Tunable Multiple Layered Dirac Cones in Optical Lattices
- 1. SUPA, Department of Physics, Heriot-Watt University, EH14 4AS, Edinburgh (United Kingdom)
- 2. ICFO - Institute of Photonic Sciences Av. Carl Friedrich Gauss, num. 3, E-08860 Castelldefels, Barcelona (Spain)
- 3. ICREA-Institucio Catalana de Recerca i Estudis Avancats, 08010 Barcelona (Spain)
- 4. ICFO - The Institute of Photonic Sciences Av. Carl Friedrich Gauss, num. 3, E-08860 Castelldefels, Barcelona (Spain)
Description
We show that multiple layered Dirac cones can emerge in the band structure of properly addressed multicomponent cold fermionic gases in optical lattices. The layered Dirac cones contain multiple copies of massless spin-1/2 Dirac fermions at the same location in momentum space, whose different Fermi velocity can be tuned at will. On-site microwave Raman transitions can further be used to mix the different Dirac species, resulting in either splitting of or preserving the Dirac point (depending on the symmetry of the on-site term). The tunability of the multiple layered Dirac cones allows us to simulate a number of fundamental phenomena in modern physics, such as neutrino oscillations and exotic particle dispersions with E∼pN for arbitrary integer N.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevLett.107.253001;
- arXiv
- arXiv:1108.1326v2;
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 107
- Journal Issue
- 25
- Journal Page Range
- p. 253001-253001.5
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43091216
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CONES; DIRAC OPERATORS; DISPERSIONS; FERMIONS; GASES; MICROWAVE RADIATION; NEUTRINO OSCILLATION; SPIN; SYMMETRY
- Descriptors DEC
- ANGULAR MOMENTUM; ELECTROMAGNETIC RADIATION; FLUIDS; MATHEMATICAL OPERATORS; PARTICLE PROPERTIES; QUANTUM OPERATORS; RADIATIONS
Optional Information
- Notes
- (c) 2011 American Institute of Physics