Philip Mocz

2.3k total citations · 2 hit papers
40 papers, 1.6k citations indexed

About

Philip Mocz is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Computational Mechanics. According to data from OpenAlex, Philip Mocz has authored 40 papers receiving a total of 1.6k indexed citations (citations by other indexed papers that have themselves been cited), including 37 papers in Astronomy and Astrophysics, 17 papers in Nuclear and High Energy Physics and 5 papers in Computational Mechanics. Recurrent topics in Philip Mocz's work include Galaxies: Formation, Evolution, Phenomena (21 papers), Cosmology and Gravitation Theories (15 papers) and Astrophysics and Star Formation Studies (14 papers). Philip Mocz is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (21 papers), Cosmology and Gravitation Theories (15 papers) and Astrophysics and Star Formation Studies (14 papers). Philip Mocz collaborates with scholars based in United States, Germany and United Kingdom. Philip Mocz's co-authors include Mark Vogelsberger, Lars Hernquist, Anastasia Fialkov, Rüdiger Pakmor, Volker Springel, Michael Boylan-Kolchin, Jesús Zavala, Victor H. Robles, Mustafa A. Amin and Federico Marinacci and has published in prestigious journals such as Physical Review Letters, The Astrophysical Journal and Journal of Computational Physics.

In The Last Decade

Philip Mocz

39 papers receiving 1.5k citations

Hit Papers

Improving the convergence properties of the moving-mesh c... 2015 2026 2018 2022 2015 2017 50 100 150 200 250

Peers

Philip Mocz
Philip A. Pinto United States
M. Haverkorn Netherlands
Gagandeep S. Anand United States
Britton Smith United States
Wenlong Yuan United States
D. O. Jones United States
N. Aghanim France
Achim Weiß Germany
Philip Mocz
Citations per year, relative to Philip Mocz Philip Mocz (= 1×) peers Hsi-Yu Schive

Countries citing papers authored by Philip Mocz

Since Specialization
Citations

This map shows the geographic impact of Philip Mocz'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 Philip Mocz with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Philip Mocz more than expected).

Fields of papers citing papers by Philip Mocz

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Philip Mocz. 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 Philip Mocz. The network helps show where Philip Mocz may publish in the future.

Co-authorship network of co-authors of Philip Mocz

This figure shows the co-authorship network connecting the top 25 collaborators of Philip Mocz. A scholar is included among the top collaborators of Philip Mocz 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 Philip Mocz. Philip Mocz 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.
Pozzo, Ana Lillian Martin‐Del, Razieh Emami, Philip Mocz, et al.. (2025). Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint. Astronomy and Astrophysics. 699. A308–A308.
2.
Boylan-Kolchin, Michael, et al.. (2024). An attractive model: simulating fuzzy dark matter with attractive self-interactions. Monthly Notices of the Royal Astronomical Society. 533(2). 2454–2472. 8 indexed citations
3.
Mocz, Philip, Anastasia Fialkov, Mark Vogelsberger, et al.. (2023). Cosmological structure formation and soliton phase transition in fuzzy dark matter with axion self-interactions. Monthly Notices of the Royal Astronomical Society. 521(2). 2608–2615. 26 indexed citations
4.
Besla, Gurtina, Philip Mocz, Nicolás Garavito-Camargo, et al.. (2023). Structure, Kinematics, and Observability of the Large Magellanic Cloud’s Dynamical Friction Wake in Cold versus Fuzzy Dark Matter. The Astrophysical Journal. 954(2). 163–163. 12 indexed citations
5.
Fialkov, Anastasia, et al.. (2023). Cosmic web dissection in fuzzy dark matter cosmologies. Monthly Notices of the Royal Astronomical Society. 525(1). 348–363. 10 indexed citations
6.
Mocz, Philip, et al.. (2023). Nested solitons in two-field fuzzy dark matter. Monthly Notices of the Royal Astronomical Society. 527(2). 4162–4172. 3 indexed citations
7.
Fialkov, Anastasia, et al.. (2022). On the cosmic web elongation in fuzzy dark matter cosmologies: Effects on density profiles, shapes, and alignments of haloes. Monthly Notices of the Royal Astronomical Society. 519(3). 4183–4202. 14 indexed citations
8.
Beattie, James R., Mark R. Krumholz, Raphael Skalidis, et al.. (2022). Energy balance and Alfvén Mach numbers in compressible magnetohydrodynamic turbulence with a large-scale magnetic field. Monthly Notices of the Royal Astronomical Society. 515(4). 5267–5284. 17 indexed citations
9.
Beattie, James R., Philip Mocz, Christoph Federrath, & Ralf S. Klessen. (2022). The density distribution and physical origins of intermittency in supersonic, highly magnetized turbulence with diverse modes of driving. Monthly Notices of the Royal Astronomical Society. 517(4). 5003–5031. 14 indexed citations
10.
Mocz, Philip, Anastasia Fialkov, Mark Vogelsberger, et al.. (2020). Galaxy formation with BECDM – II. Cosmic filaments and first galaxies. Monthly Notices of the Royal Astronomical Society. 494(2). 2027–2044. 69 indexed citations
11.
Mocz, Philip, et al.. (2020). Fuzzy dark matter soliton cores around supermassive black holes. Monthly Notices of the Royal Astronomical Society. 492(4). 5721–5729. 45 indexed citations
12.
Mocz, Philip, Anastasia Fialkov, Mark Vogelsberger, et al.. (2019). First Star-Forming Structures in Fuzzy Cosmic Filaments. Physical Review Letters. 123(14). 141301–141301. 105 indexed citations
13.
Christian, Pierre, Philip Mocz, & Abraham Loeb. (2018). Evolution of the Black Hole Mass Function in Star Clusters from Multiple Mergers. The Astrophysical Journal Letters. 858(1). L8–L8. 7 indexed citations
14.
Hull, Charles L. H., Philip Mocz, Blakesley Burkhart, et al.. (2017). Unveiling the Role of the Magnetic Field at the Smallest Scales of Star Formation. The Astrophysical Journal Letters. 842(2). L9–L9. 40 indexed citations
15.
Mocz, Philip, Mark Vogelsberger, Victor H. Robles, et al.. (2017). Galaxy formation with BECDM – I. Turbulence and relaxation of idealized haloes. Monthly Notices of the Royal Astronomical Society. 471(4). 4559–4570. 227 indexed citations breakdown →
16.
Mocz, Philip & Sauro Succi. (2015). Numerical solution of the nonlinear Schrödinger equation using smoothed-particle hydrodynamics. Physical Review E. 91(5). 53304–53304. 63 indexed citations
17.
Celotti, A., et al.. (2014). Do high-redshift quasars have powerful jets?. Monthly Notices of the Royal Astronomical Society Letters. 442(1). L81–L84. 27 indexed citations
18.
Mocz, Philip, Mark Vogelsberger, & Lars Hernquist. (2014). A constrained transport scheme for MHD on unstructured static and moving meshes. Monthly Notices of the Royal Astronomical Society. 442(1). 43–55. 35 indexed citations
19.
Mocz, Philip, et al.. (2014). Interpreting MAD within multiple accretion regimes. Monthly Notices of the Royal Astronomical Society. 447(2). 1498–1503. 2 indexed citations
20.
Mocz, Philip, A. C. Fabian, & Katherine M. Blundell. (2011). Inverse-Compton ghosts and double-lobed radio sources in the X-ray sky. Monthly Notices of the Royal Astronomical Society. 413(2). 1107–1120. 25 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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026