The Los Alamos Supernova Light Curve Project: Computational Methods
Autor: | Christopher J. Fontes, Aimee Hungerford, James Colgan, Chris L. Fryer, Wesley Even, Daniel J. Whalen, Lucille H. Frey |
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Jazyk: | angličtina |
Rok vydání: | 2012 |
Předmět: |
High Energy Astrophysical Phenomena (astro-ph.HE)
Physics COSMIC cancer database Astrophysics::High Energy Astrophysical Phenomena James Webb Space Telescope Astrophysics::Instrumentation and Methods for Astrophysics FOS: Physical sciences Astronomy Astronomy and Astrophysics Large Synoptic Survey Telescope Astrophysics::Cosmology and Extragalactic Astrophysics Light curve law.invention Telescope Supernova Stars Space and Planetary Science law Dark energy Astrophysics::Solar and Stellar Astrophysics Astrophysics - High Energy Astrophysical Phenomena Astrophysics - Instrumentation and Methods for Astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) Astrophysics::Galaxy Astrophysics |
Popis: | We have entered the era of explosive transient astronomy, in which upcoming real-time surveys like the Large Synoptic Survey Telescope (LSST), the Palomar Transient Factory (PTF) and Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) will detect supernovae in unprecedented numbers. Future telescopes such as the James Webb Space Telescope may discover supernovae from the earliest stars in the universe and reveal their masses. The observational signatures of these astrophysical transients are the key to unveiling their central engines, the environments in which they occur, and to what precision they will pinpoint cosmic acceleration and the nature of dark energy. We present a new method for modeling supernova light curves and spectra with the radiation hydrodynamics code RAGE coupled with detailed monochromatic opacities in the SPECTRUM code. We include a suite of tests that demonstrate how the improved physics is indispensable to modeling shock breakout and light curves. 18 pages, 19 figures, published in ApJ Supplements |
Databáze: | OpenAIRE |
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