The Holstein polaron: results from numerical and analytical ... - PiTP

20.11.2014 • Views

Share Embed Flag

The Holstein polaron: results from numerical and analytical ... - PiTP

The Holstein polaron: results from numerical and analytical ... - PiTP

DOWNLOAD ePAPER

pitp.physics.ubc.ca

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

START NOW

2D <strong>results</strong> for ground-state properties

1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
19
20
21
22
23
24
25
26
27
29
30
31
32

Berry-Phase Induced Kondo Effect in Single-Molecule Magnets

Robert Raussendorf Statement and Readings - Pacific Institute of ...

The Density Matrix Renormalization - PiTP

A fault-tolerant one-way quantum computer - PiTP

The UNCERTAINTY PRINCIPLE Uncertainty Principle II - PiTP

Spin pumping and spin transport in magne0c metal and insulator ...

Part 1 - PiTP

Quantum Dynamics of a Superconducting Flux-Qubit

Infinite randomness and the superconductor-metal transition - PiTP

Quantum Information, the Ambiguity of the Past, and the Birth ... - PiTP

PCE STAMP - Pacific Institute of Theoretical Physics

Angular dependence of FMR measurements in exchange ... - PiTP

LARGE-SCALE COHERENCE & DECOHERENCE - PiTP

Domain Wall Motion in Magnetic Nanowires - PiTP

2D <strong>results</strong> for ground-state properties

Page 1 and 2: The Holstein polaron: results from
Page 3 and 4: Model of interest: the Holstein Ham
Page 5 and 6: (spin is irrelevant, N = number of
Page 7 and 8: infinitely strong coupling, t=0 ele
Page 9 and 10: Quantity of interest: the Green’s
Page 11 and 12: Most numerical approaches focus on
Page 13 and 14: Quantum Monte Carlo methods (Kornil
Page 15: New proposal: the MA (n) hierarchy
Page 20 and 21: λ = 0.5 λ = 1 λ = 2 A(k,ω) in 1
Page 22 and 23: Problems easy to fix improve the a
Page 24 and 25: 1D, Ω=0.5t 1D, Ω=0.1t λ = 0.6 λ
Page 26 and 27: 1D, k=0, Ω=0.5t MA (0) MA (2)
Page 29 and 30: Generalizations: Lucian: multiple
Page 31 and 32: (ii) Spectral weight sum rules (see