World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
122
Citations
100463
World Ranking
740
National Ranking
406

D. C. Coyne 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 D. C. Coyne 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: 360 publications — 30th percentile

30% of scientists in this discipline score the same or lower.

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

D. C. Coyne 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 D. C. Coyne 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: 122 D-Index — 80th percentile

80% of scientists in this discipline score the same or lower.

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

Research.com Recognitions

  • 2015 - Fellow of American Physical Society (APS) Citation For extraordinary engineering leadership in the construction of the Laser Interferometer Gravitationalwave Observatory LIGO Laboratory and the Advanced LIGO Detectors
  • 2007 - Fellow of the American Society of Mechanical Engineers

Overview

D. C. Coyne is affiliated with the California Institute of Technology in the United States and has contributed to the fields of Physics and Astronomy as well as Engineering. Their research spans subfields including Astronomy and Astrophysics, Ocean Engineering, and Atomic and Molecular Physics, and Optics.

Their work focuses on several core topics:

  • Pulsars and Gravitational Waves Research
  • Geophysics and Sensor Technology
  • Mechanical and Optical Resonators

Coyne's recent publication includes the paper titled A cryogenic silicon interferometer for gravitational-wave detection, published in 2020 in the journal Classical and Quantum Gravity. This work has garnered a citation count of 184.

Frequent collaborators in their research include:

  • R. X. Adhikari
  • K. Arai
  • A. F. Brooks
  • C Wipf
  • O Aguiar

The primary publication venue for Coyne is Classical and Quantum Gravity, which reflects at least one of their significant papers.

Coyne has received recognitions in their professional career, including:

  • Fellow of the American Physical Society (APS), awarded in 2015, with a citation for extraordinary engineering leadership in the construction of the Laser Interferometer Gravitational-wave Observatory (LIGO) Laboratory and the Advanced LIGO Detectors
  • Fellow of the American Society of Mechanical Engineers, awarded in 2007

Best Publications

  • Observation of Gravitational Waves from a Binary Black Hole Merger

    B. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • GW170817: observation of gravitational waves from a binary neutron star inspiral

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese

  • GW151226: observation of gravitational waves from a 22-solar-mass binary black hole coalescence

    B. P. Abbott;R. Abbott

  • Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese

  • GW170814: A three-detector observation of gravitational waves from a binary black hole coalescence

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese

  • GW170817: Measurements of Neutron Star Radii and Equation of State.

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese

  • Tests of general relativity with GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Binary Black Hole Mergers in the First Advanced LIGO Observing Run

    B. P. Abbott;R. Abbott

  • Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors

    J. Abadie;B. P. Abbott;R. Abbott;M. Abernathy

  • Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors

    J. Abadie;B. P. Abbott

  • Properties of the Binary Neutron Star Merger GW170817

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese

  • Binary Black Hole Mergers in the first Advanced LIGO Observing Run

    B. P. Abbott;R. Abbott

  • Exploring the Sensitivity of Next Generation Gravitational Wave Detectors

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light

    J. Aasi;J. Abadie;B. P. Abbott;R. Abbott

  • Characterization of the LIGO detectors during their sixth science run

    J. Aasi;J. Abadie;B. P. Abbott;R. Abbott

  • Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo

    B. P. Abbott;R. Abbott

  • Properties of the Binary Black Hole Merger GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$

    B. P. Abbott;R. Abbott

  • A gravitational wave observatory operating beyond the quantum shot-noise limit

    J. Abadie;B. P. Abbott;R. Abbott;T. D. Abbott

  • GW190521: A Binary Black Hole Merger with a Total Mass of 150 M

    R. Abbott;T. D. Abbott;S. Abraham;F. Acernese

Frequent Co-Authors

N. A. Robertson
N. A. Robertson California Institute of Technology
J. A. Giaime
J. A. Giaime Louisiana State University
Bruce Allen
Bruce Allen Max Planck Society
Alessandra Buonanno
Alessandra Buonanno Max Planck Institute for Gravitational Physics
Bernard F. Schutz
Bernard F. Schutz Cardiff University
Maria Alessandra Papa
Maria Alessandra Papa Max Planck Institute for Gravitational Physics
Karsten Danzmann
Karsten Danzmann Max Planck Institute for Gravitational Physics
Roman Schnabel
Roman Schnabel Universität Hamburg
David E. McClelland
David E. McClelland Australian National University

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