PPT-Collapsar Accretion and the Gamma-Ray Burst Light Curve

Author : marina-yarberry | Published Date : 2016-06-21

Christopher C Lindner Milos Milosavljevic Sean Couch Pawan Kumar The University of Texas at Austin Results We have conducted hydrodynamic simulations of the

Presentation Embed Code

Download Presentation

Download Presentation The PPT/PDF document "Collapsar Accretion and the Gamma-Ray Bu..." is the property of its rightful owner. Permission is granted to download and print the materials on this website for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.

Collapsar Accretion and the Gamma-Ray Burst Light Curve: Transcript

Christopher C Lindner Milos Milosavljevic Sean Couch Pawan Kumar The University of Texas at Austin Results We have conducted hydrodynamic simulations of the viscous postcorecollapse accretion of a rapidly rotating 14 solar mass Wolf. J. P. U. Fynbo, Niels Bohr . Institute. /. Dark . Cosmology. . Centre. What is a gamma-ray burst?. Brief (. ms. - . min. ) . and intense (. ~10. -7. erg cm. –2. . s. –1. ) . burst. . of. soft (~. extreme physics at play. Bruce Gendre. ARTEMIS. Description of a GRB. Gamma-ray Burst : . burst of high energy photons. Isotropic distribution on the sky. extragalactic events. . quite common (~2/day. 84 . Hiroshi Nagai. (National Astronomical Observatory of Japan). In collaboration with. Monica . Orienti. , Motoki Kino, Kenta Suzuki, Keiichi Asada, Akihiro . Doi. , Gabriele . Giovannini. , Marcello . Gamma ray bursts (GRB) are an especially exciting outflow phenomena that are capable of outputting as much energy as our sun will. Christopher C. . Lindner. 1. Abstract. Relativistic Jets are streams of plasma moving throughout the universe at speeds up to 99% the speed of light. They produce high-energy X-ray, radio, and visible radiation that are observable from great distances across the universe. Manel. Martinez. 4. 3. rd. . Winter Meeting. March 2015-Benasque. Outline. 1) Introduction. 2) Basics on VHE Gamma Astronomy physics. 3) VHE gamma observatories. 4) CTA. 5. ) Conclusions. 1) INTRODUCTION. Nathalie . Japkowicz. , Colin . Bellinger. , . Shiven. Sharma, Rodney Berg, Kurt . Ungar. . University of Ottawa, Northern Illinois University. Radiation Protection Bureau, Health Canada. The Magnetic Origin of Black Hole Accretion Disk Winds Chris Shrader* (NASA Goddard Space Flight Center ) Collaborators: D. Kazanas (GSFC), K. Fukumura (JMU), F. Tombesi (UMD), Ehud Behar ( Centaurus. A. July 15, 2010: Accretion Workshop. Cambridge, Massachusetts. Gregory R. Sivakoff (. UVa. ). Chandra . Cen. . A-. Very Large Project Team. A Galaxy’s Cookbook. A Population of X-Ray Binaries. Paul A. Mason. New Mexico State University. Emmanuel Gonzalez. University of Texas at El Paso. Edward L. Robinson. University of Texas at . Austin. Special thanks to . Jorge I. Zuluaga . for discussion on time-scale estimates. . 1 - ray Imaging Ethan Hull, Matthew Kiser PHDS Corporation, 3011 Amherst Road, Knoxville, TN 37921, USA Historically, radioactive material detection and localization have been accomplished through th catch a burst and notify other observatoriesboth in space and on the ground of its approx-imate locationWithin minutes HETE-2 mayobtain a precise locationCurrent telescopestake much longer to notify o Vikram . Dwarkadas. . (U Chicago). Matthieu. Renaud, . Alexandre. . Marcowith. . (LUPM, U Montpellier). Vincent . Tatischeff. . (. Univ. Paris-. Sud. ). August 11 2017. TevPA 2017 : VVD. 1. We acknowledge support from the FACCTS program at . ABRAÃO NOVA, FREDERICO RIBEIRO, PAMALLA OLIVEIRA, DANIEL AMANCIO, CÁSSIA MACHADO, ALEXANDRA CAROLINA, MARCIO PAIXÃO, ANTONIO ANTONINO, ENIVALDO BARBOSA, ANTONIO BARBOSA, MARIA LOURENÇO, MARCOS RODRIGUES, AND RICHARD HECK. Marie-Laure Mauborgne. SLB. CSG17 – July 17. th. 2023. 1. Founded by a physicist and an engineer in 1926 to conduct the first geophysical measurements of rock formations . What is SLB?. (former Schlumberger).

Download Document

Here is the link to download the presentation.
"Collapsar Accretion and the Gamma-Ray Burst Light Curve"The content belongs to its owner. You may download and print it for personal use, without modification, and keep all copyright notices. By downloading, you agree to these terms.