Silvia Mollerach
- Astronomy and Astrophysics top 2%
- Nuclear and High Energy Physics top 5%
- Oceanography top 10%
- Statistical and Nonlinear Physics top 10%
- Finance top 10%
- Co-authors
- S. MatarreseF. LucchinAlejandro GanguiEsteban RouletA. OrtolanMarco BruniG. GolupDiego Harari
- Topics
- Cosmology and Gravitation Theories (8 papers)Dark Matter and Cosmic Phenomena (5 papers)Geophysics and Gravity Measurements (3 papers)
- Partner nations
- ItalyArgentinaUnited States
In The Last Decade
Silvia Mollerach
13 papers receiving 784 citations
Peers
Comparison fields: 5 of 40
- Astronomy and Astrophysics 756
- Nuclear and High Energy Physics 477
- Oceanography 79
- Statistical and Nonlinear Physics 64
- Finance 46
Countries citing papers authored by Silvia Mollerach
This map shows the geographic impact of Silvia Mollerach'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 Silvia Mollerach with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Silvia Mollerach more than expected).
Fields of papers citing papers by Silvia Mollerach
This network shows the impact of papers produced by Silvia Mollerach. 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 Silvia Mollerach. The network helps show where Silvia Mollerach may publish in the future.
Co-authorship network of co-authors of Silvia Mollerach
This figure shows the co-authorship network connecting the top 25 collaborators of Silvia Mollerach. A scholar is included among the top collaborators of Silvia Mollerach 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 Silvia Mollerach. Silvia Mollerach 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 | 4 | |
| 3 | 19 | |
| 4 | 10 | |
| 5 | Tests of Gaussianity of CMB Maps | 2 |
| 6 | 25 | |
| 7 | 4 | |
| 8 | Second-order perturbations of the Einstein-de Sitter Universe | 35 |
| 9 | 36 | |
| 10 | The Stochastic Gravitational-Wave Background Produced by Non-Linear Cosmological Perturbations | 1 |
| 11 | 310 | |
| 12 | 0 | |
| 13 | 22 | |
| 14 | 17 | |
| 15 | 61 | |
| 16 | 253 |
About Silvia Mollerach
Silvia Mollerach is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 16 papers that have together received 799 indexed citations. Recurring topics across this work include Cosmology and Gravitation Theories (8 papers), Dark Matter and Cosmic Phenomena (5 papers) and Geophysics and Gravity Measurements (3 papers). The work is most often cited by research in Astronomy and Astrophysics (756 citations), Nuclear and High Energy Physics (477 citations) and Instrumentation (31 citations). Silvia Mollerach has collaborated with scholars based in Italy, Argentina and United States. Frequent co-authors include S. Matarrese, F. Lucchin, Alejandro Gangui, Esteban Roulet, A. Ortolan, Marco Bruni, G. Golup, Diego Harari, J. L. Sanz and J. M. Diego. Their work appears in journals such as The Astrophysical Journal, Physics Reports and Monthly Notices of the Royal Astronomical Society.
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.