Spatial Pauli blocking of spontaneous emission in optical lattices
- 1. Institute for Quantum Optics and Quantum Information of the Austrian Academy of Sciences, A-6020 Innsbruck (Austria)
- 2. Institute for Theoretical Physics, University of Innsbruck, A-6020 Innsbruck (Austria)
- 3. Departamento de Fisica Teorica I, Universidad Complutense, E-28040 Madrid (Spain)
- 4. Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260 (United States)
Description
Spontaneous emission by an excited fermionic atom can be suppressed due to the Pauli exclusion principle if the relevant final states after the decay are already occupied by identical atoms in the ground state. Here we discuss a setup where a single atom is prepared in the first excited state on a single site of an optical lattice under conditions of very tight trapping. We investigate these phenomena in the context of two experimental realizations: (1) with alkali-metal atoms, where the decay rate of the excited state is large, and (2) with alkaline-earth-metal-like atoms, where the decay rate from metastable states can be tuned in experiments. This phenomenon has potential applications towards reservoir engineering and dissipative many-body state preparation in an optical lattice.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevA.84.043825;
- arXiv
- arXiv:1107.3375v1;
Publishing Information
- Journal Title
- Physical Review. A
- Journal Volume
- 84
- Journal Issue
- 4
- Journal Page Range
- p. 043825-043825.11
- ISSN
- 1050-2947
- CODEN
- PLRAAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44051785
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- ALKALI METALS; ALKALINE EARTH METALS; ATOMS; CHANNELING; DECAY; EXCITED STATES; FERMIONS; GROUND STATES; MANY-BODY PROBLEM; METASTABLE STATES; PAULI PRINCIPLE; POTENTIALS; TRAPPING
- Descriptors DEC
- ELEMENTS; ENERGY LEVELS; EXCITED STATES; METALS
Optional Information
- Notes
- (c) 2011 American Institute of Physics