J
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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Journal ArticleDOI
Quenching as a Contest between Galaxy Halos and Their Central Black Holes
Zhu Chen,S. M. Faber,David C. Koo,Rachel S. Somerville,Rachel S. Somerville,Joel R. Primack,Avishai Dekel,Aldo Rodríguez-Puebla,Yicheng Guo,Guillermo Barro,Dale D. Kocevski,A. van der Wel,A. van der Wel,Joanna Woo,Joanna Woo,Eric F. Bell,Jerome J. Fang,Henry C. Ferguson,Mauro Giavalisco,Marc Huertas-Company,Fangzhou Jiang,Susan A. Kassin,Lin Lin,Fengshan Liu,Fengshan Liu,Yifei Luo,Zhijian Luo,Camilla Pacifici,Viraj Pandya,Samir Salim,Chenggang Shu,Sandro Tacchella,Bryan A. Terrazas,Hassen M. Yesuf +33 more
TL;DR: In this paper, it was shown that the evolutionary tracks of star-forming galaxies are nearly parallel to the green-valley boundaries, and it is mainly the sideways motions of these boundaries with cosmic time that cause galaxies to quench.
Dark Matter and Structure Formation
TL;DR: Dekel and Ostriker as mentioned in this paper presented an introduction to current research on the nature of the cosmological dark matter and the origin of galaxies and large scale structure within the standard theoretical framework.
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Small-Scale Power Spectrum and Correlations in Lambda + Cold Dark Matter Models
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Finite Temperature Radiative Corrections to Neutron Decay and Related Processes
TL;DR: In this article, a detailed calculation of the radiative corrections at finite temperature to the processes n ν ↔ pe, ne ↔ p ν and n Δ pe ν is presented.
Journal ArticleDOI
Predicting the properties of the remnants of dissipative galaxy mergers
Matthew D. Covington,Avishai Dekel,Avishai Dekel,Thomas J. Cox,Patrik Jonsson,Joel R. Primack +5 more
TL;DR: In this paper, a physically motivated model for predicting the properties of the remnants of gaseous galaxy mergers is presented, which is calibrated using a large suite of smoothed particle hydrodynamics (SPH) merger simulations.