M. Fortin

1.6k total citations · 2 hit papers
29 papers, 1.1k citations indexed

About

M. Fortin is a scholar working on Astronomy and Astrophysics, Geophysics and Nuclear and High Energy Physics. According to data from OpenAlex, M. Fortin has authored 29 papers receiving a total of 1.1k indexed citations (citations by other indexed papers that have themselves been cited), including 29 papers in Astronomy and Astrophysics, 16 papers in Geophysics and 8 papers in Nuclear and High Energy Physics. Recurrent topics in M. Fortin's work include Pulsars and Gravitational Waves Research (29 papers), Gamma-ray bursts and supernovae (17 papers) and High-pressure geophysics and materials (16 papers). M. Fortin is often cited by papers focused on Pulsars and Gravitational Waves Research (29 papers), Gamma-ray bursts and supernovae (17 papers) and High-pressure geophysics and materials (16 papers). M. Fortin collaborates with scholars based in Poland, France and Portugal. M. Fortin's co-authors include Constança Providência, P. Haensel, J. L. Zdunik, M. Bejger, Ad. R. Raduta, Sidney S. Avancini, B. K. Agrawal, Naosad Alam, F. Gulminelli and Tuhin Malik and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Physical review. D.

In The Last Decade

M. Fortin

28 papers receiving 1.0k citations

Hit Papers

align trajectories

What are hit papers?

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.

Neutron star radii and crusts: Uncertainties and unified equations of state

2016 229 citations M. Fortin, Constança Providência et al. Physical review. C profile →
GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability

2018 198 citations Tuhin Malik, Naosad Alam et al. Physical review. C profile →

Peers

M. Fortin

AA

GEOPH

NHEP

OCEAN

AMPO

G. Raaijmakers Netherlands

Thomas E. Riley Netherlands

Eemeli Annala Finland

Lukas R. Weih Germany

Sophia Han United States

Helena Pais Portugal

Oleg Kargaltsev United States

Brendan T. Reed United States

Tuhin Malik Portugal

H. Grigorian Armenia

G. Raaijmakers Netherlands

M. Fortin

820 ×0.8

AA

222 ×0.5

GEOPH

223 ×0.7

NHEP

181 ×0.9

OCEAN

111 ×0.8

AMPO

Citations per year, relative to M. Fortin M. Fortin (= 1×) peers G. Raaijmakers

Countries citing papers authored by M. Fortin

Since Specialization

Citations

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

Fields of papers citing papers by M. Fortin

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of M. Fortin. A scholar is included among the top collaborators of M. Fortin 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. Fortin. M. Fortin is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

1.

Zdunik, J. L., et al.. (2022). Partially accreted crusts of neutron stars. Astronomy and Astrophysics. 662. A63–A63. 7 indexed citations

2.

Fortin, M., et al.. (2022). Polytropic fits of modern and unified equations of state. Physical review. C. 106(3). 5 indexed citations

3.

Fortin, M., et al.. (2021). Influence of the crust on the neutron star macrophysical quantities and universal relations. Physical review. C. 104(1). 29 indexed citations

4.

Gusakov, M. E., et al.. (2019). Bulk viscosity in neutron stars with hyperon cores. Physical review. D. 100(10). 22 indexed citations

5.

Gusakov, M. E., et al.. (2019). R-mode stabilization in neutron stars with hyperon cores. Journal of Physics Conference Series. 1400(2). 22029–22029. 4 indexed citations

6.

Haskell, B., J. L. Zdunik, M. Fortin, et al.. (2018). Fundamental physics and the absence of sub-millisecond pulsars. Astronomy and Astrophysics. 620. A69–A69. 20 indexed citations

7.

Fortin, M., Micaela Oertel, & Constança Providência. (2018). Hyperons in hot dense matter: what do the constraints tell us for equation of state?. Publications of the Astronomical Society of Australia. 35. 36 indexed citations

8.

Malik, Tuhin, Naosad Alam, M. Fortin, et al.. (2018). GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability. Physical review. C. 98(3). 198 indexed citations breakdown →

9.

Bejger, M., D. Blaschke, P. Haensel, J. L. Zdunik, & M. Fortin. (2017). Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars. Astronomy and Astrophysics. 600. A39–A39. 34 indexed citations

10.

Fortin, M., et al.. (2017). Neutrino luminosities and heat capacities of neutron stars in analytic form. Physical review. D. 96(4). 11 indexed citations

11.

Fortin, M., Sidney S. Avancini, Constança Providência, & Isaac Vidaña. (2017). Hypernuclei and massive neutron stars. Physical review. C. 95(6). 87 indexed citations

12.

Zdunik, J. L., M. Fortin, & P. Haensel. (2016). Neutron star properties and the equation of state for the core. Astronomy and Astrophysics. 599. A119–A119. 31 indexed citations

13.

Alam, Naosad, B. K. Agrawal, M. Fortin, et al.. (2016). Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation. Physical review. C. 94(5). 67 indexed citations

14.

Fortin, M., Constança Providência, Ad. R. Raduta, et al.. (2016). Neutron star radii and crusts: Uncertainties and unified equations of state. Physical review. C. 94(3). 229 indexed citations breakdown →

15.

Beznogov, Mikhail V., M. Fortin, P. Haensel, D. G. Yakovlev, & J. L. Zdunik. (2016). Cooling of neutron stars with diffusive envelopes. Monthly Notices of the Royal Astronomical Society. 463(2). 1307–1313. 10 indexed citations

16.

Fortin, M., J. L. Zdunik, P. Haensel, & M. Bejger. (2015). Neutron stars with hyperon cores: stellar radii and equation of state near nuclear density. Springer Link (Chiba Institute of Technology). 29 indexed citations

17.

Fortin, M., M. Bejger, P. Haensel, & J. L. Zdunik. (2015). Progenitor neutron stars of the lightest and heaviest millisecond pulsars. Astronomy and Astrophysics. 586. A109–A109. 10 indexed citations

18.

Bejger, M., M. Fortin, P. Haensel, & J. L. Zdunik. (2011). Implications of the measured parameters of PSR J1903+0327 for its progenitor neutron star. Springer Link (Chiba Institute of Technology). 10 indexed citations

19.

Bejger, M., J. L. Zdunik, P. Haensel, & M. Fortin. (2011). Compression of matter in the center of accreting neutron stars. Astronomy and Astrophysics. 536. A92–A92. 12 indexed citations

20.

Margueron, J., et al.. (2011). Thermalization time of hot neutron star crust. Journal of Physics Conference Series. 321. 12031–12031. 2 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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