G
Gabriel Martínez-Pinedo
Researcher at Technische Universität Darmstadt
Publications - 373
Citations - 18118
Gabriel Martínez-Pinedo is an academic researcher from Technische Universität Darmstadt. The author has contributed to research in topics: Nucleosynthesis & Supernova. The author has an hindex of 66, co-authored 360 publications receiving 15707 citations. Previous affiliations of Gabriel Martínez-Pinedo include GSI Helmholtz Centre for Heavy Ion Research & Aarhus University.
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Journal ArticleDOI
Electromagnetic counterparts of compact object mergers powered by the radioactive decay of r‐process nuclei
Brian D. Metzger,Gabriel Martínez-Pinedo,Swaroop Darbha,Eliot Quataert,Almudena Arcones,Daniel Kasen,R. C. Thomas,Peter Nugent,I. V. Panov,I. V. Panov,Nikolaj Thomas Zinner +10 more
TL;DR: In this paper, the authors present the first calculations of the optical transients from compact object mergers that self-consistently determine the radioactive heating by means of a nuclear reaction network; using this heating rate, they model the light curve with a one-dimensional Monte Carlo radiation transfer calculation.
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The shell model as a unified view of nuclear structure
TL;DR: In this article, the Lanczos tridiagonal construction has been used to diagonalize matrices in determinantal spaces of dimensionality up to 10^9 using the Shell Model.
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Theory of core-collapse supernovae
TL;DR: In this paper, it was shown that the prompt bounce-shock mechanism is not the driver of supernova explosions, and that the delayed neutrino-heating mechanism can produce explosions without the aid of multi-dimensional processes only if the progenitor star has an ONeMg core inside a very dilute He-core, i.e., has a mass in the 8-10 M⊙ range.
Journal ArticleDOI
Theory of Core-Collapse Supernovae
TL;DR: In this paper, it was shown that the prompt bounce-shock mechanism is not the driver of supernova explosions, and that the delayed neutrino-heating mechanism can produce explosions without the aid of multi-dimensional processes only if the progenitor star has an ONeMg core inside a very dilute He-core.
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Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45−65 in supernovae environments
TL;DR: In this paper, the electron capture, positron capture and beta-decay rates for more than 100 nuclei in the mass range A=45 −65 were determined based on large-scale shell-model calculations.