activity
20022019
most citedFour-Body Effects in Globular Cluster Black Hole Coalescence

250 citations · 1.4k across the 13 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2019★ 76 cited

Star Formation in Accretion Disks and SMBH Growth

Alexander J. Dittmann, M. Coleman Miller

Accretion disks around active galactic nuclei are potentially unstable to star formation at large radii. We note that when the compact objects formed from some of these stars spira…

astro-ph.HE2016★ 28 cited

Energetic constraints on electromagnetic signals from double black hole mergers

Lixin Dai, Jonathan C. McKinney, M. Coleman Miller

The possible Fermi detection of an electromagnetic counterpart to the double black hole merger GW150914 has inspired many theoretical models, some of which propose that the holes s…

astro-ph.HE2016★ 34 cited

Identifying Ultrahigh-Energy Cosmic-Ray Accelerators with Future Ultrahigh-Energy Neutrino Detectors

Ke Fang, Kumiko Kotera, M. Coleman Miller +2

The detection of ultrahigh-energy (UHE) neutrino sources would contribute significantly to solving the decades-old mystery of the origin of the highest-energy cosmic rays. We inves…

astro-ph.HE2016★ 128 cited

The Role of the Kozai-Lidov Mechanism in Black Hole Binary Mergers in Galactic Centers

John H. VanLandingham, M. Coleman Miller, Douglas P. Hamilton +1

In order to understand the rate of merger of stellar-mass black hole binaries (BHBs) by gravitational wave (GW) emission it is important to determine the major pathways to merger.…

astro-ph.HE2013

Astrophysical Constraints on Dense Matter in Neutron Stars

M. Coleman Miller

Ever since the discovery of neutron stars it has been realized that they serve as probes of a physical regime that cannot be accessed in laboratories: strongly degenerate matter at…

astro-ph.HE2013★ 76 cited

Alignment of supermassive black hole binary orbits and spins

M. Coleman Miller, Julian H. Krolik

Recent studies of accretion onto supermassive black hole binaries suggest that much, perhaps most, of the matter eventually accretes onto one hole or the other. If so, then for bin…