'Evolution equations' presentation slideshows

A New Code for Axisymmetric Numerical Relativity

A New Code for Axisymmetric Numerical Relativity. Eric Hircshmann, BYU Steve Liebling, LIU Frans Pretorius, UBC Matthew Choptuik CIAR/UBC. Black Holes III Kananaskis, Alberta May 22, 2001. Outline. Motivation Previous Work (other axisymmetric codes) Formalism & equations of motion

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Nondegenerate Solutions of Dispersionless Toda Hierarchy and Tau Functions

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Growth, Structure and Pattern Formation for Thin Films Lecture 1. Growth of Thin Films

Growth, Structure and Pattern Formation for Thin Films Lecture 1. Growth of Thin Films. Russel Caflisch Mathematics Department Materials Science and Engineering Department UCLA. www.math.ucla.edu/~material. Outline. Epitaxial Growth molecular beam epitaxy (MBE) Step edges and islands

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PERTURBED NONLINEAR EVOLUTION EQUATIONS AND ASYMPTOTIC INTEGRABILITY

PERTURBED NONLINEAR EVOLUTION EQUATIONS AND ASYMPTOTIC INTEGRABILITY. Yair Zarmi Physics Department & Jacob Blaustein Institutes for Desert Research Ben-Gurion University of the Negev Midreshet Ben-Gurion, Israel. INTEGRABLE EVOLUTION EQUATIONS. APPROXIMATIONS TO MORE COMPLEX SYSTEMS

474 views • 39 slides

PDF from Hadronic Tensor on the Lattice and Connected Sea Evolution

PDF from Hadronic Tensor on the Lattice and Connected Sea Evolution. Path-integral Formulation of Hadronic Tensor in DIS Parton Degrees of Freedom Evolution of Connected Sea Partons Numerical Challenges. Workshop on PDF at Beida , July 14-16, 2017. Experimental Data.

375 views • 37 slides

The present and (near) future of Di hadron F ragmentation F unctions ( DiFF )

The present and (near) future of Di hadron F ragmentation F unctions ( DiFF ). Transverse momentum, spin, and position distributions of partons in hadrons. ECT* (Trento), 11-15 June 2007. Marco Radici. Pavia. In collaboration with: A. Bacchetta (DESY)

453 views • 35 slides

The present and (near) future of Di hadron F ragmentation F unctions ( DiFF )

The present and (near) future of Di hadron F ragmentation F unctions ( DiFF ). Transverse momentum, spin, and position distributions of partons in hadrons. ECT* (Trento), 11-15 June 2007. Marco Radici. Pavia. In collaboration with: A. Bacchetta (DESY)

371 views • 35 slides

Overview

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Numerical simulation of forming processes: present achievements and future challenges

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Quantum Kinetic Theory

Quantum Kinetic Theory. Jian-Hua Gao Shandong University at Weihai. In collaboration with Zuo-Tang Liang, Shi Pu, Qun Wang and Xin-Nian Wang PRL 109, 232301(2012), PRD 83, 094017(2011).

436 views • 27 slides

Cristina VOLPE (AstroParticule et Cosmologie -APC)

Open issues in neutrino flavor conversion in media. Cristina VOLPE (AstroParticule et Cosmologie -APC). Neutrino flavor conversion in media. SOLAR NEUTRINOS. n e. Core-collapse supernovae (SN) and Accretion disk-black holes. Massive stars (M > 6 M sun ) emit

411 views • 26 slides

Cristina VOLPE (AstroParticule et Cosmologie -APC)

Open issues in neutrino flavor conversion in media. Cristina VOLPE (AstroParticule et Cosmologie -APC). Neutrino flavor conversion in media. SOLAR NEUTRINOS. n e. Core-collapse supernovae (SN) and Accretion disk-black holes. Massive stars (M > 6 M sun ) emit

265 views • 26 slides

Making the Constraint Hypersurface and Attractor in Free Evolution

Making the Constraint Hypersurface and Attractor in Free Evolution. David R. Fiske Department of Physics University of Maryland. Advisor: Charles Misner. gr-qc/0304024. Overview. The Problem Evolution v. Constraints Free Evolution Method of Correction Adding Terms to Evolution Equations

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Making the Constraint Hypersurface and Attractor in Free Evolution

Making the Constraint Hypersurface and Attractor in Free Evolution. David R. Fiske Department of Physics University of Maryland. Advisor: Charles Misner. gr-qc/0304024. Overview. The Problem Evolution v. Constraints Free Evolution Method of Correction Adding Terms to Evolution Equations

230 views • 23 slides

Details: frequently used expressions

Details: frequently used expressions. Leading quark distributions. For gluons we have. QCD evolution. Evolution equations. For flavor singlet combinations we have coupled equations:. First momentum. Data from CERN, SLAC & HERMES. The isotopic SU(2) invariance of strong interactions,.

282 views • 20 slides

EROFEEV Vasily MESHCHERIAKOV Dmitry a) Laboratory of nonlinear physics

A decay of electromagnetic wave quanta in a turbulent plasma during their interaction with Langmuir waves. a,b. a,c. IA&E SB RAS. EROFEEV Vasily MESHCHERIAKOV Dmitry a) Laboratory of nonlinear physics Institute of Automation and Electometry Siberian Branch of Russian Academy

341 views • 19 slides

BSSN: why/when does it work?

BSSN: why/when does it work?. Miguel Alcubierre Mexico City, May 2002. The linearized ADM equations. Consider the vacuum ADM equations, with geodesic slicing and zero shift. Consider also a linear perturbation of flat space:. The evolution equations become:. And the constraints are:.

254 views • 17 slides

Development of Cerebral Aneurysms. A Prediction Model

Development of Cerebral Aneurysms. A Prediction Model. Ihor Machyshyn. Supervisors. Dr. Ir. P.M.J. Rongen (Philips Medical Systems) Dr. Ir. A.A.F. van de Ven (TU/e, W&I) Dr. Ir. S.J.L. van Eijndhoven (TU/e, W&I) P rof. D r. I r. F.N. van de Vosse (TU/e, BMT)

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Super-lattice HAMILTONIAN (Barletti, Bonilla,Escobedo)

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