Titlebook: Laser Optics of Condensed Matter; Volume 2 The Physics Elsa Garmire,Alexei A. Maradudin (Chairman),Karl K Book 1991 Springer Science+Busine

cliche

鉤針織物

F. Vallée,G. Gale,C. Flytzanishe hadronic vacuum polarisation and light-by-light scattering contributions to ??. Results from an ancillary calculation of the spectrum in the isovector channel are crucial in order to further increase the precision of our determination of the hadronic vacuum polarisation contribution.

Mirage

B. H. Bairamov,I. P. Ipatova,V. V. Toporov,V. A. Voitenkorface for an important class of electrocatalysts, iridium (di)oxide. Leveraging the computing power of Hawk enabled the use of computational models with explicit solvent to compute realistic surface phase diagrams of IrO. and test its role on the kinetics of the oxygen evolution reaction on those su

迎合

Vincent Jaccarinohe hadronic vacuum polarisation and light-by-light scattering contributions to ??. Results from an ancillary calculation of the spectrum in the isovector channel are crucial in order to further increase the precision of our determination of the hadronic vacuum polarisation contribution.

FLING

虛度

Y. R. Shenectrolyte/solid interface requires 100s to 1000s of atoms for minimal simulations, and finite temperature effects must be included to prevent electrolyte freezing. Thus, realistic study of even the simplest electrocatalytic system requires long ab initio quality molecular dynamics simulations. In th

紳士

V. S. Bagaev,D. V. Kazantsev,A. G. Poiarkov,A. A. Serovted. The simulations have shown that the interaction between the ionizable cationic lipids and RNA is attractive only at low pH and effectively repulsive at high pH. In addition, the ionizable lipid, when uncharged, also shows a significantly increased flip-flop probability, which may have consequen

不斷的變動

T. F. Heinz,F. J. Himpsel,M. M. T. Loy,E. Palange,E. Bursteinrder to find analytical models of such collision processes in the future. Simulations of such increasingly complex systems require constant improvement of the numerical solver regarding the code’s performance. Thus, the red-black Gauss-Seidel smoother in the multi-grid solver, the iterative red-blac

insidious

J. Aaviksoo,J. Kuhl,I. Reimands. The initial focus of the project is the first systematic exploration of mergers from dynamical encounters (hyperbolic orbits). Such numerical relativity simulations have strengthen recent evidence that the signal GW190521 was originated by a dynamical capture of black holes.

Debark

R. W. Schoenlein,J. G. Fujimoto,G. L. Eesley,W. Capehartified. Again, synthetic seismograms are calculated, until those and observed seismograms are similar enough to stop this iterative process. In this paper we discuss several applications of synthetic seismograms calculated with finite difference schemes that can significantly improve our knowledge ab