World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
127
Citations
127462
World Ranking
608
National Ranking
336

Todor Stanev publications per year

1972: 1 publications 1973: 0 publications 1974: 0 publications 1975: 2 publications 1976: 0 publications 1977: 5 publications 1978: 0 publications 1979: 3 publications 1980: 1 publications 1981: 4 publications 1982: 4 publications 1983: 4 publications 1984: 3 publications 1985: 8 publications 1986: 3 publications 1987: 5 publications 1988: 7 publications 1989: 10 publications 1990: 9 publications 1991: 13 publications 1992: 3 publications 1993: 17 publications 1994: 7 publications 1995: 11 publications 1996: 9 publications 1997: 7 publications 1998: 9 publications 1999: 11 publications 2000: 10 publications 2001: 9 publications 2002: 8 publications 2003: 7 publications 2004: 16 publications 2005: 7 publications 2006: 13 publications 2007: 14 publications 2008: 13 publications 2009: 20 publications 2010: 23 publications 2011: 24 publications 2012: 15 publications 2013: 29 publications 2014: 19 publications 2015: 25 publications 2016: 25 publications 2017: 35 publications 2018: 19 publications 2019: 23 publications 2020: 24 publications 2021: 29 publications 2022: 0 publications 2023: 1 publications 2024: 6 publications
1972 2024

570 publications in total across all disciplines

Todor Stanev 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 Todor Stanev 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: 625 publications — 71st percentile

71% of scientists in this discipline score the same or lower.

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

Todor Stanev 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 Todor Stanev 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: 127 D-Index — 83rd percentile

83% 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

  • 1997 - Fellow of American Physical Society (APS) Citation For outstanding contributions to understanding the origin of cosmic rays at ultrahigh energies and for pioneering research in the field of neutrino astrophysics

Overview

Todor Stanev is affiliated with the University of Delaware in the United States and has contributed extensively to the field of Physics and Astronomy, specializing particularly in Nuclear and High Energy Physics as well as Astronomy and Astrophysics. Their research spans a variety of topics including Astrophysics and Cosmic Phenomena, Dark Matter and Cosmic Phenomena, Gamma-ray bursts and supernovae, Neutrino Physics Research, Astrophysical Phenomena and Observations, Particle physics theoretical and experimental studies, and Pulsars and Gravitational Waves Research.

Their publication record includes several recent papers such as Hadronic interaction model sibyll 2.3d and extensive air showers (2020, Physical review. D/Physical review. D.), Loaded layer-cake model for cosmic ray interaction around exploding super-giant stars making black holes (2024, Astroparticle Physics), A two-step strategy to identify episodic sources of gravitational waves and high-energy neutrinos in starburst galaxies (2024, Frontiers in Astronomy and Space Sciences), Cosmic ray contributions from rapidly rotating stellar mass black holes: Cosmic Ray GeV to EeV proton and anti-proton sources (2024, arXiv (Cornell University)), and another iteration of the loaded layer-cake model paper published in 2024 within arXiv (Cornell University).

Stanev's work has been published in a range of venues with notable frequent publication outlets including:

  • Frontiers in Astronomy and Space Sciences
  • arXiv (Cornell University)
  • Physical review. D/Physical review. D.
  • Astroparticle Physics

Their collaborations involve several frequent co-authors such as A. Chieffi, D. Frekers, L. Gergely, B. Harms, and Pankaj S. Joshi.

In addition to journal publications, Todor Stanev has authored books, including High Energy Cosmic Rays published by Springer Nature (Netherlands) in 2021.

The work and contributions of Todor Stanev have been recognized through the award of Fellow of the American Physical Society (APS) in 1997, based on outstanding contributions to understanding the origin of cosmic rays at ultrahigh energies and pioneering research in neutrino astrophysics.

Best Publications

  • Review of Particle Physics

    C. Amsler;M. Doser;M. Antonelli;D. M. Asner

  • Review of Particle Physics

    K. A. Olive;K. Agashe;C. Amsler;M. Antonelli

  • Review of Particle Physics: Particle data group

    K. Hagiwara;K. Hikasa;K. Nakamura;M. Tanabashi

  • APS : Review of Particle Physics, 2018-2019

    M Tanabashi;P Richardson;A Bettini;A Vogt

  • Review of Particle Physics

    K. Nakamura;K. Hagiwara;K. Hikasa;H. Murayama;H. Murayama;H. Murayama

  • Review of Particle Physics, 2002-2003

    O Zenin;Mark A Srednicki;Kirill Slava Lugovsky;Donald E Groom

  • Review of particle properties.

    K. Hagiwara;K. Hikasa;K. Nakamura;M. Tanabashi

  • Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector

    M. G. Aartsen;R. Abbasi;Y. Abdou;M. Ackermann

  • Observation of high-energy astrophysical neutrinos in three years of icecube data

    M. G. Aartsen;M. Ackermann;J. Adams;J. A. Aguilar

  • Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert

    Mark Aartsen;Markus Ackermann;Jenni Adams

  • First observation of PeV-energy neutrinos with IceCube

    M. G. Aartsen;R. Abbasi;Y. Abdou;M. Ackermann

  • Evidence for correlated changes in the spectrum and composition of cosmic rays at extremely high energies.

    D. J. Bird;S. C. Corbató;H. Y. Dai;B. R. Dawson

  • Particle astrophysics with high energy neutrinos

    Thomas K. Gaisser;Francis Halzen;Todor Stanev

  • The IceCube Neutrino Observatory: Instrumentation and Online Systems

    M.G. Aartsen;M. Ackermann;J. Adams;J.A. Aguilar

  • BL Lac objects in the synchrotron proton blazar model

    A. Mücke;R.J. Protheroe;R. Engel;J.P. Rachen

  • First year performance of the IceCube neutrino telescope

    A. Achterberg;M. Ackermann;J. Adams;J. Ahrens

  • Neutrinos from propagation of ultrahigh energy protons

    Ralph Engel;David Seckel;Todor Stanev

  • Cosmic ray interaction event generator SIBYLL 2.1

    Eun-Joo Ahn;Eun-Joo Ahn;Ralph Engel;Thomas K. Gaisser;Paolo Lipari

  • BL Lac Objects in the Synchrotron Proton Blazar Model

    A. Muecke;R. J. Protheroe;R. Engel;J. P. Rachen

  • Review of Particle Physics, 2008-2009

    Claude Amsler;P Richardson;O Zenin;L Garren

Frequent Co-Authors

Francis Halzen
Francis Halzen University of Wisconsin–Madison
Teresa Montaruli
Teresa Montaruli University of Geneva
Hermann Kolanoski
Hermann Kolanoski Deutsches Elektronen-Synchrotron DESY
A. Karle
A. Karle University of Wisconsin–Madison
Paul Evenson
Paul Evenson University of Delaware
R. G. Stokstad
R. G. Stokstad Lawrence Berkeley National Laboratory
D. Berley
D. Berley University of Maryland, College Park
S. W. Barwick
S. W. Barwick University of California, Irvine
J. J. Beatty
J. J. Beatty The Ohio State University
G. W. Sullivan
G. W. Sullivan University of Maryland, College Park

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