Download presentation
Presentation is loading. Please wait.
Published byWilliam Edwards Modified over 9 years ago
1
Connecting Experiment and Theory across Length and Time-scales Algorithms and Software for Materials Research C yber I nfrastructure J. J. Rehr Department of Physics University of Washington Seattle, WA
2
Why we need computational theory: ``If I can’t calculate it, I don’t understand it.” R.P. Feynman
3
What’s going on outside NSF in CI for computational materials research?
4
CI at the DOE CMSNCMSN Currently five CRTs linking scientists at Universities, National Laboratories and Industry Advanced Computation Synchrotron x-ray sources
5
CI in Europe E uropean T heoretical S pectroscopy F acility n anoquanta Psi_k WIEN2k, VASP, ABINIT, ADF, …
6
Example 1: Multiple frequency scales: X-ray Absorption Spectra (XAS) Photon energy (eV) fcc Al UVX-ray arXiv:cond-mat/0601242 http://leonardo.phys.washington.edu/feff/opcons theory vs expt
7
CI: New Theory/Algorithm development: Green’s Function Codes ● Beyond Ground State Density Functional Theory and Quasiparticles ● Inelastic losses, self-energy Σ, vibrations, … ● Core-hole effects + Σ
8
Paradigm shift: Use Green’s functions not wave functions! Efficient! Ψ
9
FEFF8 USER FRIENDLY ab initio XAS Code BN Core-hole, SCF potentials Essential! 89 atom cluster Matrix inversion
10
FAST Parallel Computing Algorithms MPI: Natural parallelization G(E) Each CPU does few energies Lanczos: Iterative matrix inverse Smooth crossover between XANES and EXAFS! 1/N CPU FEFFMPI
11
J. J. Rehr & R.C. Albers Rev. Mod. Phys. 72, 621 (2000) Impact: Quantitative Theory of XAS; Quantitative Analysis of EXAFS and XANES 1000’s of applications
12
Impact on Science: Quantitative Theory of Optical Response UV – X-ray Optical Response Dielectric function Energy Loss (EELS) Absorption coefficient Refractive index Reflectivity X-ray scattering factors f = f 0 +f 1 + if 2 Full spectrum Green’s function (FEFF8MPI) codes
13
CI: Bayesian Fit to Experiment Approach: Minimize χ 2 =Σ i |μ i theory (X) -μ i expt | 2 + xAx (a priori information) → [Q + A] x = b Q information matrix A a priori matrix b normalized signal x parameters R,N, … μ 0 J. Synchrotron Rad. 12,70 (2004) Natural separation into Relevant (Q dominates) or Irrelevant (A dominates) parameters Combined fit of XAFS+XANES w/ a priori information
14
Real time approach for non-linear optical response in nano-scale systems Photonics Devices Y. Takimoto, F. Vila, and J. J. Rehr Supported by NSF Science and Technology Center at UW Grant DMR-0120967 (Y.T. and F.V) and DOE Grant DE-FG02-97ER45623 (JJR) and facilitated by the DOE CMSN. Example 2: Multiple length/time scales
15
CI: Real Time-TDDFT for Nano-scale systems* Perturbation ΔH(t) = − E · x θ(-t) Real space/real time solution to Kohn-Sham equations *TDDFT extension of SIESTA (LCAO Basis) A.Tsolakidis, D. Sanchez-Portal and R.M. Martin, Phys. Rev. B 235416 (2002); extended by Y. Takimoto et al.
16
Static Limit
17
Optical absorption of FTC chromophores from RT-TDDFT vs experiment FTC(A) FTC(B) FTC(C) Expt: L. Dalton et al. (UW)
18
CI: New Algorithms for Frequency Dependent Nonlinear response of large organic photonic chromophores Response function Re B 333 (ω) is related to the imaginary part of the first-order non-linear polarizability β 333. Nonlinear response of FTC chromophore
19
CI Computer-science Nuts and Bolts for Combined, user-friendly codes NEED: standard Input/Output protocols e.g. XML I/O new international standardXML (SIESTA, ABINIT, chemistry CPL …) Graphical User Interfaces GUIs e.g. JAVA, PERL or XML based: XFORM – XHTMLJAVA International cooperation (e.g. EU: n anoquanta, CML)
20
FEFFML – prototype XML for FEFF XML (Yoshi Takimoto, UW) schema for FEFF output xmu.dat 8985.121 - 3.348 0 3.19E-01 4.51E-01 -1.53E-01 8985.131 - 3.339 0.05 xmu.xml in Excel
21
CI: GUI Development in FEFF (JAVA)JAVA (J. Kas UW)
22
R x CI for MR Theory Develop user-friendly codes for materials research Combined ground state, excited state, & analysis codes Condensed matter toolkit Develop Quantitative understanding of excited states Linking theory and experiment across length & time scales Quantitative Interpretation of Spectra Train high-performance-computation savvy grad students and postdocs
23
That ’ s all folks!
24
CMSN-ESESRF
25
ETSF
26
Inelastic losses Ab initio Inelastic Mean Free Path Ab initio Collision Stopping Power Application: New Detector Design (PNNL - DHS) FEFF8-MP λ[ ε(ω) ] CSP [ ε(ω) ] arXiv:cond-mat/0605135
27
Optical Constants FEFF8 vs DESY TablesTables http://www.leonardo.washington.edu/feff/opcons
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.