Published February 15, 2010
| Version v1
Report
Semiclassical Time Evolution of the Holes from Luttinger Hamiltonian
Description
We study the semi-classical motion of holes by exact numerical solution of the Luttinger model. The trajectories obtained for the heavy and light holes agree well with the higher order corrections to the abelian and the non-abelian adiabatic theories in Ref. [1] [S. Murakami et al., Science 301, 1378 (2003)], respectively. It is found that the hole trajectories contain rapid oscillations reminiscent of the 'Zitterbewegung' of relativistic electrons. We also comment on the non-conservation of helicity of the light holes.
Availability note (English)
Available from http://www.slac.stanford.edu/cgi-wrap/getdoc/slac-pub-13905.pdf; http://www.slac.stanford.edu/cgi-wrap/pubpage?slac-pub-13905.html; PURL: https://www.osti.gov/servlets/purl/972235-UUJE9M/Additional details
Identifiers
Publishing Information
- Imprint Pagination
- 4 p.
- Report number
- SLAC-PUB--13905
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 41049785
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Non-conventional Literature
- Descriptors DEI
- ELECTRONS; HAMILTONIANS; HELICITY; NUMERICAL SOLUTION; OSCILLATIONS; TRAJECTORIES; ZITTERBEWEGUNG
- Descriptors DEC
- ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MATHEMATICAL OPERATORS; MATHEMATICAL SOLUTIONS; PARTICLE PROPERTIES; QUANTUM OPERATORS
Optional Information
- Contract/Grant/Project number
- AC02-76SF00515
- Notes
- Submitted to Physical Review
- Funding organization
- US Department of Energy (United States)