World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
96
Citations
46504
World Ranking
1848
National Ranking
958

Roman Scoccimarro 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 Roman Scoccimarro 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: 160 publications — 1st percentile

1% of scientists in this discipline score the same or lower.

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

Roman Scoccimarro 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 Roman Scoccimarro 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: 96 D-Index — 50th percentile

50% of scientists in this discipline score the same or lower.

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

Overview

Roman Scoccimarro is affiliated with New York University in the United States and specializes in the fields of Physics and Astronomy, with a particular focus on subfields such as Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Statistical and Nonlinear Physics, and Applied Mathematics.

Their research contributions cover several main topics, including:

  • Cosmology and Gravitation Theories
  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Scientific Research and Discoveries
  • Geophysics and Gravity Measurements
  • Stellar, planetary, and galactic studies
  • Solar and Space Plasma Dynamics

Roman Scoccimarro has authored papers primarily published in journals such as Physical Review D, Monthly Notices of the Royal Astronomical Society, and arXiv. Frequent publication venues include:

  • Physical review. D/Physical review. D.
  • arXiv (Cornell University)
  • Monthly Notices of the Royal Astronomical Society

Notable recent papers include:

  • The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the quasar sample in configuration space between redshift 0.8 and 2.2, 2020, Monthly Notices of the Royal Astronomical Society
  • Galaxy power spectrum multipoles covariance in perturbation theory, 2020, Physical review. D/Physical review. D.
  • Cosmological constraints from BOSS with analytic covariance matrices, 2020, Physical review. D/Physical review. D.
  • Testing one-loop galaxy bias: Joint analysis of power spectrum and bispectrum, 2021, Physical review. D/Physical review. D.
  • Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS, 2021, arXiv (Cornell University)

They often collaborate with a number of co-authors, including:

  • Alexander Eggemeier
  • A Pezzotta
  • Ariel G. Sánchez
  • M. Crocce
  • Mathias Garny

Best Publications

  • Cosmological parameters from SDSS and WMAP

    Max Tegmark;Max Tegmark;Michael Abram Strauss;Michael R. Blanton;Kevork Abazajian

  • Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies

    Daniel J. Eisenstein;Daniel J. Eisenstein;Idit Zehavi;David W. Hogg;Roman Scoccimarro

  • THE THREE-DIMENSIONAL POWER SPECTRUM OF GALAXIES FROM THE SLOAN DIGITAL SKY SURVEY

    Max Tegmark;Michael R. Blanton;Michael A. Strauss;Fiona Hoyle

  • The 3D power spectrum of galaxies from the SDSS

    M Tegmark;M Blanton;M Strauss;F Hoyle

  • Large scale structure of the universe and cosmological perturbation theory

    F. Bernardeau;S. Colombi;E. Gaztañaga;E. Gaztañaga;R. Scoccimarro;R. Scoccimarro

  • Cosmological constraints from the SDSS luminous red galaxies

    Max Tegmark;Daniel J. Eisenstein;Michael A. Strauss;David H. Weinberg

  • The Luminosity and Color Dependence of the Galaxy Correlation Function

    I. Zehavi;Z. Zheng;D. H. Weinberg;J. A. Frieman

  • The Luminosity and Color Dependence of the Galaxy Correlation Function

    Idit Zehavi;Zheng Zheng;David H. Weinberg;Joshua A. Frieman;Joshua A. Frieman

  • How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering

    Román Scoccimarro;Ravi K. Sheth;Lam Hui;Bhuvnesh Jain

  • Galaxy clustering in early sloan digital sky survey redshift data

    Idit Zehavi;Idit Zehavi;Michael R. Blanton;Michael R. Blanton;Joshua A. Frieman;Joshua A. Frieman;David H. Weinberg

  • Redshift-space distortions, pairwise velocities and nonlinearities

    Roman Scoccimarro

  • Transients from initial conditions in cosmological simulations

    Martín Crocce;Sebastián Pueblas;Román Scoccimarro

  • Renormalized cosmological perturbation theory

    Martín Crocce;Román Scoccimarro

  • Percolation Galaxy Groups and Clusters in the SDSS Redshift Survey: Identification, Catalogs, and the Multiplicity Function

    Andreas A. Berlind;Joshua A. Frieman;David H. Weinberg;Michael R. Blanton

  • Nonlinear evolution of baryon acoustic oscillations

    Martín Crocce;Martín Crocce;Román Scoccimarro

  • Percolation Galaxy Groups and Clusters in the SDSS Redshift Survey: Identification, Catalogs, and the Multiplicity Function

    Andreas A. Berlind;Andreas A. Berlind;Joshua Frieman;David H. Weinberg;Michael R. Blanton

  • Gravity and Large-Scale Nonlocal Bias

    Kwan Chuen Chan;Román Scoccimarro;Ravi K. Sheth;Ravi K. Sheth

  • Probing Newton's constant on vast scales: Dvali-Gabadadze-Porrati gravity, cosmic acceleration, and large scale structure

    Arthur Lue;Arthur Lue;Román Scoccimarro;Glenn D. Starkman;Glenn D. Starkman

  • On Departures From a Power Law in the Galaxy Correlation Function

    Idit Zehavi;David H. Weinberg;Zheng Zheng;Andreas A. Berlind

  • On Departures from a Power Law in the Galaxy Correlation Function

    Idit Zehavi;Idit Zehavi;David H. Weinberg;Zheng Zheng;Andreas A. Berlind;Andreas A. Berlind

Frequent Co-Authors

Joshua A. Frieman
Joshua A. Frieman University of Chicago
Ravi K. Sheth
Ravi K. Sheth University of Pennsylvania
Andreas A. Berlind
Andreas A. Berlind Vanderbilt University
Daniel J. Eisenstein
Daniel J. Eisenstein Harvard University
Idit Zehavi
Idit Zehavi Case Western Reserve University
Donald P. Schneider
Donald P. Schneider Pennsylvania State University
Scott Dodelson
Scott Dodelson Carnegie Mellon University
Alexander S. Szalay
Alexander S. Szalay Johns Hopkins University
Robert C. Nichol
Robert C. Nichol University of Surrey

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