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 C. W. Walter sits on this spectrum.
This scientist: 344 publications — 26th percentile
26% 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 C. W. Walter sits on this spectrum.
This scientist: 104 D-Index — 62nd percentile
62% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
C. W. Walter is affiliated with Duke University in the United States and has made significant contributions in the field of Physics and Astronomy, particularly focusing on Nuclear and High Energy Physics and Astronomy and Astrophysics. Their research spans several key topics including Neutrino Physics Research, Astrophysics and Cosmic Phenomena, Particle Physics theoretical and experimental studies, Dark Matter and Cosmic Phenomena, Astronomy and Astrophysical Research, Gamma-ray bursts and supernovae, and Radiation Detection and Scintillator Technologies.
The scientist's recent publications reflect a strong involvement in experimental and observational studies related to neutrinos and cosmic phenomena. Notable papers include:
The scientist collaborates frequently with a select group of researchers, including L. Wan, E. Kearns, Th. A. Mueller, Y. Hayato, and T. Yano. These collaborations underline ongoing research efforts primarily focused on neutrino physics and astrophysics.
Research outputs by C. W. Walter are predominantly published in a range of scientific venues such as:
In recognition of their contributions to the field of neutrino physics, C. W. Walter was named a Fellow of the American Physical Society (APS) in 2017. The award citation highlights their experimental study of neutrino oscillation physics, including the first observations of neutrino flavor appearance and systematic studies of neutrino flavor disappearance using atmospheric and long-baseline neutrinos in experiments such as SuperKamiokande, K2K, and T2K.
K. A. Olive;K. Agashe;C. Amsler;M. Antonelli
M Tanabashi;P Richardson;A Bettini;A Vogt
K. Nakamura;K. Hagiwara;K. Hikasa;H. Murayama;H. Murayama;H. Murayama
Y. Fukuda;T. Hayakawa;E. Ichihara;K. Inoue
P A Zyla;P Richardson;O Zenin;A Bettini
Željko Ivezić;Steven M. Kahn;J. Anthony Tyson;Bob Abel
K. Abe;N. Abgrall;Y. Ajima;H. Aihara
Y. Fukuda;M. Ishitsuka;Y. Itow;T. Kajita
M. H. Ahn;S. Aoki;H. Bhang;S. Boyd
Y. Ashie;J. Hosaka;K. Ishihara;Y. Itow
M. H. Ahn;E. Aliu;S. Andringa;S. Aoki
Željko Ivezić;Steven M. Kahn;J. Anthony Tyson;Bob Abel
S. Fukuda;Y. Fukuda;T. Hayakawa;E. Ichihara
S. Fukuda;Y. Fukuda;M. Ishitsuka;Y. Itow
S. Fukuda;Y. Fukuda;M. Ishitsuka;Y. Itow
Y. Fukuda;T. Hayakawa;E. Ichihara;K. Inoue
Y. Fukuda;T. Hayakawa;E. Ichihara;K. Inoue
K. Abe;N. Abgrall;H. Aihara;Y. Ajima
S. Fukuda;Y. Fukuda;M. Ishitsuka;Y. Itow
Y. Fukuda;T. Hayakawa;E. Ichihara;K. Inoue
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