Titlebook: Handbook of Supernovae; Athem W. Alsabti,Paul Murdin Living reference work 2020Latest edition Cosmology from Supernovae.Explosion Mechani

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Cosmology with Type IIP Supernovae, progenitors prior to the supernova event, the explosion itself is well understood to be that of a single red supergiant star undergoing core collapse and depositing?～?10.?ergs of energy into its atmosphere. While the past two decades have been dominated by the success of using Type Ia supernovae as

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Schlemms-Canal

Diffuse Neutrino Flux from Supernovae, constant in time, this flux represents an attractive opportunity for steady progress in the field of supernova?neutrinos. The DSNB?has a unique potential, because it offers an image of the whole population of collapsing stars, including cosmologically distant supernovae?and rare collapse types that

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Discovery of Cosmic Acceleration,tieth century. Two teams of scientists took advantage of advances in detector technology and improved understanding of supernovae to map the expansion history of the universe half way back to the Big Bang. Their original goal was to estimate the mass density of the universe, but as their measurement

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Dust and Molecular Formation in Supernovae,trons in young SNe can destroy molecules, and strong X-ray radiation and shocks can destroy molecules and dust grains in SNRs. That concept was broken by detection of CO, SiO, and dust thermal emission in Supernova 1987A. Since 1987, the number of studies which have found molecules and dust in SNe a

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Dynamical Evolution and Radiative Processes of Supernova Remnants, (CSM) through to the final dissolution of the remnant into the interstellar medium (ISM). Supernova ejecta drive a blast wave through any CSM from the progenitor system; as material is swept up, a reverse shock forms in the ejecta, reheating them. This ejecta-driven phase lasts until ten or more ti

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Effect of Supernovae on the Local Interstellar Material, interstellar medium near the heliosphere. In this paper, we review the characteristics of the local interstellar medium that have been affected by supernovae. The kinematics, magnetic field, elemental abundances, and configuration of the nearest interstellar material support the view that the Sun i