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D-Index & Metrics

Physics

D-Index
81
Citations
30765
World Ranking
2901
National Ranking
1413

Kim Griest 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 Kim Griest 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: 296 publications — 17th percentile

17% of scientists in this discipline score the same or lower.

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

Kim Griest 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 Kim Griest 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: 81 D-Index — 22nd percentile

22% 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

  • 2001 - Fellow of American Physical Society (APS) Citation For contributions to understanding the nature of dark matter, including the theory of relic abundance and detection of particle dark matter, and the theory, discovery, and interpretation of gravitational microlensing
  • 1994 - Fellow of Alfred P. Sloan Foundation

Overview

Kim Griest is a researcher affiliated with the University of California, San Diego in the United States. Their academic focus spans a range of topics within physics, particularly involving the nature of dark matter and gravitational microlensing phenomena.

Their recognized contributions include advancing the theoretical understanding of relic abundance and detection mechanisms for particle dark matter. Additionally, they have contributed to the theory, discovery, and interpretation of gravitational microlensing, which is a technique used to detect objects that emit little or no light by observing the bending of light from distant stars.

Kim Griest has been acknowledged by professional organizations with notable awards. In 2001, they were named a Fellow of the American Physical Society (APS) with a citation emphasizing contributions to dark matter research and gravitational microlensing. Earlier, in 1994, they were awarded a Fellowship by the Alfred P. Sloan Foundation.

Best Publications

  • Supersymmetric Dark Matter

    Gerard Jungman;Marc Kamionkowski;Marc Kamionkowski;Kim Griest

  • Three exceptions in the calculation of relic abundances

    Kim Griest;David Seckel

  • The MACHO Project: Microlensing Results from 5.7 Years of Large Magellanic Cloud Observations

    Charles Alcock;Charles Alcock;Robyn Allsman;David R Alves;Tim Axelrod

  • 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

  • The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations

    C. Alcock;R. A. Allsman;D. R. Alves

  • Unitarity limits on the mass and radius of dark-matter particles

    Kim Griest;Marc Kamionkowski;Marc Kamionkowski

  • The MACHO Project Large Magellanic Cloud Microlensing Results from the First Two Years and the Nature of the Galactic Dark Halo

    C. Alcock;C. Alcock;R. A. Allsman;D. Alves;D. Alves;T. S. Axelrod

  • The MACHO Project LMC Microlensing Results from the First Two Years and the Nature of the Galactic Dark Halo

    C. Alcock;R. A. Allsman;D. Alves;T. S. Axelrod

  • The Use of High-Magnification Microlensing Events in Discovering Extrasolar Planets

    Kim Griest;Neda Safizadeh

  • The Use of High Magnification Microlensing Events in Discovering Extra-solar Planets

    Kim Griest;Neda Safizadeh

  • Cosmic asymmetry, neutrinos and the sun☆

    Kim Griest;David Seckel;David Seckel

  • Galactic microlensing as a method of detecting massive compact halo objects

    Kim Griest

  • The Macho Project: 45 Candidate Microlensing Events from the First Year Galactic Bulge Data

    C. Alcock;C. Alcock;R. A. Allsman;D. Alves;T. S. Axelrod;T. S. Axelrod

  • MACHO Project Limits on Black Hole Dark Matter in the 1-30 Solar Mass Range

    C. Alcock;R. A. Allsman;D. R. Alves

  • EROS and MACHO combined limits on planetary-mass dark matter in the galactic halo

    C Alcock;C Alcock;RA Allsman;D Alves;D Alves;R Ansari

  • First Observation of Parallax in a Gravitational Microlensing Event

    C. Alcock;C. Alcock;R. A. Allsman;D. Alves;D. Alves;T. S. Axelrod;T. S. Axelrod

  • The MACHO Project: 45 Candidate Microlensing Events from the First Year Galactic Bulge Data

    C. Alcock;R. A. Allsman;T. S. Axelrod;D. P. Bennett

  • EXPERIMENTAL LIMITS ON THE DARK MATTER HALO OF THE GALAXY FROM GRAVITATIONAL MICROLENSING

    C. Alcock;C. Alcock;R. A. Allsman;T. S. Axelrod;T. S. Axelrod;D. P. Bennett;D. P. Bennett

  • Cross sections, relic abundance, and detection rates for neutralino dark matter.

    Kim Griest;Kim Griest

  • The MACHO Project: Microlensing Optical Depth Toward the Galactic Bulge from Difference Image Analysis

    Charles Alcock;Charles Alcock;Robyn Allsman;David R Alves;Tim Axelrod

Frequent Co-Authors

David P. Bennett
David P. Bennett Goddard Space Flight Center
Charles Alcock
Charles Alcock Harvard University
Christopher W. Stubbs
Christopher W. Stubbs Harvard University
Kenneth C. Freeman
Kenneth C. Freeman Australian National University
Bruce A. Peterson
Bruce A. Peterson Australian National University
William J. Sutherland
William J. Sutherland University of Cambridge
Dante Minniti
Dante Minniti Andrés Bello University
Saul Perlmutter
Saul Perlmutter Lawrence Berkeley National Laboratory
Marc Kamionkowski
Marc Kamionkowski Johns Hopkins University
Andrew Gould
Andrew Gould The Ohio State University

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