Numerical renormalization group calculation of near-gap peaks in spectral functions of the Anderson model with superconducting leads

Physics – Condensed Matter – Strongly Correlated Electrons

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

18 pages, 7 figures, accepted for publication in Journal of Physics: Condensed Matter

Scientific paper

We use the numerical renormalization group method (NRG) to investigate a single-impurity Anderson model with a coupling of the impurity to a superconducting host. Analysis of the energy flow shows, in contrast to previous belief, that NRG iterations can be performed up to a large number of sites, corresponding to energy differences far below the superconducting gap. This allows us to calculate the impurity spectral function very accurately for frequencies near the gap edge, and to resolve, in a certain parameter regime, sharp peaks in the spectral function close to the gap edge.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Numerical renormalization group calculation of near-gap peaks in spectral functions of the Anderson model with superconducting leads does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Numerical renormalization group calculation of near-gap peaks in spectral functions of the Anderson model with superconducting leads, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical renormalization group calculation of near-gap peaks in spectral functions of the Anderson model with superconducting leads will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-445460

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.