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.
Nucleosynthesis, neutrino bursts and γ-rays from coalescing neutron stars
19891.2k citationsDavid Eichler, Mario Livio et al.Natureprofile →
Particle acceleration at astrophysical shocks: A theory of cosmic ray origin
This map shows the geographic impact of David Eichler'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 David Eichler with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites David Eichler more than expected).
This network shows the impact of papers produced by David Eichler. 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 David Eichler. The network helps show where David Eichler may publish in the future.
Co-authorship network of co-authors of David Eichler
This figure shows the co-authorship network connecting the top 25 collaborators of David Eichler.
A scholar is included among the top collaborators of David Eichler 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 David Eichler. David Eichler is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Burns, Eric, A. Tohuvavohu, J. H. Buckley, et al.. (2019). A Summary of Multimessenger Science with Neutron Star Mergers. arXiv (Cornell University). 51(3). 38.4 indexed citations
Eichler, David & M. Pohl. (2011). Can ultrahigh energy cosmic rays come from gamma-ray bursts? Cosmic rays below the ankle and galactic gamma-ray bursts. DESY Publication Database (PUBDB) (Deutsches Elektronen-Synchrotron).10 indexed citations
7.
Eichler, David, D. Guetta, & M. Pohl. (2010). The high energy budget allocations in shocks and gamma ray bursts. DESY Publication Database (PUBDB) (Deutsches Elektronen-Synchrotron).19 indexed citations
Eichler, David, Tsvi Piran, Mario Livio, & David N. Schramm. (1989). Coalescing Neutron Stars, Naked Neutrino Bursts, Gamma Rays Gravitational Radiation, Millisecond Pulsars and r-Process Nucleosynthesis. Nature.2 indexed citations
13.
Wandel, Amri, David Eichler, J. R. Letaw, R. Silberberg, & C. H. Tsao. (1987). Distributed reacceleration of cosmic rays. The Astrophysical Journal. 316. 676–676.32 indexed citations
14.
Ellison, Donald C., F. C. Jones, & David Eichler. (1983). Monte Carlo simulation of steady state shock structure including cosmic ray mediation and particle escape. International Cosmic Ray Conference. 2. 271.1 indexed citations
Eichler, David, M. E. Pesses, & J. R. Jokipii. (1981). Cosmic-Ray Drift, Shock Acceleration and the Anomalous Component of Cosmic Rays. International Cosmic Ray Conference. 3. 463.3 indexed citations
17.
Ellison, Donald C., F. C. Jones, & David Eichler. (1981). Monte Carlo simulation of collisionless shocks showing preferential acceleration of high A/Z particles. 50(2). 110–113.11 indexed citations
18.
Scott, J. S., P. Morrison, Gordon D. Holman, David Eichler, & J. A. Ionson. (1979). On the Escape of Cosmic Rays from Supernova Remnants. International Cosmic Ray Conference. 2. 123.1 indexed citations
19.
Eichler, David. (1979). The Constant-Composition Variable in Shock Acceleration: AN Application to the Earth's Bow Shock. ICRC. 5. 302.4 indexed citations
20.
Eichler, David & David N. Schramm. (1978). High energy neutrino astronomy. Nature. 275(5682). 704–706.10 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.