M
M. Coleman Miller
Researcher at University of Maryland, College Park
Publications - 305
Citations - 14363
M. Coleman Miller is an academic researcher from University of Maryland, College Park. The author has contributed to research in topics: Neutron star & Black hole. The author has an hindex of 68, co-authored 293 publications receiving 12880 citations. Previous affiliations of M. Coleman Miller include University of Copenhagen & Johns Hopkins University.
Papers
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Journal ArticleDOI
Identifying ultrahigh-energy cosmic-ray accelerators with future ultrahigh-energy neutrino detectors
Ke Fang,Ke Fang,Kumiko Kotera,Kumiko Kotera,M. Coleman Miller,M. Coleman Miller,Kohta Murase,Kohta Murase,Foteini Oikonomou +8 more
TL;DR: In this paper, the authors investigate the ability of a future UHE neutrino detector to identify the brightest Neutrino point sources, by exploring the parameter space of the total number of observed events and the angular resolution of the detector.
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Constraints on alternatives to supermassive black holes
TL;DR: In this paper, it was shown that the keyhole through which alternatives to supermassive black holes must pass is substantially smaller and more contrived than it was even a few years ago.
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Gravitational Lensing Limits on the Average Redshift of Gamma-Ray Bursts
TL;DR: In this paper, an upper limit to the average redshift of gamma-ray burst (GRB) is derived, independent of the physical model for GRBs, using a new statistical lensing method that removes distance ambiguities and thus permits accurate computation of the lensing rate at high z.
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Suppression of Gravitational Structure Formation by Cosmological Accretion Heating
TL;DR: In this paper, the authors consider the effects of ionization sources on the cosmic microwave background power spectrum and show that if an ionization source exists, then it would also heat the universe, hence increasing the Jeans mass and suppressing early gravitational structure formation.
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An upper limit to the velocity dispersion of relaxed stellar systems without massive black holes
TL;DR: In this article, it was shown that massive central black holes can form in relaxed stellar systems at any cosmic epoch, and that the accretion rate after disruption is many orders of magnitude above Eddington.