| Discipline name | D-Index | World Ranking | Current World Ranking | National Ranking | Current National Ranking | Publications | Citations |
|---|---|---|---|---|---|---|---|
| Physics | 116 | 931 | 878 | 493 | 457 | 323 | 83949 |
The chart shows the history of publications by Michele Vallisneri between 1999 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Michele Vallisneri published across 27 years, from 1999 to 2025, averaging 13 papers a year. Output peaked at 24 publications in 2017. 27 of the 351 publications appeared in the last two years.
351 publications in total across all disciplines
| Year | Publications |
|---|---|
| 1999 | 1 |
| 2000 | 2 |
| 2001 | 1 |
| 2002 | 3 |
| 2003 | 5 |
| 2004 | 12 |
| 2005 | 13 |
| 2006 | 11 |
| 2007 | 17 |
| 2008 | 15 |
| 2009 | 16 |
| 2010 | 16 |
| 2011 | 20 |
| 2012 | 17 |
| 2013 | 12 |
| 2014 | 22 |
| 2015 | 12 |
| 2016 | 23 |
| 2017 | 24 |
| 2018 | 11 |
| 2019 | 19 |
| 2020 | 18 |
| 2021 | 12 |
| 2022 | 4 |
| 2023 | 18 |
| 2024 | 14 |
| 2025 | 13 |
| Total | 351 |
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 Michele Vallisneri sits on this spectrum.
This scientist: 323 publications — 22nd percentile
22% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
| Publications | Scientists | This scientist |
|---|---|---|
| 103–122 | 7 | |
| 123–142 | 10 | |
| 143–162 | 31 | |
| 163–182 | 35 | |
| 183–202 | 53 | |
| 203–222 | 81 | |
| 223–242 | 85 | |
| 243–262 | 112 | |
| 263–282 | 114 | |
| 283–302 | 126 | |
| 303–322 | 136 | |
| 323–342 | 162 | 323 |
| 343–362 | 155 | |
| 363–382 | 156 | |
| 383–402 | 134 | |
| 403–422 | 145 | |
| 423–442 | 147 | |
| 443–462 | 131 | |
| 463–482 | 131 | |
| 483–502 | 116 | |
| 503–522 | 106 | |
| 523–542 | 103 | |
| 543–562 | 87 | |
| 563–582 | 84 | |
| 583–602 | 94 | |
| 603–622 | 70 | |
| 623–642 | 76 | |
| 643–662 | 60 | |
| 663–682 | 54 | |
| 683–702 | 60 | |
| 703–722 | 48 | |
| 723–742 | 64 | |
| 743–762 | 48 | |
| 763–782 | 37 | |
| 783–802 | 43 | |
| 803–822 | 34 | |
| 823–842 | 36 | |
| 843–862 | 32 | |
| 863–882 | 32 | |
| 883–902 | 31 | |
| 903–922 | 25 | |
| 923–942 | 15 | |
| 943–962 | 24 | |
| 963–982 | 13 | |
| 983–1,002 | 21 | |
| 1,003–1,022 | 21 | |
| 1,023–1,042 | 16 | |
| 1,043–1,062 | 9 | |
| 1,063–1,082 | 19 | |
| 1,083–1,102 | 11 | |
| 1,103–1,122 | 17 | |
| 1,123–1,142 | 11 | |
| 1,143–1,162 | 7 | |
| 1,163–1,182 | 4 | |
| 1,183–1,202 | 10 | |
| 1,203–1,222 | 8 | |
| 1,223–1,242 | 16 | |
| 1,243–1,262 | 4 | |
| 1,263–1,282 | 10 | |
| 1,283–1,302 | 5 | |
| 1,303–1,322 | 7 | |
| 1,323–1,342 | 4 | |
| 1,343–1,362 | 8 | |
| 1,363–1,382 | 6 | |
| 1,383–1,402 | 7 | |
| 1,403–1,422 | 3 | |
| 1,423–1,442 | 4 | |
| 1,443–1,462 | 4 | |
| 1,463–1,468 | 3 | |
| 1,469+ | 100 |
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Michele Vallisneri sits on this spectrum.
This scientist: 116 D-Index — 75th percentile
75% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
| D-Index | Scientists | This scientist |
|---|---|---|
| 70–71 | 76 | |
| 72–73 | 110 | |
| 74–75 | 143 | |
| 76–77 | 153 | |
| 78–79 | 144 | |
| 80–81 | 167 | |
| 82–83 | 167 | |
| 84–85 | 166 | |
| 86–87 | 132 | |
| 88–89 | 155 | |
| 90–91 | 134 | |
| 92–93 | 137 | |
| 94–95 | 102 | |
| 96–97 | 112 | |
| 98–99 | 110 | |
| 100–101 | 116 | |
| 102–103 | 97 | |
| 104–105 | 103 | |
| 106–107 | 87 | |
| 108–109 | 90 | |
| 110–111 | 67 | |
| 112–113 | 78 | |
| 114–115 | 75 | |
| 116–117 | 67 | 116 |
| 118–119 | 69 | |
| 120–121 | 60 | |
| 122–123 | 59 | |
| 124–125 | 53 | |
| 126–127 | 42 | |
| 128–129 | 41 | |
| 130–131 | 33 | |
| 132–133 | 32 | |
| 134–135 | 45 | |
| 136–137 | 19 | |
| 138–139 | 24 | |
| 140–141 | 28 | |
| 142–143 | 31 | |
| 144–145 | 22 | |
| 146–147 | 20 | |
| 148–149 | 12 | |
| 150–151 | 16 | |
| 152–153 | 24 | |
| 154–155 | 23 | |
| 156–157 | 15 | |
| 158–159 | 15 | |
| 160–161 | 11 | |
| 162–163 | 17 | |
| 164–165 | 12 | |
| 166–167 | 11 | |
| 168–169 | 9 | |
| 170–171 | 9 | |
| 172–173 | 11 | |
| 174–175 | 4 | |
| 176–177 | 8 | |
| 178–179 | 5 | |
| 180–181 | 3 | |
| 182–183 | 4 | |
| 184 | 4 | |
| 185+ | 99 |
Michele Vallisneri 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 in the subfields of Astronomy and Astrophysics, Oceanography, Atomic and Molecular Physics and Optics, Nuclear and High Energy Physics, and Artificial Intelligence.
The scientist's main topics of work include:
Their frequent co-authors include:
Vallisneri has contributed frequently to the following publication venues:
Selected recent papers include:
Vallisneri was named a Fellow of the American Physical Society (APS) in 2016. The citation recognized their contributions to the statistical theory and computational practice of gravitational wave detection and parameter estimation, as well as efforts in applying techniques across ground-based, space-based, and pulsar-timing detection programs.
B. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy
B. P. Abbott;R. Abbott
J. Abadie;B. P. Abbott;R. Abbott;M. Abernathy
J. Abadie;B. P. Abbott
B. P. Abbott;R. Abbott
J. Aasi;J. Abadie;B. P. Abbott;R. Abbott
J. Aasi;J. Abadie;B. P. Abbott;R. Abbott
J. Abadie;B. P. Abbott;R. Abbott;T. D. Abbott
Michele Vallisneri
Zaven Arzoumanian;Adam Brazier;Sarah Burke-Spolaor;Sydney Chamberlin
Pau Amaro-Seoane;Sofiane Aoudia;Stanislav Babak;Pierre Binetruy
B. P. Abbott;R. Abbott;F. Acernese;R. Adhikari
Zaven Arzoumanian;Adam Brazier;Sarah Burke-Spolaor;Sydney Chamberlin
Z. Arzoumanian;P. T. Baker;A. Brazier;S. Burke-Spolaor
Zaven Arzoumanian;Paul T. Baker;Harsha Blumer;Bence Bécsy
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