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361por Robinson, Keith“…Can we know which stars will go supernova and which will end up as white dwarfs or black holes? …”
Publicado 2009
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362“…Skies are recreated to display critical events as they would have appeared to ancient observers—events such as the supernova of 1054 A.D., the "lion horoscope," and the Star of Bethlehem. …”
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363“…It is effectively demonstrated that processes of neutrino interactions with active media of astrophysical objects may lead, under some physical conditions, to such interesting effects as neutrino-driven shockwave revival in a supernova explosion, a “cherry stone shooting” mechanism for pulsar natal kick, and a neutrino pulsar. …”
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364por Verschuur, Gerrit“…This is the story of radio astronomy, of how radio waves are generated by stars, supernova, quasars, colliding galaxies and by the very beginnings of the universe itself. …”
Publicado 2015
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365por Brailsford, Dominic“…Moreover, DUNE will be sensitive to the electron neutrino flux from a core-collapse supernova, providing valuable information on the phenomenon's underlying mechanisms. …”
Publicado 2018
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366por Wang, Xilu, Clark, Adam M., Ellis, John, Ertel, Adrienne F., Fields, Brian D., Fry, Brian J., Liu, Zhenghai, Miller, Jesse A., Surman, Rebecca“…244Pu has recently been discovered in deep-sea deposits spanning the past 10 Myr, a period that includes two 60Fe pulses from nearby supernovae. 244Pu is among the heaviest $r$-process products, and we consider whether it was created in the supernovae, which is disfavored by nucleosynthesis simulations, or in an earlier kilonova event that seeded 244Pu in the nearby interstellar medium that was subsequently swept up by the supernova debris. …”
Publicado 2021
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367por Badertscher, Andreas“…The physics program of the collaboration is to study neutrino oscillations with the long base line neutrino beam from CERN to the Gran Sasso laboratory (CNGS), atmospheric, solar and supernova neutrinos, and a sensitive search for nucleon decays. …”
Publicado 2004
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368por Görres, Joachim“…Two examples are presented to illustrate this interplay: the measurement of the lifetime of (44)Ti to allow an improved determination of the (44)Ti mass of the supernova remnant Cassiopeia A from the observed γ ray activity and the measurements of excited states in (24)Si to determine the reaction rate of (23)Al(p, γ)(24)Si which might be important for a reduced production of (22)Na in novae.…”
Publicado 2000
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369“…In the CB model the process leading to the ejection of highly relativistic jetted CBs in core-collapse supernova (SN) explosions is akin to the one observed in quasars and microquasars. …”
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370por Coombe, Lauren, Zhang, Jessica, Vandervalk, Benjamin P., Chu, Justin, Jackman, Shaun D., Birol, Inanc, Warren, René L.“…Following ARKS scaffolding of a human genome 10xG Supernova assembly (of cell line NA12878), fewer than 9 scaffolds cover each chromosome, except the largest (chromosome 1, n = 13). …”
Publicado 2018
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371“…These non-magnetized detectors have a rich physics program outside the context of a neutrino factory, including topics like supernova neutrinos and proton decay. Hence, our observation opens the possibility to use a multi-purpose detector also in a neutrino factory beam.…”
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372“…The proposed decoherence may partially explain the results of Gallium detector calibrations and it can strongly affect supernova neutrino signals.…”
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373por Bisnovatyi-Kogan, Gennady S“…This second edition is carefully updated in the areas of pre-supernova models, magnetorotational supernovae, and the theory of accretion disks around black holes. …”
Publicado 2011
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374por Kyrala, G.A“…The conference brought together different scientists interested in this emerging new filed, with topics covering: - Hydrodynamic instabilities in astrophysics, - Supernovae and supernova remnant evolution, - Aastrophysical shocks, blast waves, and jets, - Stellar opacities, - Radiation and thermal transport, - Dense plasma atomic physics and EOS - X-ray photoionized plasmas, - Ultrastrong magnetic field generation Reprinted from Astrophysics and Space Science, volume 298, Nos. 1-2, 2005…”
Publicado 2005
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375por Close, Frank“…He may be considered the father of neutrino astronomy with his successful prediction that neutrinos from a supernova could be detected, but contrary to widespread folklore, the idea of solar neutrinos did not originate with him. …”
Publicado 2016
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376por McLeod, Alexus“…He then goes on to explore the contemporary understanding of supernovae, contrasting it with that of the ancient Americas. …”
Publicado 2016
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377por Sofue, Yoshiaki“…In addition, more advanced topics relevant to the Galaxy and galaxies are also contained here: star formation, supernova remnants, the Galactic Center and black holes, galactic dynamics and dark-matter halos, magnetism of galaxies, interstellar gases in galaxies, and starbursts. …”
Publicado 2017
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378por Klapdor-Kleingrothaus, H V, Hillebrandt, W, Metzinger, J, Oda, T, Thielemann, F K“…The heavy element synthesis by explosive He burning then is calculated using these beta -rates and using realistic star models treating the supernova explosion hydrodynamically. It is shown that-as a consequence of the revised beta -decay rates-explosive He burning seems at present to be the most convincing site of an r-process leading to a solar r-element distribution in one event. (77 refs).…”
Publicado 1981
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379por Marrocchesi, P S, Ahn, H S, Bagliesi, M G, Basti, A, Bigongiari, G, Castellina, A, Ganel, O, Lee, M H, Lomtadze, T A, Lutz, L, Maestro, P, Malinine, A, Meucci, M, Millucci, V, Morsani, F, Seo, E S, Zinn, S Y“…Cosmic Ray Energetics And Mass (CREAM) is a balloon-borne experiment designed to perform direct measurements of cosmic ray composition over the elemental range from proton to iron to the supernova energy scale of 10 **1**5eV in a series of balloon flights using the new Ultra Long Duration Balloon (ULDB) capability under development by NASA. …”
Publicado 2004
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380por Sipos, Roland“…Therefore, real-time processing of the data stream for hit and trigger primitive finding is essential for the requirement of continuous readout. The supernova burst trigger requires a large and fast buffering technique, where 3D XPoint persistent memory solutions are evaluated and integrated. …”
Publicado 2020
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