J
John F. Beacom
Researcher at Ohio State University
Publications - 359
Citations - 28360
John F. Beacom is an academic researcher from Ohio State University. The author has contributed to research in topics: Neutrino & Supernova. The author has an hindex of 80, co-authored 338 publications receiving 24601 citations. Previous affiliations of John F. Beacom include Fermilab & University of Wisconsin-Madison.
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The Southern Wide-Field Gamma-Ray Observatory (SWGO): A Next-Generation Ground-Based Survey Instrument for VHE Gamma-Ray Astronomy
P. Abreu,A. Albert,Ruben Alfaro,C. Alvarez,R. Arceo,Pedro Assis,Fernando Barão,J.L. Bazo,John F. Beacom,Jose A. Bellido,S. Y. BenZvi,Thomas Bretz,Chad Brisbois,A. M. Brown,Francois Brun,Mario Buscemi,K. S. Caballero Mora,P. Camarri,A. Carraminana,Sabrina Casanova,Andrea Chiavassa,R. Conceição,Garret Cotter,P. Cristofari,Sergio Dasso,A. De Angelis,M. De Maria,P. Desiati,G. Di Sciascio,J. C. Díaz Vélez,Claudio O. Dib,Brenda Dingus,Daniela Dorner,Michele Doro,Connor Duffy,Michael DuVernois,R. Engel,M. Fernandez Alonso,Henrike Fleischhack,P. Fonte,Nissim Illich Fraija,Stefan Funk,Jose Andres Garcia-Gonzalez,M. J. Martínez González,J. A. Goodman,T. Greenshaw,J. P. Harding,A. Haungs,Binita Hona,P. Huentemeyer,A. Insolia,Armelle Jardin-Blicq,V. Joshi,K. Kawata,Samridha Kunwar,G. La Mura,Jonathan S. Lapington,J.-P. Lenain,R. López-Coto,Kelly Malone,Jesús Martínez-Castro,H. Martínez-Huerta,L. Mendes,E. Moreno,Miguel Mostafa,K. C. Y. Ng,M. U. Nisa,F. Peron,A. Pichel,M. Pimenta,E. Prandini,S. Rainò,Andreas Reisenegger,J. L. Rodriguez,Markus Roth,A. C. Rovero,Edna Ruiz-Velasco,T. Sako,A. Sandoval,Marcos Santander,Konstancja Satalecka,M. Schneider,Harm Schoorlemmer,F. Schüssler,R. C. Shellard,Andrew Smith,Samuel Timothy Spencer,W. Springer,Pooja Surajbali,K. Tollefson,B. Tome,Ibrahim Torres,A. Viana,Thomas Weisgarber,R. Wischnewski,A. Zepeda,Bei Zhou,Hao Zhou +97 more
TL;DR: Plans for the development of the Southern Wide-field Gamma-ray Observatory (SWGO), a next-generation instrument with sensitivity to the very-high-energy (VHE) band to be constructed in the Southern Hemisphere, are described.
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New experimental constraints in a new landscape for composite dark matter
TL;DR: Recently, it was shown that strongly interacting dark matter is still theoretically possible for composite particles, with much parameter space open as discussed by the authors, and a wide range of wide-ranging limits based on data from a novel detector at the University of Chicago.
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Effects of stellar rotation on star formation rates and comparison to core-collapse supernova rates
Shunsaku Horiuchi,Shunsaku Horiuchi,John F. Beacom,Matt Bothwell,Matt Bothwell,Todd A. Thompson +5 more
TL;DR: In this paper, the authors investigate star formation rate (SFR) calibrations in light of recent developments in the modeling of stellar rotation and find that the estimated SFR for the rotating stellar population is 30% smaller than for the non-rotating stellar population, and 40% smaller for the Halpha to SFR calibration.
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Very-high-energy gamma-ray signal from nuclear photodisintegration as a probe of extragalactic sources of ultrahigh-energy nuclei
TL;DR: In this paper, the authors predict a diagnostic gamma-ray signal, unique to nuclei, which is the emission of deexcitation gamma rays following photodisintegration, which can be used to identify and study individual ultrahigh-energy nuclei accelerators.
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Dark Matter Velocity Spectroscopy.
TL;DR: In this paper, velocity spectroscopy was used to separate dark matter decays or annihilations that produce linelike spectra may be smoking-gun signals with minimal theoretical uncertainties.