World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
98
Citations
59113
World Ranking
1727
National Ranking
912

Nicolas Regnault 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 Nicolas Regnault 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: 418 publications — 41st percentile

41% of scientists in this discipline score the same or lower.

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

Nicolas Regnault 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 Nicolas Regnault 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: 98 D-Index — 53rd percentile

53% of scientists in this discipline score the same or lower.

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

Overview

Nicolas Regnault is affiliated with Princeton University in the United States, with a research focus primarily in the fields of Physics and Astronomy as well as Materials Science. Their work spans several subfields including Atomic and Molecular Physics and Optics, Materials Chemistry, Condensed Matter Physics, Electrical and Electronic Engineering, and Statistical and Nonlinear Physics.

The scientist's research interests cover a range of topics, notably Topological Materials and Phenomena, Graphene Research and Applications, Quantum and Electron Transport Phenomena, Quantum Many-Body Systems, 2D Materials and Applications, Cold Atom Physics and Bose-Einstein Condensates, and Advanced Condensed Matter Physics.

Regnault has contributed extensively to scholarly literature, with frequent publications appearing in several key venues:

  • arXiv (Cornell University)
  • Physical Review B
  • Nature
  • Physical Review Letters
  • Zenodo (CERN European Organization for Nuclear Research)

Their most cited recent papers include:

  • "Quantum many-body scars and Hilbert space fragmentation: a review of exact results" (2022, Reports on Progress in Physics)
  • "High-throughput calculations of magnetic topological materials" (2020, Nature)
  • "Twisted bilayer graphene. IV. Exact insulator ground states and phase diagram" (2021, Physical Review B)
  • "Data for 'All Topological Bands of All Non-Magnetic Stoichiometric Materials'" (2022, Zenodo)
  • "Twisted bilayer graphene. III. Interacting Hamiltonian and exact symmetries" (2021, Physical Review B)

Their frequent coauthors include B. Andrei Bernevig, Zhida Song, Luis Elcoro, Jonah Herzog-Arbeitman, and Claudia Felser. Collaboration with these researchers reflects a significant interconnected network within the materials physics and condensed matter communities.

Best Publications

  • The CMS experiment at the CERN LHC

    S. Chatrchyan;G. Hmayakyan;V. Khachatryan;A. M. Sirunyan

  • LSST: from Science Drivers to Reference Design and Anticipated Data Products

    Željko Ivezić;Steven M. Kahn;J. Anthony Tyson;Bob Abel

  • The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda,and w from the First Year Data Set

    P. Astier;J. Guy;N. Regnault;R. Pain

  • New Constraints on $\Omega_M$, $\Omega_\Lambda$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST

    R. A. Knop;G. Aldering;R. Amanullah;P. Astier

  • Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

    M. Betoule;R. Kessler;J. Guy;J. Guy;J. Mosher

  • Improved Cosmological Constraints from New, Old and Combined Supernova Datasets

    M.Kowalski;D.Rubin;G.Aldering;R.J.Agostinho

  • Improved Cosmological Constraints from New, Old, and Combined Supernova Data Sets

    M. Kowalski;D. Rubin;D. Rubin;G. Aldering;R. J. Agostinho

  • LSST: From Science Drivers to Reference Design and Anticipated Data Products

    Željko Ivezić;Steven M. Kahn;J. Anthony Tyson;Bob Abel

  • SUPERNOVA CONSTRAINTS AND SYSTEMATIC UNCERTAINTIES FROM THE FIRST THREE YEARS OF THE SUPERNOVA LEGACY SURVEY

    A. Conley;A. Conley;J. Guy;M. Sullivan;N. Regnault

  • Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey

    A. Conley;J. Guy;M. Sullivan;N. Regnault

  • A complete catalogue of high-quality topological materials

    M. G. Vergniory;M. G. Vergniory;M. G. Vergniory;L. Elcoro;Claudia Felser;Nicolas Regnault

  • SALT2: using distant supernovae to improve the use of type Ia supernovae as distance indicators

    J. Guy;P. Astier;S. Baumont;D. Hardin

  • SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes

    M. Sullivan;J. Guy;A. Conley;N. Regnault

  • The (High Quality) Topological Materials In The World

    M. G. Vergniory;L. Elcoro;C. Felser;N. Regnault

  • The Supernova Legacy Survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints ,

    J. Guy;M. Sullivan;A. Conley;A. Conley;N. Regnault

  • SNLS3: Constraints on dark energy combining the supernova legacy survey three-year data with other probes

    M. Sullivan;J. Guy;A. Conley;A. Conley;N. Regnault

  • Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies

    M. Sullivan;D. Le Borgne;C. J. Pritchet;A. Hodsman

  • The dependence of Type Ia Supernovae luminosities on their host galaxies

    M. Sullivan;A. Conley;D. A. Howell;D. A. Howell;J. D. Neill

  • Fractional Chern Insulator

    N. Regnault;B. Andrei Bernevig

  • The Dependence of Type Ia Supernova Luminosities on their Host Galaxies

    M. Sullivan;A. Conley;D. A. Howell;J. D. Neill

Frequent Co-Authors

Mark Sullivan
Mark Sullivan University of Southampton
B. Andrei Bernevig
B. Andrei Bernevig Princeton University
Saul Perlmutter
Saul Perlmutter Lawrence Berkeley National Laboratory
Raymond G. Carlberg
Raymond G. Carlberg University of Toronto
Nathalie Palanque-Delabrouille
Nathalie Palanque-Delabrouille University of Paris-Saclay
Peter Nugent
Peter Nugent Lawrence Berkeley National Laboratory
W. M. Wood-Vasey
W. M. Wood-Vasey University of Pittsburgh
Richard S. Ellis
Richard S. Ellis University College London
Éric Aubourg
Éric Aubourg Université Paris Cité
Ariel Goobar
Ariel Goobar Stockholm University

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