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

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书目名称Handbook of Supernovae影响因子(影响力)




书目名称Handbook of Supernovae影响因子(影响力)学科排名




书目名称Handbook of Supernovae网络公开度




书目名称Handbook of Supernovae网络公开度学科排名




书目名称Handbook of Supernovae被引频次




书目名称Handbook of Supernovae被引频次学科排名




书目名称Handbook of Supernovae年度引用




书目名称Handbook of Supernovae年度引用学科排名




书目名称Handbook of Supernovae读者反馈




书目名称Handbook of Supernovae读者反馈学科排名

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rom across many subdisciplines.Serves as a starting point fo.There is a great deal of primary and specialist literature on supernovae, with a great many scientific groups around the world focusing on the phenomenon and related subdisciplines, but what is missing is a comprehensive and balanced refer

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Adam G. Riessoversial policy-making process, occurred at the end of a turbulent decade for Berlin. On the same day, the President of the . (the German National Audit Office) criticised the city’s government for being around $46 Billion (DM 90 Billion) in debt (Schomaker 1999).

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Tamara M. Davis,David Parkinsonof a variety of social spheres to media logic and the primacy of media in everyday human activities. Ultimately, post-truth is governed by collective efforts to maximise the pleasure of encountering the world and attempts to set hegemonic benchmarks for such pleasure.978-3-319-97713-3

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Detecting Gravitational Waves from Supernovae with Advanced LIGO,tector status and perspectives, and the statistical methodology used to detect these transients are reviewed. While detection of gravitational waves from supernovae with Advanced LIGO is by no means guaranteed, plausible emission mechanisms offer significant discovery potential.

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Determining Amino Acid Chirality in the Supernova Neutrino Processing Model,uld have become enantiomeric. We have studied the capability of this model for selective destruction of one molecular chirality. Although some aspects of the model are speculative, tests may be possible to at least check the capability of this most basic aspect of the model.

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Diffuse Neutrino Flux from Supernovae,on facilities of tens of kilotons in mass, which will use water, liquid argon, and liquid scintillator and will implement important advancements in background rejection. Typical rates of detection will be ∼ 0.2–2 events per year. The potential of future DSNB observations to advance astrophysics and particle/nuclear physics is discussed briefly.