World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
88
Citations
32413
World Ranking
2373
National Ranking
1194

Michael Boylan-Kolchin 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 Michael Boylan-Kolchin 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: 247 publications — 9th percentile

9% of scientists in this discipline score the same or lower.

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

Michael Boylan-Kolchin 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 Michael Boylan-Kolchin 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: 88 D-Index — 36th percentile

36% of scientists in this discipline score the same or lower.

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

Overview

Michael Boylan-Kolchin is affiliated with The University of Texas at Austin in the United States and primarily works in the field of Physics and Astronomy. Their research spans several subfields including Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Statistical and Nonlinear Physics, and Electrical and Electronic Engineering.

Their scholarly output includes work on key topics such as:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Stellar, planetary, and galactic studies
  • Astrophysics and Star Formation Studies
  • Cosmology and Gravitation Theories
  • Dark Matter and Cosmic Phenomena
  • Gamma-ray bursts and supernovae

Michael Boylan-Kolchin has contributed extensively to scientific literature, publishing in frequent venues like:

  • arXiv (Cornell University)
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal
  • Nature Astronomy
  • The Astrophysical Journal Supplement Series

Among their recent significant papers are:

  • Stress testing ΛCDM with high-redshift galaxy candidates (2023, Nature Astronomy)
  • A dark matter profile to model diverse feedback-induced core sizes of ΛCDM haloes (2020, Monthly Notices of the Royal Astronomical Society)
  • Public Data Release of the FIRE-2 Cosmological Zoom-in Simulations of Galaxy Formation (2023, The Astrophysical Journal Supplement Series)
  • The impact of UV variability on the abundance of bright galaxies at z ≥ 9 (2023, Monthly Notices of the Royal Astronomical Society)
  • FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations (2022, Monthly Notices of the Royal Astronomical Society)

Their work reflects frequent collaborations with other researchers, including:

  • Andrew Wetzel
  • James S. Bullock
  • Philip F. Hopkins
  • Claude-André Faucher-Giguère
  • Daniel R. Weisz

Best Publications

  • From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology

    Qi Guo;Simon White;Michael Boylan-Kolchin;Gabriella De Lucia

  • Too big to fail? The puzzling darkness of massive Milky Way subhaloes

    Michael Boylan-Kolchin;James S. Bullock;Manoj Kaplinghat

  • From dwarf spheroidals to cD galaxies: simulating the galaxy population in a ΛCDM cosmology

    Qi Guo;Simon White;Michael Boylan-Kolchin;Gabriella De Lucia

  • How do galaxies populate dark matter haloes

    Qi Guo;Simon White;Cheng Li;Michael Boylan-Kolchin

  • Resolving cosmic structure formation with the Millennium-II simulation

    Michael Boylan-Kolchin;Volker Springel;Simon D. M. White;Adrian Jenkins

  • Small-Scale Challenges to the $\Lambda$CDM Paradigm.

    James S. Bullock;Michael Boylan-Kolchin

  • FIRE-2 simulations: physics versus numerics in galaxy formation

    Philip F. Hopkins;Andrew Wetzel;Andrew Wetzel;Andrew Wetzel;Dušan Kereš;Claude André Faucher-Giguère

  • The Milky Way's bright satellites as an apparent failure of LCDM

    Michael Boylan-Kolchin;James S. Bullock;Manoj Kaplinghat

  • The Milky Way’s bright satellites as an apparent failure of ΛCDM

    Michael Boylan-Kolchin;James S. Bullock;Manoj Kaplinghat

  • Small-Scale Challenges to the ΛCDM Paradigm

    James S. Bullock;Michael Boylan-Kolchin

  • The merger rates and mass assembly histories of dark matter haloes in the two Millennium simulations

    Onsi Fakhouri;Chung-Pei Ma;Michael Boylan-Kolchin

  • Dynamical Friction and Galaxy Merging Timescales

    Michael Boylan-Kolchin;Chung-Pei Ma;Eliot Quataert

  • How do galaxies populate Dark Matter halos

    Qi Guo;Simon White;Cheng Li;Michael Boylan-Kolchin

  • Dynamical friction and galaxy merging time-scales

    Michael Boylan-Kolchin;Chung Pei Ma;Eliot Quataert

  • ELVIS: Exploring the Local Volume in Simulations

    Shea Garrison-Kimmel;Michael Boylan-Kolchin;Michael Boylan-Kolchin;James S. Bullock;Kyle Lee

  • Forged in FIRE: cusps, cores and baryons in low-mass dwarf galaxies

    Jose Oñorbe;Jose Oñorbe;Michael Boylan-Kolchin;Michael Boylan-Kolchin;James S. Bullock;Philip F. Hopkins

  • Galaxy formation in WMAP1 and WMAP7 cosmologies

    Qi Guo;Simon White;Raul E. Angulo;Bruno Henriques

  • Not so lumpy after all: modelling the depletion of dark matter subhaloes by Milky Way-like galaxies

    Shea Garrison-Kimmel;Andrew R. Wetzel;Andrew R. Wetzel;Andrew R. Wetzel;James S. Bullock;Philip F. Hopkins

  • The mass–concentration–redshift relation of cold dark matter haloes

    Aaron D. Ludlow;Julio F. Navarro;Raúl E. Angulo;Michael Boylan-Kolchin

  • Galaxy formation with BECDM - I. Turbulence and relaxation of idealized haloes.

    Philip Mocz;Mark Vogelsberger;Victor H. Robles;Jesús Zavala

Frequent Co-Authors

James S. Bullock
James S. Bullock University of California, Irvine
Philip F. Hopkins
Philip F. Hopkins California Institute of Technology
Claude André Faucher-Giguère
Claude André Faucher-Giguère Northwestern University
Dušan Kereš
Dušan Kereš University of California, San Diego
Daniel R. Weisz
Daniel R. Weisz University of California, Berkeley
Eliot Quataert
Eliot Quataert Princeton University
Volker Springel
Volker Springel Max Planck Institute for Astrophysics
Andrew A. Cole
Andrew A. Cole University of Tasmania
Antonio Aparicio
Antonio Aparicio University of La Laguna
Simon D. M. White
Simon D. M. White Max Planck Institute for Astrophysics

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