nero- a post-maximum supernova radiation transport code
نویسندگان
چکیده
منابع مشابه
Towards a 3D Space Radiation Transport Code
High-speed computational procedures for space radiation shielding have relied on asymptotic expansions in terms of the off-axis scatter and replacement of the general geometry problem by a collection of flat plates. This type of solution was derived for application to human rated systems in which the radius of the shielded volume is large compared to the off-axis diffusion limiting leakage at l...
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Radiation transport eeects on X-ray line emission are important in modeling spectroscopic-quality, synthetic spectra of mid-and high-Z tracer elements in hot dense plasmas. Plasmas produced in the laboratory are usually in non-equilibrium, i.e. the ion-ization balance and distribution of atomic-level populations are determined by a set of collisional and radiative atomic processes. In these con...
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Core collapse supernovae (SN) are the final stages of stellar evolution in massive stars during which the central region collapses, forms a neutron star (NS), and the outer layers are ejected. Recent explosion scenarios assumed that the ejection is due to energy deposition by neutrinos into the envelope but detailed models do not produce powerful explosions. There is new and mounting evidence f...
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One of the hazards faced by crews of spacecraft in space is exposure to ionizing radiation in the space environment. The main sources of these radiations are the trapped radiation in the Van Allen belts, consisting mainly of protons in the inner belt and electrons in the outer belt, the galactic cosmic ray (GCR) background, composed of all naturallyoccurring elements, and solar energetic partic...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2011
ISSN: 0035-8711
DOI: 10.1111/j.1365-2966.2011.19376.x