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D. Hamilton

4 papers hereh-index 446.1k citations251 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • last author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • D. Hamilton — 3 papers
  • D. Hamilton — 2 papers, h 6
  • D. Hamilton — 1 paper, h 14
  • D. Hamilton — 1 paper, h 28

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20032008
most citedIntermediate Mass Black Hole Induced Quenching of Mass Segregation in Star Clusters

82 citations · 82 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph2008★ 82 cited

Intermediate Mass Black Hole Induced Quenching of Mass Segregation in Star Clusters

Michael Gill, Michele Trenti, M. Coleman Miller +3

In many theoretical scenarios it is expected that intermediate-mass black holes (IMBHs, with masses M ~ 100-10000 solar masses) reside at the centers of some globular clusters. How…

astro-ph2005

Three-Body Dynamics with Gravitational Wave Emission

Kayhan Gultekin, M. Coleman Miller, Douglas P. Hamilton

We present numerical three-body experiments that include the effects of gravitational radiation reaction by using equations of motion that include the 2.5-order post-Newtonian forc…

astro-ph2004

Growth of Intermediate-Mass Black Holes in Globular Clusters

Kayhan Gultekin, M. Coleman Miller, Douglas P. Hamilton

We present results of numerical simulations of sequences of binary-single scattering events of black holes in dense stellar environments. The simulations cover a wide range of mass…

astro-ph2003

Three-Body Encounters of Black Holes in Globular Clusters

Kayhan Gultekin, M. Coleman Miller, Douglas P. Hamilton

Evidence has been mounting for the existence of black holes with masses from 10^2 to 10^4 M_Solar associated with stellar clusters. Such intermediate-mass black holes (IMBHs) will…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.