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 P. Lukens sits on this spectrum.
This scientist: 845 publications — 86th percentile
86% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where P. Lukens sits on this spectrum.
This scientist: 105 D-Index — 63rd percentile
63% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
P. Lukens is affiliated with Fermilab in the United States and has contributed extensively to research in physics and astronomy, with a particular focus on nuclear and high energy physics. Their work spans multiple subfields, including astronomy and astrophysics, atomic and molecular physics and optics, radiation, and condensed matter physics.
The scientist's primary research topics encompass dark matter and cosmic phenomena, particle detector development and performance, particle physics theoretical and experimental studies, atomic and subatomic physics research, superconducting and THz device technology, radiation detection and scintillator technologies, and neutrino physics research.
Their recent scholarly output includes the following papers:
Their frequent co-authors include:
P. Lukens has published primarily in the following venues:
The scientist was recognized as a Fellow of the American Physical Society in 2011, with a citation highlighting their leadership roles and contributions during the CDF II experiment. This included responsibilities in construction, installation, data-taking operations, and data analyses, such as the observation and precision measurement of three new baryons containing a b-quark.
F. Abe;H. Akimoto;A. Akopian;M. G. Albrow
F. Abe;D. Amidei;G. Apollinari;M. Atac
T. Aaltonen;B. Álvarez González;B. Álvarez González;S. Amerio;D. Amidei
F. Abe;H. Akimoto;A. Akopian;M. G. Albrow
F. Abe;H. Akimoto;A. Akopian;M. G. Albrow
F. Abe;M. Albrow;D. Amidei;C. Anway-Wiese
D. Acosta;J. Adelman;T. Affolder;T. Akimoto
T. Aaltonen;V. M. Abazov;B. Abbott;M. Abolins
T. Affolder;H. Akimoto;A. Akopian;M. G. Albrow
A. Abulencia;D. Acosta;J. Adelman;T. Affolder
T. Aaltonen;J. Adelman;T. Akimoto;B. Álvarez González;B. Álvarez González
F. Abe;H. Akimoto;A. Akopian;M. G. Albrow
T. Aaltonen;V. M. Abazov;B. Abbott;B. S. Acharya
F. Abe;H. Akimoto;A. Akopian;M. G. Albrow
T. Affolder;H. Akimoto;A. Akopian;M. G. Albrow
T. Aaltonen;S. Amerio;D. Amidei;A. Anastassov
A. Abulencia;D. Acosta;J. Adelman;T. Affolder
P. Adamson;C. Ader;M. Andrews;N. Anfimov
F. Abe;H. Akimoto;A. Akopian;M. G. Albrow
T. Aaltonen;R. Field;A. Clark;J.R. Dittmann
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