M. Centelles

4.3k total citations · 1 hit paper
86 papers, 3.2k citations indexed

About

M. Centelles is a scholar working on Nuclear and High Energy Physics, Atomic and Molecular Physics, and Optics and Astronomy and Astrophysics. According to data from OpenAlex, M. Centelles has authored 86 papers receiving a total of 3.2k indexed citations (citations by other indexed papers that have themselves been cited), including 73 papers in Nuclear and High Energy Physics, 25 papers in Atomic and Molecular Physics, and Optics and 18 papers in Astronomy and Astrophysics. Recurrent topics in M. Centelles's work include Nuclear physics research studies (70 papers), Quantum Chromodynamics and Particle Interactions (34 papers) and Pulsars and Gravitational Waves Research (17 papers). M. Centelles is often cited by papers focused on Nuclear physics research studies (70 papers), Quantum Chromodynamics and Particle Interactions (34 papers) and Pulsars and Gravitational Waves Research (17 papers). M. Centelles collaborates with scholars based in Spain, India and France. M. Centelles's co-authors include X. Viñas, X. Roca-Maza, M. Warda, J. Piekarewicz, S. K. Patra, B. K. Agrawal, P. Schuck, B. K. Sharma, J. N. De and G. Colò and has published in prestigious journals such as Physical Review Letters, Physics Letters B and Physical Review A.

In The Last Decade

M. Centelles

84 papers receiving 3.1k citations

Hit Papers

Nuclear Symmetry Energy Probed by Neutron Skin Thickness ... 2009 2026 2014 2020 2009 100 200 300 400

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
M. Centelles Spain 28 2.6k 1.1k 839 590 391 86 3.2k
J. R. Stone United Kingdom 23 2.5k 1.0× 1.6k 1.4× 871 1.0× 664 1.1× 293 0.7× 74 3.4k
X. Roca-Maza Italy 25 3.0k 1.2× 1.1k 1.0× 936 1.1× 568 1.0× 541 1.4× 78 3.6k
X. Viñas Spain 31 3.2k 1.2× 1.1k 1.0× 1.3k 1.5× 655 1.1× 469 1.2× 167 3.8k
B. K. Agrawal India 28 2.1k 0.8× 1.5k 1.3× 681 0.8× 540 0.9× 231 0.6× 115 2.9k
H.H. Wolter Germany 31 3.5k 1.4× 1.4k 1.2× 1.3k 1.6× 595 1.0× 439 1.1× 146 4.3k
J. Margueron France 32 1.9k 0.7× 1.6k 1.5× 729 0.9× 710 1.2× 157 0.4× 112 2.9k
S. Typel Germany 35 3.7k 1.4× 2.9k 2.6× 1.3k 1.5× 1.1k 1.9× 429 1.1× 124 5.4k
E. Khan France 31 2.3k 0.9× 475 0.4× 960 1.1× 285 0.5× 381 1.0× 116 2.6k
Brian D. Serot United States 26 3.7k 1.4× 1.4k 1.3× 1.4k 1.7× 707 1.2× 141 0.4× 63 4.4k
M. Di Toro Italy 32 3.0k 1.2× 713 0.6× 990 1.2× 388 0.7× 242 0.6× 203 3.4k

Countries citing papers authored by M. Centelles

Since Specialization
Citations

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

Fields of papers citing papers by M. Centelles

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Centelles

This figure shows the co-authorship network connecting the top 25 collaborators of M. Centelles. A scholar is included among the top collaborators of M. Centelles 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 M. Centelles. M. Centelles 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.
Bhagwat, A., M. Centelles, X. Viñas, & R. Wyss. (2023). Mic–Mac model based on the Wigner–Kirkwood method. The European Physical Journal A. 59(12). 1 indexed citations
2.
Centelles, M., et al.. (2023). Correlations between charge radii differences of mirror nuclei and stellar observables. Physical review. C. 108(1). 13 indexed citations
3.
Viñas, X., et al.. (2022). Finite-range simple effective interaction including tensor terms. Physical review. C. 106(2). 3 indexed citations
4.
Routray, T. R., et al.. (2021). Influence of direct Urca on the r -mode spin down features of newborn neutron star pulsars. Physica Scripta. 96(4). 45301–45301. 4 indexed citations
5.
Centelles, M., et al.. (2021). Finite-size instabilities in finite-range forces. Physical review. C. 103(6). 6 indexed citations
6.
Routray, T. R., et al.. (2021). Reexamination of the N=50 and Z=28 shell closure. Physical review. C. 104(1). 4 indexed citations
7.
Viñas, X., et al.. (2021). Unified equation of state for neutron stars based on the Gogny interaction. Dipòsit Digital de la Universitat de Barcelona (Universitat de Barcelona). 18 indexed citations
8.
Lourenço, O., M. Bhuyan, César H. Lenzi, et al.. (2020). GW170817 constraints analyzed with Gogny forces and momentum-dependent interactions. Physics Letters B. 803. 135306–135306. 13 indexed citations
9.
Pattnaik, Subhaswaraj, T. R. Routray, X. Viñas, et al.. (2018). Addendum: Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction (2018 J. Phys. G: Nucl. Part. Phys. 45 055202). Journal of Physics G Nuclear and Particle Physics. 45(11). 119401–119401. 2 indexed citations
10.
Centelles, M., et al.. (2018). New Gogny interaction suitable for astrophysical applications. Physics Letters B. 779. 195–200. 44 indexed citations
11.
Mondal, C., J. N. De, M. Centelles, et al.. (2017). Searching for a universal correlation among symmetry energy parameters. 62. 72–73. 1 indexed citations
12.
Tolós, Laura, M. Centelles, & À. Ramos. (2017). The equation of state for the nucleonic and hyperonic core of neutron stars. Dipòsit Digital de la Universitat de Barcelona (Universitat de Barcelona). 66 indexed citations
13.
Roca-Maza, X., B. K. Agrawal, P. F. Bortignon, et al.. (2014). Nuclear Symmetry Energy: constraints from Giant Quadrupole Resonances and Parity Violating Electron Scattering. Springer Link (Chiba Institute of Technology). 3 indexed citations
14.
Roca-Maza, X., M. Centelles, X. Viñas, & M. Warda. (2011). Neutron Skin ofPb208, Nuclear Symmetry Energy, and the Parity Radius Experiment. Physical Review Letters. 106(25). 252501–252501. 293 indexed citations
15.
Roca-Maza, X., X. Viñas, M. Centelles, P. Ring, & Peter Schuck. (2011). Relativistic mean-field interaction with density-dependent meson-nucleon vertices based on microscopical calculations. Physical Review C. 84(5). 146 indexed citations
16.
Centelles, M., X. Roca-Maza, X. Viñas, & M. Warda. (2009). Nuclear Symmetry Energy Probed by Neutron Skin Thickness of Nuclei. Physical Review Letters. 102(12). 122502–122502. 420 indexed citations breakdown →
17.
Warda, M., X. Viñas, X. Roca-Maza, & M. Centelles. (2009). Neutron skin thickness in the droplet model with surface width dependence: Indications of softness of the nuclear symmetry energy. Physical Review C. 80(2). 162 indexed citations
18.
Guilleumas, M., M. Centelles, M. Barranco, R. Mayol, & M. Pí. (2005). 光格子中,Bose-Fermi混合体の渦核形成に対する臨界周波数. Physical Review A. 72. 1–53602. 4 indexed citations
19.
Sil, Tapas, M. Centelles, X. Viñas, & J. Piekarewicz. (2005). Atomic parity nonconservation, neutron radii, and effective field theories of nuclei. Physical Review C. 71(4). 64 indexed citations
20.
Centelles, M., X. Viñas, M. Barranco, & P. Schuck. (1990). On the relativistic extended Thomas-Fermi method. Nuclear Physics A. 519(1-2). 73–82. 28 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.

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