World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
109
Citations
125781
World Ranking
1178
National Ranking
615

Saul Perlmutter 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 Saul Perlmutter 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: 792 publications — 84th percentile

84% of scientists in this discipline score the same or lower.

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

Saul Perlmutter 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 Saul Perlmutter 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: 109 D-Index — 68th percentile

68% 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 - Breakthrough Prize in Fundamental Physics For the most unexpected discovery that the expansion of the universe is accelerating, rather than slowing as had been long assumed.
  • 2011 - Nobel Prize for the discovery of the accelerating expansion of the Universe through observations of distant supernovae
  • 2007 - Fellow of the American Academy of Arts and Sciences
  • 2003 - Fellow of the American Association for the Advancement of Science (AAAS)
  • 2002 - Member of the National Academy of Sciences
  • 2000 - Fellow of American Physical Society (APS) Citation For pioneering contributions to cosmology, including development of new search techniques that led to discovery of numerous distant supernovae and strong evidence for the accelerated expansion of the universe

Overview

Saul Perlmutter is affiliated with the Lawrence Berkeley National Laboratory in the United States. Their research primarily focuses on physics and astronomy, with significant contributions in the subfields of astronomy and astrophysics, instrumentation, nuclear and high energy physics, atomic and molecular physics, and optics, as well as artificial intelligence.

The main topics covered in their work include gamma-ray bursts and supernovae, astronomy and astrophysical research, stellar, planetary, and galactic studies, astrophysics and cosmic phenomena, neutrino physics research, pulsars and gravitational waves research, and various astrophysical phenomena and observations.

Their recent publications include the following papers:

  • Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework, 2023, arXiv (Cornell University)
  • Protecting scientific integrity in an age of generative AI, 2024, Proceedings of the National Academy of Sciences
  • Carnegie Supernova Project II: The Slowest Rising Type Ia Supernova LSQ14fmg and Clues to the Origin of Super-Chandrasekhar/03fg-like Events, 2020, The Astrophysical Journal
  • Accuracy of environmental tracers and consequences for determining the Type Ia supernova magnitude step, 2021, Astronomy and Astrophysics
  • The Twins Embedding of Type Ia Supernovae. II. Improving Cosmological Distance Estimates, 2021, The Astrophysical Journal

Frequent co-authors in their research collaborations include:

  • G. Aldering
  • D. Rubin
  • C. Baltay
  • D. Rabinowitz
  • N. Suzuki

The primary venues where they have published their work cover a range of respected journals and archives such as:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • Research Notes of the AAS
  • Proceedings of the National Academy of Sciences

Among the recognitions for their work, Saul Perlmutter has received multiple awards including the Breakthrough Prize in Fundamental Physics in 2015 for demonstrating that the expansion of the universe is accelerating. They were awarded the Nobel Prize in 2011 for the discovery of the accelerating expansion of the universe through observations of distant supernovae.

Additional honors include fellowships with the American Academy of Arts and Sciences, the American Association for the Advancement of Science (AAAS), and the American Physical Society (APS), as well as membership in the National Academy of Sciences. The fellowship with APS specifically cites pioneering contributions to cosmology and the development of search techniques that led to the discovery of numerous distant supernovae and evidence for the accelerated cosmic expansion.

Best Publications

  • Measurements of Omega and Lambda from 42 High-Redshift Supernovae

    S. Perlmutter;G. Aldering;G. Goldhaber;R.A. Knop

  • Measurements of Omega and Lambda from 42 High-Redshift Supernovae

    S. Perlmutter;S. Perlmutter;G. Aldering;G. Goldhaber;G. Goldhaber;R. A. Knop

  • 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

  • Discovery of a supernova explosion at half the age of the Universe

    S. Perlmutter;S. Perlmutter;G. Aldering;M. Della Valle;S. Deustua;S. Deustua

  • Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications

    S. Perlmutter;G. Aldering;M. Della Valle;S. Deustua

  • Measurements* of the Cosmological Parameters Ω and Λ from the First Seven Supernovae at z ≥ 0.35

    Saul Perlmutter;Saul Perlmutter;S. Gabi;S. Gabi;G. Goldhaber;G. Goldhaber;Ariel Goobar;Ariel Goobar;Ariel Goobar

  • 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

  • New Constraints on ΩM, ΩΛ, and w from an Independent Set of 11 High-Redshift Supernovae Observed with the Hubble Space Telescope*

    R. A. Knop;R. A. Knop;G. Aldering;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

  • The Hubble Space Telescope Cluster Supernova Survey. V. Improving the Dark-energy Constraints above z > 1 and Building an Early-type-hosted Supernova Sample

    N. Suzuki;N. Suzuki;D. Rubin;D. Rubin;C. Lidman;G. Aldering

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

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

  • Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation

    R. Amanullah;C. Lidman;D. Rubin;G. Aldering

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

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

  • Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35

    S. Perlmutter;S. Gabi;G. Goldhaber;D. E. Groom

  • The Cosmic Triangle : Revealing the State of the Universe

    Neta Bahcall;Jeremiah P. Ostriker;Saul Perlmutter;Paul Joseph Steinhardt

  • SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 <z< 1.12 AND THE UNION2 COMPILATION ∗

    Rahman Amanullah;Chris Lidman;D. Rubin;D. Rubin;G. Aldering

  • Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

    D. Spergel;N. Gehrels;C. Baltay;D. Bennett

  • Possible gravitational microlensing of a star in the Large Magellanic Cloud

    C. Alcock;C. Alcock;Carl W. Akerlof;Carl W. Akerlof;R. A. Allsman;T. S. Axelrod

  • 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

Frequent Co-Authors

Peter Nugent
Peter Nugent Lawrence Berkeley National Laboratory
Charling Tao
Charling Tao Aix-Marseille University
Stephen Bailey
Stephen Bailey Lawrence Berkeley National Laboratory
Mark Sullivan
Mark Sullivan University of Southampton
Ryan J. Foley
Ryan J. Foley University of California, Santa Cruz
Ariel Goobar
Ariel Goobar Stockholm University
Richard S. Ellis
Richard S. Ellis University College London
Joshua A. Frieman
Joshua A. Frieman University of Chicago
Eric V. Linder
Eric V. Linder Lawrence Berkeley National Laboratory
Nicolas Regnault
Nicolas Regnault Princeton University

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