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Joel R. Primack

Researcher at University of California, Santa Cruz

Publications -  492
Citations -  55170

Joel R. Primack is an academic researcher from University of California, Santa Cruz. The author has contributed to research in topics: Galaxy & Galaxy formation and evolution. The author has an hindex of 101, co-authored 483 publications receiving 50646 citations. Previous affiliations of Joel R. Primack include Stanford University & Harvard University.

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CANDELS Meets GSWLC: Evolution of the Relationship between Morphology and Star Formation Since z = 2

TL;DR: In this article, the relationship between morphology and star formation has been studied by using consistent SED fitting with flexible dust attenuation laws, and it was shown that the clumpy disk contribution to the star formation budget peaks at z ~ 1, rather than z ~ 2, suggesting that the principal epoch of disk assembly continues to lower redshift.
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Space Reactor Arms Control: Overview

TL;DR: A working group associated with the Federation of American Scientists (FAS) and the Committee of Soviet Scientists for Peace and Against the Nuclear Threat (CSS) has been studying a proposed ban on orbiting reactors.
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A Little Hot Dark Matter Matters

TL;DR: In this paper, the authors discuss the nature of the hot dark matter, which may consist of neutrinos with mass, and the one that best agrees with the data is a model in which the universe is made of 70% cold dark matter.
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Radiogenic Heating and its Influence on Rocky Planet Dynamos and Habitability

TL;DR: In this paper, the authors discuss the effects of these variations on the thermal evolution of an Earth-size planet, using a 1D parameterized convection model, and find that Earth had just enough radiogenic heating to maintain a persistent dynamo.
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Status of Cold Dark Matter Cosmology

TL;DR: The cold dark matter (CDM) theory has become the standard modern theory of cosmological structure formation as discussed by the authors. But despite its many successes, there has been concern about CDM on small scales because of the possible contradiction between the linearly rising rotation curves observed in some dark-matter-dominated galaxies vs the $1/r$ density cusps at the centers of simulated CDM halos.