World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
110
Citations
81380
World Ranking
1145
National Ranking
22

S. Caudill 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 S. Caudill 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: 312 publications — 20th percentile

20% of scientists in this discipline score the same or lower.

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

S. Caudill 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 S. Caudill 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: 110 D-Index — 69th percentile

69% of scientists in this discipline score the same or lower.

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

Overview

S. Caudill is affiliated with the National Institute for Subatomic Physics in the Netherlands. Their research primarily centers around physics and astronomy, with a significant emphasis on subfields such as astronomy and astrophysics, atomic and molecular physics and optics, oceanography, and nuclear and high energy physics.

Their work covers a range of main topics including pulsars and gravitational waves research, geophysics and gravity measurements, mechanical and optical resonators, advanced frequency and time standards, cold atom physics and Bose-Einstein condensates, astrophysical phenomena and observations, and magnetic confinement fusion research.

S. Caudill has contributed to several publications spanning multiple venues. Frequent publication venues include:

  • Journal of Physics Conference Series
  • Physical Review Letters
  • Archivio Istituzionale della Ricerca (Universita Degli Studi Di Milano)
  • Classical and Quantum Gravity

Collaborations have been an integral part of Caudill's research output. Notable frequent co-authors include:

  • A. Allocca
  • A. Amato
  • N. Arnaud
  • P. Astone
  • G. Ballardin

Recent significant publications by S. Caudill include:

  • "Quantum Backaction on Kg-Scale Mirrors: Observation of Radiation Pressure Noise in the Advanced Virgo Detector", 2020, Physical Review Letters
  • "Calibration of advanced Virgo and reconstruction of the detector strain h( t) during the observing run O3", 2022, Archivio Istituzionale della Ricerca (Universita Degli Studi Di Milano)
  • "Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector", 2023, Physical Review Letters
  • "Advanced Virgo Status", 2020, Journal of Physics Conference Series
  • "Advanced Virgo Plus: Future Perspectives", 2023, Journal of Physics Conference Series

Their research predominantly involves experimental and observational aspects of gravitational wave detectors, resonators, and related physical phenomena. The body of work reflects engagement with instrumentation calibration, noise characterization, advancements in squeezed vacuum states for detectors, and future perspectives of projects such as Advanced Virgo.

Best Publications

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

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

  • 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

  • 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

  • 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

  • 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

  • Properties of the Binary Neutron Star Merger GW170817

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

  • Characterization of the LIGO detectors during their sixth science run

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

  • A gravitational-wave standard siren measurement of the Hubble constant

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

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

    B. P. Abbott;R. Abbott

  • 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

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

    B. P. Abbott

  • GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object

    R. Abbott;T. D. Abbott

  • Exploring the Sensitivity of Next Generation Gravitational Wave Detectors

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

Frequent Co-Authors

N. A. Robertson
N. A. Robertson California Institute of Technology
Alessandra Buonanno
Alessandra Buonanno Max Planck Institute for Gravitational Physics
J. A. Giaime
J. A. Giaime Louisiana State University
Nelson Christensen
Nelson Christensen Observatoire de la Côte d’Azur
Bruce Allen
Bruce Allen Max Planck Society
Bernard F. Schutz
Bernard F. Schutz Cardiff University
Roman Schnabel
Roman Schnabel Universität Hamburg
Patrick Brady
Patrick Brady University of Wisconsin–Milwaukee
G. Bergmann
G. Bergmann Max Planck Society

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