'Core collapse' presentation slideshows

Modelling SN Type II: collapse and simple bounce

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Core Collapse SNe

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Core-Collapse Supernovae: Magnetorotational Explosions and Jet Formation

Core-Collapse Supernovae: Magnetorotational Explosions and Jet Formation. G.S.Bisnovatyi-Kogan, JINR and Space Research Institute, Moscow. Dubna, August 21, 2006. Content. 1. Presupernovae 2. Development of SN theory 3. Magnetorotational mechanism of explosion

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Magnetorotational core-collapse supernovae.

Magnetorotational core-collapse supernovae. Sergey Moiseenko, Gennady Bisnovatyi-Kogan Space Research Institute, Moscow, Russia. Outline. Introduction Numerical method (implicit Lagrangian scheme) Magnetorotational(MR) mechanism of supernova explosion. Core-collapse simulations.

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Cosmology with Supernovae

Cosmology with Supernovae. Bruno Leibundgut European Southern Observatory. Outline. Supernova types core-collapse supernovae thermonuclear supernovae Cosmology with supernovae Hubble constant, H 0 ? lecture I mapping of the cosmological expansion history, H(z) ? lecture II.

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Mounib El Eid American University of Beirut Department of Physics

Nucleosynthesis & Cosmology. Infrared light from first stars: Spitzer image ( z=11). You are back to about 400 million years after Big Bang. Mounib El Eid American University of Beirut Department of Physics. Santa Tecla : Sept. 18, 2011. program. 1. General comments.

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Chapters Eighteen / Nineteen

Chapters Eighteen / Nineteen. Questions for the Day. What are stars born? How do stars evolve? How do stars die?. How are stars born?. Stars are born from interstellar medium. Disturbances from motion of the galaxy and other stars in the medium cause cores to form.

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John M. Blondin NC State University

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Agnieszka Janiuk

Agnieszka Janiuk. N. Copernicus Astronomical Center, Warsaw. Gamma Ray Bursts from Collapsing Massive Stars. Collaborations: R. Moderski (CAMK), D. Proga(UNLV), Y. Yuan (ChAS), R. Perna (JILA), T. Di Matteo (CMU), B. Czerny (CAMK), D. Cline (UCLA), S. Otwinowski (CERN), C. Matthey (CERN).

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Cosmological measurements with Supernovae Ia

Cosmological measurements with Supernovae Ia. What is a SNIa ? Distance and cosmology Observations Standardisation (x1,c) Hubble diagram Spectra : SNfactory Variability / spectra. G. Smadja (IPNL). Supernovae Ia Luminosity. f. Extremely luminous (10 10 L A )

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The Diffuse Supernova Neutrino Background

The Diffuse Supernova Neutrino Background. Louie Strigari The Ohio State University. Collaborators: John Beacom, Manoj Kaplinghat, Gary Steigman, Terry Walker, Pengjie Zhang. The Plan. Diffuse Supernova Neutrino Background Theoretical Prediction

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Soft Disks: Proto-Planetary Disks in your Computer

Soft Disks: Proto-Planetary Disks in your Computer. Garrelt Mellema. Numerical Models. Reasons to use numerical models: Reproduce observations / fitting parameters Observations = radiation, so always requires radiative transfer of some sort.

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The structure and evolution of stars

The structure and evolution of stars. Lecture13: Supernovae - deaths of massive stars. Complete notes available online: http://star.pst.qub.ac.uk/~sjs/teaching.html. Learning Outcomes. In these final two lectures the student will learn about the following issues: What is a supernova

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Detection and study of supernovae with the 4m International Liquid Mirror Telescope

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Phase transition induced collapse of Neutron stars

Phase transition induced collapse of Neutron stars. Kim, Hee Il Astronomy Program, SNU 13th Haengdang Symposium, 11/30/2007. Neutron star collapse. Howto? Find a (initial) equilibrium star Perturb the equilbrium star Follow the evolution ? Various instability modes

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Rezo Shanidze

KM3NeT sensitivity to neutrino bursts from galactic supernovae. Rezo Shanidze. VLVnT08 - Toulon, Var, France 22-24 April 2008. Introduction. Is a n -burst from a core collapse of a massive star (Supernova type-II) in Galaxy detectable with KM3NeT ?

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Supernovae Light Curves Powered by Young Magnetars

Supernovae Light Curves Powered by Young Magnetars. The past/current (e.g. ROTSE, SNLS, SDSS, Palomar Transient Factory,Pan-Starrs1) and future (Dark Energy Survey, SkyMapper) supernovae surveys probe large volumes, revealing a diversity of supernovae not previously known.

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Core-collapse SN neutrinos and GW bursts

?. Core-collapse SN neutrinos and GW bursts. We are developing a proposal to the LSC-Virgo to search for associated bursts of low-energy neutrinos and GW bursts Goal: to present proposal for March L-V meeting. Neutrino community: W Fulgione (LNGS, LVD), K Scholberg (Duke U, Super-K)

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