World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
86
Citations
23073
World Ranking
2549
National Ranking
1264

M. Coleman Miller publication distribution in Physics in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where M. Coleman Miller sits on this spectrum.

103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103 publications 1,469+

This scientist: 367 publications — 31st percentile

31% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

M. Coleman Miller D-index placement in Physics in 2026

The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where M. Coleman Miller sits on this spectrum.

70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70 D-Index 185+

This scientist: 86 D-Index — 32nd percentile

32% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

Overview

M. Coleman Miller is affiliated with the University of Maryland, College Park in the United States. Their research spans primarily the field of Physics and Astronomy with a significant focus on subfields such as Astronomy and Astrophysics, Nuclear and High Energy Physics, Oceanography, Geophysics, and Atomic and Molecular Physics, and Optics.

The scientist's main topics of work include:

  • Pulsars and Gravitational Waves Research
  • Gamma-ray bursts and supernovae
  • Astrophysical Phenomena and Observations
  • Geophysics and Gravity Measurements
  • Astrophysics and Cosmic Phenomena
  • High-pressure geophysics and materials
  • Radio Astronomy Observations and Technology

Miller has published extensively in several venues, particularly:

  • arXiv (Cornell University) with 21 publications
  • The Astrophysical Journal with 7 publications
  • Monthly Notices of the Royal Astronomical Society with 5 publications
  • The Astrophysical Journal Letters with 5 publications
  • Zenodo (CERN European Organization for Nuclear Research) with 4 publications

Frequent co-authors in Miller's work include:

  • Alexander J. Dittmann
  • Sébastien Guillot
  • Slavko Bogdanov
  • Zaven Arzoumanian
  • Wynn C. G. Ho

Notable recent papers authored or co-authored by Miller include:

  • "Astrophysics with the Laser Interferometer Space Antenna," 2023, Archivio Istituzionale della Ricerca (Universita Degli Studi Di Milano)
  • "Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes," 2020, Springer Link (Chiba Institute of Technology)
  • "A very luminous jet from the disruption of a star by a massive black hole," 2022, Nature
  • "The Radius of PSR J0740+6620 from NICER with NICER Background Estimates," 2022, The Astrophysical Journal
  • "Electromagnetic counterparts to massive black-hole mergers," 2022, Living Reviews in Relativity

Best Publications

  • The Radius of PSR J0740+6620 from NICER and XMM-Newton Data

    M. C. Miller;F. K. Lamb;A. J. Dittmann;S. Bogdanov

  • Sonic-Point Model of Kilohertz Quasi-periodic Brightness Oscillations in Low-Mass X-Ray Binaries

    M. Coleman Miller;Frederick K. Lamb;Dimitrios Psaltis;Dimitrios Psaltis

  • Intermediate - mass black holes

    M. Coleman Miller;E. J. M. Colbert

  • Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA

    Pau Amaro-Seoane;Jonathan R Gair;Marc Freitag;M Coleman Miller

  • Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions

    T. Klähn;T. Klähn;D. Blaschke;S. Typel;E. N. E. van Dalen

  • PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

    M. C. Miller;F. K. Lamb;A. J. Dittmann;S. Bogdanov

  • Production of intermediate-mass black holes in globular clusters

    M. Coleman Miller;Douglas P. Hamilton

  • X-ray Spectroscopic Evidence for Intermediate Mass Black Holes: Cool Accretion Disks in Two Ultra--Luminous X-ray Sources

    J. M. Miller;G. Fabbiano;M. C. Miller;A. C. Fabian

  • X-Ray Spectroscopic Evidence for Intermediate-Mass Black Holes: Cool Accretion Disks in Two Ultraluminous X-Ray Sources

    J. M. Miller;J. M. Miller;G. Fabbiano;M. C. Miller;A. C. Fabian

  • Colloquium: Measuring the neutron star equation of state using x-ray timing

    Anna L. Watts;Nils Andersson;Deepto Chakrabarty;Marco Feroci

  • Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes

    K. Belczynski;J. Klencki;C. E. Fields;A. Olejak;A. Olejak

  • Alignment of the spins of supermassive black holes prior to coalescence

    Tamara Bogdanović;Christopher S. Reynolds;M. Coleman Miller

  • A Unified Model for Tidal Disruption Events

    Lixin Dai;Lixin Dai;Jonathan C. McKinney;Nathaniel Roth;Enrico Ramirez-Ruiz;Enrico Ramirez-Ruiz

  • Distinguishing spin-aligned and isotropic black hole populations with gravitational waves

    Will M. Farr;Simon Stevenson;Simon Stevenson;M. Coleman Miller;Ilya Mandel;Ilya Mandel

  • A Comparison of Intermediate Mass Black Hole Candidate ULXs and Stellar-Mass Black Holes

    J. M. Miller;A. C. Fabian;M. C. Miller

  • FOUR-BODY EFFECTS IN GLOBULAR CLUSTER BLACK HOLE COALESCENCE

    M. Coleman Miller;Douglas P. Hamilton

  • The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes

    K. Belczynski;J. Klencki;C.E. Fields;A. Olejak

  • Thorium abundances on the lunar surface

    D. J. Lawrence;W. C. Feldman;B. L. Barraclough;A. B. Binder

  • Getting a Kick Out of Numerical Relativity

    John G. Baker;Joan Centrella;Dae-Il Choi;Dae-Il Choi;Michael Koppitz

  • The Large Observatory For X-ray Timing: LOFT

    M. Feroci;L. Stella;M. van der Klis;T. J.-L. Courvoisier

Frequent Co-Authors

Didier Barret
Didier Barret Federal University of Toulouse Midi-Pyrénées
Christopher S. Reynolds
Christopher S. Reynolds University of Cambridge
Dimitrios Psaltis
Dimitrios Psaltis University of Arizona
Tod E. Strohmayer
Tod E. Strohmayer Goddard Space Flight Center
Ilya Mandel
Ilya Mandel Monash University
Jonathan R. Gair
Jonathan R. Gair Max Planck Society
Alessandra Buonanno
Alessandra Buonanno Max Planck Institute for Gravitational Physics
Alexander Heger
Alexander Heger Monash University
Nicolás Yunes
Nicolás Yunes University of Illinois at Urbana-Champaign
Paul S. Ray
Paul S. Ray United States Naval Research Laboratory

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