Edmund Bertschinger
About
In The Last Decade
Edmund Bertschinger
88 papers receiving 3.9k citations
Hit Papers
Peers
Comparison fields: 5 of 75
- Astronomy and Astrophysics 3.7k
- Nuclear and High Energy Physics 1.8k
- Instrumentation 698
- Statistical and Nonlinear Physics 465
- Atomic and Molecular Physics, and Optics 95
Countries citing papers authored by Edmund Bertschinger
This map shows the geographic impact of Edmund Bertschinger'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 Edmund Bertschinger with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Edmund Bertschinger more than expected).
Fields of papers citing papers by Edmund Bertschinger
This network shows the impact of papers produced by Edmund Bertschinger. 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 Edmund Bertschinger. The network helps show where Edmund Bertschinger may publish in the future.
Co-authorship network of co-authors of Edmund Bertschinger
This figure shows the co-authorship network connecting the top 25 collaborators of Edmund Bertschinger. A scholar is included among the top collaborators of Edmund Bertschinger 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 Edmund Bertschinger. Edmund Bertschinger is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 0 | |
| 3 | Providing a Timely Review of Input Demographics to Advisory Committees | 1 |
| 4 | An extension of the Faddeev–Jackiw technique to fields in curved spacetimes | 4 |
| 5 | GRAFIC-2: Multiscale Gaussian Random Fields for Cosmological Simulations | 1 |
| 6 | A Generalized Secondary Infall Model | 1 |
| 7 | Hierarchical phase space structure of dark matter haloes: Tidal debris, caustics, and dark matter annihilation | 2 |
| 8 | 23 | |
| 9 | Self-Similar Evolution of Gravitational Clustering II: N-Body Simulations of the n = −2 Spectrum | 21 |
| 10 | Gravitational Simulations of Cosmic Structure Formation | 1 |
| 11 | Accurate Calculations of CMB Anistropies in Cold and Mixed Dark Matter Models | 1 |
| 12 | Cosmics : cosmological initial conditions and microwave anisotropy codes | 2 |
| 13 | Cosmological dynamics: Course 1 | 19 |
| 14 | 3 | |
| 15 | Stability of the Expansion Wave Solution of Collapsing Isothermal Spheres | 3 |
| 16 | Large Cosmological N-Body Simulations | 1 |
| 17 | The Kinematics and Luminosity of Supernova Remnants Evolving in Homogeneous Uniform Media | 1 |
| 18 | Numerical Simulations of Secondary Infall onto Galaxies | 1 |
| 19 | 27 | |
| 20 | Self-Similar Growth of Cosmological Voids | 1 |
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.