramirez, David M. and Rangamani, Mukund},
abstractNote = {We examine, in a quantum mechanical setting, the Hilbert space representation of the Becchi, Rouet, Stora, and Tyutin (BRST) symmetry associated with Schwinger-Keldysh path integrals. This structure had been postulated to encode important constraints on influence functionals in coarse-grained systems with dissipation, or in open quantum systems. Operationally, this entails uplifting the standard Schwinger-Keldysh two-copy formalism into superspace by appending BRST ghost degrees of freedom. These statements were previously argued at the level of the correlation functions. We provide herein a complementary perspective by working out the Hilbert space structure explicitly. Our analysis clarifies two crucial issues not evident in earlier works: first, certain background ghost insertions necessary to reproduce the correct Schwinger-Keldysh correlators arise naturally, and, second, the Schwinger-Keldysh difference operators are systematically dressed by the ghost bilinears, which turn out to be necessary to give rise to a consistent operator algebra. We also elaborate on the structure of the final state (which is BRST closed) and the future boundary condition of the ghost fields.},
doi = {10.1103/PhysRevD.97.105023},
journal = {Physical Review D},
number = 10,
volume = 97,
place = {United States},
year = {Tue May 29 00:00:00 EDT 2018},
month = {Tue May 29 00:00:00 EDT 2018}
}
https://doi.org/10.1103/PhysRevD.97.105023
Web of Science
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