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Physics
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2026

D-Index & Metrics

Physics

D-Index
170
Citations
117926
World Ranking
145
National Ranking
95

Shrinivas R. Kulkarni 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 Shrinivas R. Kulkarni 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: 1,390 publications — 97th percentile

97% of scientists in this discipline score the same or lower.

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

Shrinivas R. Kulkarni 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 Shrinivas R. Kulkarni 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: 170 D-Index — 96th percentile

96% 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

  • 2026 - Research.com Physics in United States Leader Award
  • 2025 - Research.com Physics in United States Leader Award

Overview

Shrinivas R. Kulkarni is affiliated with the California Institute of Technology in the United States. Their research primarily focuses on physics and astronomy, with a significant number of publications contributing to the subfields of astronomy and astrophysics, nuclear and high energy physics, instrumentation, computational mechanics, and biomedical engineering.

The scientist's work covers diverse main topics, prominently including gamma-ray bursts and supernovae, stellar, planetary, and galactic studies, pulsars and gravitational waves research, astrophysical phenomena and observations, astrophysics and cosmic phenomena, astronomy and astrophysical research, and astro and planetary science.

Shrinivas R. Kulkarni has published extensively in several venues, with frequent contributions to:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • Publications of the Astronomical Society of the Pacific
  • The Astrophysical Journal Letters

Among the most recent papers are:

  • The Zwicky Transient Facility Bright Transient Survey. I. Spectroscopic Classification and the Redshift Completeness of Local Galaxy Catalogs (2020), The Astrophysical Journal
  • The Final Season Reimagined: 30 Tidal Disruption Events from the ZTF-I Survey (2022), The Astrophysical Journal
  • Tidal Disruption Event Demographics with the Zwicky Transient Facility: Volumetric Rates, Luminosity Function, and Implications for the Local Black Hole Mass Function (2023), The Astrophysical Journal Letters
  • First tidal disruption events discovered by SRG/eROSITA: X-ray/optical properties and X-ray luminosity function at z < 0.6 (2021), Monthly Notices of the Royal Astronomical Society
  • A Systematic Search of Zwicky Transient Facility Data for Ultracompact Binary LISA-detectable Gravitational-wave Sources (2020), The Astrophysical Journal

Frequent co-authors include:

  • M. J. Graham
  • M. M. Kasliwal
  • Eric C. Bellm
  • J. Sollerman
  • Reed Riddle

Best Publications

  • The Swift Gamma-Ray Burst Mission

    N. Gehrels;G. Chincarini;G. Chincarini;P. Giommi;K. O. Mason

  • LSST: from Science Drivers to Reference Design and Anticipated Data Products

    Željko Ivezić;Steven M. Kahn;J. Anthony Tyson;Bob Abel

  • The Palomar Transient Factory: System Overview, Performance and First Results

    N. M. Law;S. R. Kulkarni;R. G. Dekany;E. O. Ofek

  • BEAMING IN GAMMA-RAY BURSTS: EVIDENCE FOR A STANDARD ENERGY RESERVOIR

    D. A. Frail;S. R. Kulkarni;R. Sari;S. G. Djorgovski

  • The zwicky transient facility: System overview, performance, and first results

    Eric C. Bellm;Shrinivas R. Kulkarni;Matthew J. Graham;Richard Dekany

  • The Palomar Transient Factory: system overview, performance and first results

    Nicholas M. Law;Shrinivas R. Kulkarni;Richard G. Dekany;Eran O. Ofek

  • LSST Science Book, Version 2.0

    Paul A. Abell;Julius Allison;Scott F. Anderson

  • Spectral constraints on the redshift of the optical counterpart to the γ-ray burst of 8 May 1997

    M. R. Metzger;S. G. Djorgovski;S. R. Kulkarni;C. C. Steidel

  • Discovery of a cool brown dwarf

    T. Nakajima;B. R. Oppenheimer;S. R. Kulkarni;D. A. Golimowski

  • Electrodynamics of Magnetars: Implications for the Persistent X-Ray Emission and Spin-down of the Soft Gamma Repeaters and Anomalous X-Ray Pulsars

    C. Thompson;M. Lyutikov;M. Lyutikov;S. R. Kulkarni

  • A millisecond pulsar

    D. C. Backer;Shrinivas R. Kulkarni;Carl Heiles;M. M. Davis

  • The radio afterglow from the γ-ray burst of 8 May 1997

    D. A. Frail;S. R. Kulkarni;L. Nicastro;M. Feroci

  • Exploring the Optical Transient Sky with the Palomar Transient Factory

    Arne Rau;Shrinivas R. Kulkarni;Nicholas M. Law;Joshua S. Bloom

  • The Observed Offset Distribution of Gamma-Ray Bursts from Their Host Galaxies: A Robust Clue to the Nature of the Progenitors* **

    J. S. Bloom;S. R. Kulkarni;S. G. Djorgovski

  • A γ-ray burst at a redshift of z ≈ 8.2

    N. R. Tanvir;D. B. Fox;A. J. Levan;E. Berger

  • Radio emission from the unusual supernova 1998bw and its association with the γ-ray burst of 25 April 1998

    Shri R. Kulkarni;D. A. Frail;M. H. Wieringa;R. D. Ekers

  • The Zwicky Transient Facility: Science Objectives

    Matthew J. Graham;S. R. Kulkarni;Eric C. Bellm;Scott M. Adams

  • An ultraluminous X-ray source powered by an accreting neutron star

    M. Bachetti;F. A. Harrison;D. J. Walton;B. W. Grefenstette

  • The afterglow of GRB 050709 and the nature of the short-hard γ-ray bursts

    Derek B Fox;Derek B Fox;Dale A Frail;Paul Antony Price;Shrinivas R Kulkarni

  • The Swift Gamma-Ray Burst Mission

    N. Gehrels;G Chincarini;P. Giommi;K. O. Mason

Frequent Co-Authors

Peter Nugent
Peter Nugent Lawrence Berkeley National Laboratory
Mansi M. Kasliwal
Mansi M. Kasliwal California Institute of Technology
Dale A. Frail
Dale A. Frail National Radio Astronomy Observatory
Avishay Gal-Yam
Avishay Gal-Yam Weizmann Institute of Science
Eran O. Ofek
Eran O. Ofek Weizmann Institute of Science
Joshua S. Bloom
Joshua S. Bloom University of California, Berkeley
Daniel A. Perley
Daniel A. Perley Liverpool John Moores University
Dovi Poznanski
Dovi Poznanski Tel Aviv University
Jesper Sollerman
Jesper Sollerman Stockholm University
Mark Sullivan
Mark Sullivan University of Southampton

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