World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
100
Citations
34998
World Ranking
1657
National Ranking
873

Daniel Kasen 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 Daniel Kasen 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: 286 publications — 15th percentile

15% of scientists in this discipline score the same or lower.

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

Daniel Kasen 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 Daniel Kasen 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: 100 D-Index — 56th percentile

56% 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

  • 2017 - Fellow of American Physical Society (APS) Citation For leadership in developing predictive theories and models of supernova light curves and spectra, impacting our understanding of the widthluminosity relation in Type Ia supernova, the transient optical and IR signals from neutron star mergers, supernova explosion mechanisms, and nucleosynthesis

Overview

Daniel Kasen is affiliated with the University of California, Berkeley in the United States. Their primary field of study is Physics and Astronomy, with a focused expertise in subfields such as Astronomy and Astrophysics, Nuclear and High Energy Physics, Biomedical Engineering, Oceanography, and Applied Mathematics.

Kasen's body of work includes 111 publications in Physics and Astronomy, with a majority concentrating on Astronomy and Astrophysics. Their research covers several specialized topics including gamma-ray bursts and supernovae, pulsars and gravitational waves research, astrophysical phenomena and observations, stellar, planetary, and galactic studies, astrophysics and cosmic phenomena, mechanics and biomechanics studies, as well as astrophysics and star formation studies.

Some of their recent papers include:

  • Exascale applications: skin in the game, 2020, Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences
  • The rapid reddening and featureless optical spectra of the optical counterpart of GW170817, at 2017gfo, during the first four days, 2024, OPAL (Open@LaTrobe) (La Trobe University)
  • Radiative Emission Mechanisms of Tidal Disruption Events, 2020, arXiv (Cornell University)
  • The Next Generation Global Gravitational Wave Observatory: The Science Book, 2021, Data Archiving and Networked Services (DANS)
  • Nebular Models of Sub-Chandrasekhar Mass Type Ia Supernovae: Clues to the Origin of Ca-rich Transients, 2021, The Astrophysical Journal

Kasen collaborates frequently with other scientists, including Brian D. Metzger, A. Rest, Nathaniel Roth, R. J. Foley, and R. Margutti.

Their publications appear most often in:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal Letters
  • Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences

Daniel Kasen was awarded the title of Fellow of the American Physical Society (APS) in 2017. The citation recognized their leadership in developing predictive theories and models related to supernova light curves and spectra, particularly influencing the understanding of the width-luminosity relation in Type Ia supernovae, transient optical and infrared signals from neutron star mergers, supernova explosion mechanisms, and nucleosynthesis processes.

Best Publications

  • Electromagnetic counterparts of compact object mergers powered by the radioactive decay of r‐process nuclei

    B. D. Metzger;G. Martínez-Pinedo;S. Darbha;E. Quataert

  • A gravitational-wave standard siren measurement of the Hubble constant

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese;F. Acernese

  • Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave event

    Daniel Kasen;Brian Metzger;Jennifer Barnes;Eliot Quataert

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models

    P. S. Cowperthwaite;E. Berger;V. A. Villar;B. D. Metzger

  • Supernova Light Curves Powered by Young Magnetars

    Daniel Kasen;Lars Bildsten

  • Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source

    D. A. Coulter;R. J. Foley;C. D. Kilpatrick;M. R. Drout

  • Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis

    M. R. Drout;A. L. Piro;B. J. Shappee;C. D. Kilpatrick

  • EFFECT OF A HIGH OPACITY ON THE LIGHT CURVES OF RADIOACTIVELY POWERED TRANSIENTS FROM COMPACT OBJECT MERGERS

    Jennifer Barnes;Jennifer Barnes;Daniel Kasen;Daniel Kasen

  • Supernova SN 2011fe from an exploding carbon–oxygen white dwarf star

    Peter E. Nugent;Peter E. Nugent;Mark Sullivan;S. Bradley Cenko;Rollin C. Thomas

  • Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger

    Iair Arcavi;Iair Arcavi;Griffin Hosseinzadeh;Griffin Hosseinzadeh;D. Andrew Howell;D. Andrew Howell;Curtis McCully;Curtis McCully

  • Supernova 2007bi as a pair-instability explosion.

    Avishay Gal-Yam;P. Mazzali;E. O. Ofek;P. E. Nugent

  • Opacities and Spectra of the $r$-process Ejecta from Neutron Star Mergers

    Daniel Kasen;Daniel Kasen;N. R. Badnell;Jennifer Barnes;Jennifer Barnes

  • Illuminating gravitational waves: A concordant picture of photons from a neutron star merger

    M. M. Kasliwal;E. Nakar;L. P. Singer;L. P. Singer;D. L. Kaplan

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Discovery of the Optical Counterpart Using the Dark Energy Camera

    M. Soares-Santos;M. Soares-Santos;D. E. Holz;J. Annis;R. Chornock

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South

    R. Chornock;E. Berger;D. Kasen;P. S. Cowperthwaite

  • Time-dependent Monte Carlo Radiative Transfer Calculations for Three-dimensional Supernova Spectra, Light Curves, and Polarization

    Daniel Kasen;Daniel Kasen;R.C. Thomas;Peter Nugent

  • Sub-Chandrasekhar Mass Models for Supernovae

    S. E. Woosley;Daniel Kasen;Daniel Kasen

  • SEEING THE COLLISION OF A SUPERNOVA WITH ITS COMPANION STAR

    Daniel Kasen

  • Time Dependent Monte Carlo Radiative Transfer Calculations For 3-Dimensional Supernova Spectra, Lightcurves, and Polarization

    Daniel Kasen;R. C. Thomas;Peter Nugent

  • Sub-Chandrasekhar Mass Models For Type Ia Supernovae

    S. E. Woosley;Daniel Kasen

Frequent Co-Authors

Enrico Ramirez-Ruiz
Enrico Ramirez-Ruiz University of California, Santa Cruz
Peter M. Garnavich
Peter M. Garnavich University of Notre Dame
Eliot Quataert
Eliot Quataert Princeton University
Brian D. Metzger
Brian D. Metzger Columbia University
Peter Nugent
Peter Nugent Lawrence Berkeley National Laboratory
Ryan J. Foley
Ryan J. Foley University of California, Santa Cruz
Marcelle Soares-Santos
Marcelle Soares-Santos Brandeis University
Barry F. Madore
Barry F. Madore Carnegie Institution for Science
Alexei V. Filippenko
Alexei V. Filippenko University of California, Berkeley
Stefano Valenti
Stefano Valenti University of California, Davis

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