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 R. M. S. Schofield sits on this spectrum.
This scientist: 394 publications — 37th percentile
37% 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 R. M. S. Schofield sits on this spectrum.
This scientist: 132 D-Index — 86th percentile
86% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
R. M. S. Schofield is affiliated with the University of Oregon in the United States and specializes in materials science and engineering. The scientist's research spans multiple subfields including biomedical engineering, biomaterials, polymers and plastics, electrical and electronic engineering, and materials chemistry.
The work conducted by Schofield primarily focuses on advanced sensor and energy harvesting materials, conducting polymers and their applications, organic electronics and photovoltaics, electrospun nanofibers in biomedical applications, supercapacitor materials and fabrication, silk-based biomaterials, and graphene research.
Frequent coauthors collaborating with Schofield include Barbara M. Maciejewska, Nicole Grobert, George T. Tebbutt, Hazel E. Assender, and Shiling Dong.
Schofield's recent publications illustrate a strong emphasis on nanofiber technologies and their applications in energy and biomedical fields:
Schofield frequently publishes in journals such as Advanced Composites and Hybrid Materials, ACS Nano, Small, Research Square (Research Square), and ACS Applied Polymer Materials.
In 2014, Schofield was recognized as a Fellow of the American Physical Society (APS) for leadership in identifying and mitigating environmental factors impacting the sensitivity of terrestrial gravitational wave detectors and eliminating spurious noise sources in LIGO.
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