Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Hadron masses in a gauge theory
19751.3k citationsA. De Rújula, Howard Georgi et al.Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fieldsprofile →
Demythification of electroproduction local duality and precocious scaling
1977340 citationsA. De Rújula, Howard Georgi et al.profile →
Is Bound Charm Found?
1975252 citationsA. De Rújula, Sheldon L. GlashowPhysical Review Lettersprofile →
Spectroscopy of the New Mesons
1975202 citationsA. De Rújula, H. David Politzer et al.Physical Review Lettersprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of A. De Rújula's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by A. De Rújula with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. De Rújula more than expected).
This network shows the impact of papers produced by A. De Rújula. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by A. De Rújula. The network helps show where A. De Rújula may publish in the future.
Co-authorship network of co-authors of A. De Rújula
This figure shows the co-authorship network connecting the top 25 collaborators of A. De Rújula.
A scholar is included among the top collaborators of A. De Rújula based on the total number of
citations received by their joint publications. Widths of edges
represent the number of papers authors have co-authored together.
Node borders
signify the number of papers an author published with A. De Rújula. A. De Rújula is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
20 of 20 papers shown
1.
Rújula, A. De, Joseph Lykken, M. Pierini, C. Rogan, & M. Spiropulu. (2010). Higgs boson look-alikes at the LHC. Physical review. D. Particles, fields, gravitation, and cosmology. 82(1).87 indexed citations
Dado, S., Ajaz A. Dar, & A. De Rújula. (2008). XRF 080109 in NGC2770: detectable superluminal motion.. GRB Coordinates Network. 7174. 1.1 indexed citations
Cohen, Andrew G., A. De Rújula, & Sheldon L. Glashow. (1997). A MATTER–ANTIMATTER UNIVERSE?. Rare & Special e-Zone (The Hong Kong University of Science and Technology).96 indexed citations
12.
Rújula, A. De. (1986). Are there more than four. 323(6091). 760–761.1 indexed citations
Rújula, A. De, Howard Georgi, & H. David Politzer. (1977). Trouble withξscaling?. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 15(9). 2495–2502.47 indexed citations
18.
Rújula, A. De, Howard Georgi, & Sheldon L. Glashow. (1976). Is Charm Found?. Physical Review Letters. 37(7). 398–401.112 indexed citations
19.
Rújula, A. De, Howard Georgi, & Sheldon L. Glashow. (1975). Are Heavy Leptons Found?. Physical Review Letters. 35(10). 628–631.15 indexed citations
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
bibliographic database. While OpenAlex provides broad and valuable coverage of the global
research landscape, it—like all bibliographic datasets—has inherent limitations. These include
incomplete records, variations in author disambiguation, differences in journal indexing, and
delays in data updates. As a result, some metrics and network relationships displayed in
Rankless may not fully capture the entirety of a scholar's output or impact.