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Physics
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2026

D-Index & Metrics

Physics

D-Index
168
Citations
160720
World Ranking
155
National Ranking
101

Robert L. Byer 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 Robert L. Byer 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: 1,238 publications — 95th percentile

95% of scientists in this discipline score the same or lower.

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

Robert L. Byer 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 Robert L. Byer 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: 168 D-Index — 96th percentile

96% 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

  • 2026 - Research.com Physics in United States Leader Award
  • 2012 - Fellow, National Academy of Inventors
  • 2009 - Frederic Ives Medal, The Optical Society For pioneering contributions to optical science and the commercial development of optical technologies and for wide-ranging leadership activities within the optics community.
  • 2000 - Member of the National Academy of Sciences
  • 1992 - Fellow of the American Association for the Advancement of Science (AAAS)
  • 1991 - Fellow of American Physical Society (APS) Citation For fundamental contributions to the development and application of stable, tunable solid state laser sources and to nonlinear optical phenomena such as four wave mixing and harmonic generation
  • 1987 - Member of the National Academy of Engineering For major contributions to the science and technology of nonlinear optics.
  • 1987 - IEEE Fellow For major contributions to laser, nonlinear optics, and spectroscopy.
  • 1974 - Fellow of Alfred P. Sloan Foundation

Overview

Robert L. Byer is affiliated with Stanford University in the United States. Their research spans multiple areas within physics and engineering, focusing heavily on optics and photonics technologies. The main fields of study for Byer include Physics and Astronomy as well as Engineering, with specific attention to the subfields of Atomic and Molecular Physics, and Optics; Electrical and Electronic Engineering; and Nuclear and High Energy Physics.

Byer's work covers a range of scientific topics including Laser-Plasma Interactions and Diagnostics, Ga2O3 and related materials, Photonic and Optical Devices, and Advanced Electron Microscopy Techniques and Applications. Additional interests encompass Laser-Matter Interactions and Applications, Advanced X-ray Imaging Techniques, and Advanced Fiber Laser Technologies.

Frequent collaborators in Byer's research include Dylan S. Black, Yu Miao, Kenneth J. Leedle, Olav Solgaard, and Zhexin Zhao.

Recent published papers by Byer or involving them address developments relevant to advanced optics and photonics. These include:

  • A cryogenic silicon interferometer for gravitational-wave detection, 2020, Classical and Quantum Gravity
  • Gallium Oxide for High-Power Optical Applications, 2020, Advanced Optical Materials
  • Miniature light-driven nanophotonic electron acceleration and control, 2022, Advances in Optics and Photonics
  • Quantum Nature of Dielectric Laser Accelerators, 2021, Physical Review X
  • A compact electron source for the dielectric laser accelerator, 2020, Applied Physics Letters

The venues where Byer frequently publishes include the Conference on Lasers and Electro-Optics, arXiv (Cornell University), Advanced Optical Materials, Physical Review Letters, and Classical and Quantum Gravity. These platforms reflect a strong emphasis on laser technology, nonlinear optics, and cutting-edge developments in photonics.

Byer has received multiple professional recognitions including election to the National Academy of Sciences (2000) and the National Academy of Engineering (1987). Other honors include Fellowships in the American Association for the Advancement of Science, American Physical Society, Alfred P. Sloan Foundation, and the National Academy of Inventors. The IEEE recognized Byer as a Fellow for contributions to laser, nonlinear optics, and spectroscopy. Additionally, the Optical Society awarded Byer the Frederic Ives Medal in 2009 for contributions to optical science and commercial technology development.

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

  • GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

    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

  • Quasi-phase-matched second harmonic generation: tuning and tolerances

    M.M. Fejer;G.A. Magel;D.H. Jundt;R.L. Byer

  • GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

    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

  • Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

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

  • 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

  • Quasi-phase-matched optical parametric oscillators in bulk periodically poled LiNbO 3

    L. E. Myers;R. C. Eckardt;M. M. Fejer;R. L. Byer

  • 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

  • GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence

    B. P. Abbott;R. Abbott

  • GW170608: Observation of a 19 solar-mass binary black hole coalescence

    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

  • 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

Frequent Co-Authors

N. A. Robertson
N. A. Robertson California Institute of Technology
Martin M. Fejer
Martin M. Fejer Stanford University
J. A. Giaime
J. A. Giaime Louisiana State University
Bernard F. Schutz
Bernard F. Schutz Cardiff University
Alessandra Buonanno
Alessandra Buonanno Max Planck Institute for Gravitational Physics
Nelson Christensen
Nelson Christensen Observatoire de la Côte d’Azur
J. H. Hough
J. H. Hough University of Glasgow
Laura Cadonati
Laura Cadonati Georgia Institute of Technology
Rana X. Adhikari
Rana X. Adhikari California Institute of Technology

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