'Relativistic' presentation slideshows

Relativistic effects & Non-collinear magnetism (WIEN2k / WIENncm)

1.42k views • 80 slides

Chapter 6: Evolution of Post -main sequence star Stellar Physics PHYS3040

Chapter 6: Evolution of Post -main sequence star Stellar Physics PHYS3040 . TexPoint fonts used in EMF. Read the TexPoint manual before you delete this box.: A A. 6.1 Overview . Hertzsprun -Russell (HR) Diagram .

974 views • 79 slides

Accelerator Physics

Accelerator Physics. Alex Bogacz (Jefferson Lab) / bogacz@jlab.org Geoff Krafft (Jefferson Lab/ODU) / krafft@jlab.org Timofey Zolkin (U. Chicago/Fermilab) / t.v.zolkin@gmail.com. Accelerator Physics. Introductions and Outline. Syllabus Week 1 Week 2 Introduction

650 views • 54 slides

Sergei A.Klioner

Ephemerides in the relativistic framework: _ time scales, spatial coordinates, astronomical constants and units. Sergei A.Klioner. Lohrmann Observatory, Dresden Technical University Paris Observatory, 6 April 2006. Newtonian astrometry and Newtonian equations of motion Why relativity? ?

726 views • 52 slides

Gamma Ray Bursts

Gamma Ray Bursts. S. R. Kulkarni California Institute of Technology. Acknowledgements. Alicia Soderberg Caltech/NRAO/Carnegie gang Berger, Cenko, Fox, Frail, Harrison, Price, Schmidt T. Sakamoto & R. Yamazaki. Quasars: A Historical Analogy, I.

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What is the Apparent Temperature of Relativistically Moving Bodies ?

492 views • 41 slides

Relativistic MHD Simulations of Relativistic Jets

Relativistic MHD Simulations of Relativistic Jets. Yosuke Mizuno NASA Postdoctoral Program Fellow NASA Marshall Space Flight Center (MSFC) National Space Science and Technology Center (NSSTC). Context. Introduction Development of 3D GRMHD code 2D GRMHD simulations of Jet Formation

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Relativistic Description of the Ground State of Atomic Nuclei Including Deformation

Relativistic Description of the Ground State of Atomic Nuclei Including Deformation and Superfluidity. Jean-Paul EBRAN. CEA/DAM/DIF. 24/11/2010. Goal. Description of the ground state of atomic nuclei including nuclea r deformation and superfluidity.

443 views • 33 slides

Neutron Stars 1: Basics

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Neutron Stars 1: Basics

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Large enhancement of KK dark matter annihilation rate due to threshold singularity

Large enhancement of KK dark matter annihilation rate due to threshold singularity. Mitsuru Kakizaki (ICRR, University of Tokyo). Dec. 2004 @ Stanford Univ. Collaborated with Shigeki Matsumoto and Masato Senami (ICRR), in preparation.

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352 views • 24 slides

Stellar neutrino emission at finite temperature in relativistic mean field theory

Quarks and Compact Stars 2014, October, 20-22 , 2014 , Beijing, China. Stellar neutrino emission at finite temperature in relativistic mean field theory. Jinniu Hu. School of Physics, Nankai University. Jinniu Hu. 11/20/13. 20/10/2014. 1. Outline. Introduction

349 views • 23 slides

Relativistic nonlinear optics in laser-plasma interaction

Relativistic nonlinear optics in laser-plasma interaction. Jyhpyng Wang. Institute of Atomic and Molecular Sciences Academia Sinica, Taiwan. National Central University, Taiwan. National Taiwan University, Taiwan. Outline. Relativistic nonlinearity in laser-plasma interaction

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Relativistic nonlinear optics in laser-plasma interaction

Relativistic nonlinear optics in laser-plasma interaction. Jyhpyng Wang. Institute of Atomic and Molecular Sciences Academia Sinica, Taiwan. National Central University, Taiwan. National Taiwan University, Taiwan. Outline. Relativistic nonlinearity in laser-plasma interaction

371 views • 22 slides

Relativistic Mass and Energy

Relativistic Mass and Energy. Physics 12. Jokes of the day:. Clip of a day:. http:// www.youtube.com/watch?v=lR4tJr7sMPM&list=PLDA75FE6344666889. Universal Speed Limit. When considering gamma, we know that we must be dealing with real numbers so the value under the root must be positive

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Non-linear dynamics of relativistic particles: How good is the classical phase space approach?

Non-linear dynamics of relativistic particles: How good is the classical phase space approach?. Peter J. Peverly Sophomore Intense Laser Physics Theory Unit Illinois State University. www.phy.ilstu.edu/ILP. Acknowledgment. Undergrad researchers: R. Wagner, cycloatoms

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What are Cycloatoms?

What are Cycloatoms?. Robert E. Wagner Sophomore Intense Laser Physics Theory Unit Illinois State University. www.phy.ilstu.edu/ILP. Support: NSF, Res. Corp., and ISU Honors Program. Magnetic field. Laser. More Technical:. Use RK4 to solve this. Maximum speed v/c for each W.

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Solitons in relativistic mean field models

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Stellar Structure

253 views • 7 slides