Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Loïc Perot"'
Autor:
Loïc Perot, Nicolas Chamel
Publikováno v:
Universe, Vol 9, Iss 9, p 382 (2023)
In 1995, Glendenning, Kettner and Weber postulated the existence of a new class of compact stars resembling white dwarfs but containing a small strange quark-matter core surrounded by hadronic layers attaining much higher densities than those found i
Externí odkaz:
https://doaj.org/article/922c34f614d248209189eec959f7759a
Autor:
Loïc Perot, Nicolas Chamel
Publikováno v:
Physical Sciences Forum, Vol 7, Iss 1, p 3 (2023)
Space-based gravitational-wave detectors, such as the Laser Interferometer Space Antenna, allow for the probing of the interior of white dwarfs in binaries through the imprints of tidal effects on the gravitational wave signal. In this study, we have
Externí odkaz:
https://doaj.org/article/e00d1706215045d19fe05c3b87ff8a85
Autor:
Nicolas Chamel, Loïc Perot
Publikováno v:
Physical Review D. 106
Autor:
Nicolas Chamel, Loïc Perot
Publikováno v:
Physical Review C, 103 (2
The role of dense-matter properties in the tidal deformability of a cold nonaccreted neutron star is further investigated. Using the set of Brussels-Montreal unified equations of state, we have computed the gravitoelectric Love numbers $k_\ell$ and t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5512c86c32f5f929e6571cce58e1df2d
http://arxiv.org/abs/2102.02004
http://arxiv.org/abs/2102.02004
Publikováno v:
Phys.Rev.C
Phys.Rev.C, 2020, 101 (1), pp.015806. ⟨10.1103/PhysRevC.101.015806⟩
Physical Review C
Physical Review C, American Physical Society, 2020, 101 (1), pp.015806. ⟨10.1103/PhysRevC.101.015806⟩
Physical Review C, 101
Phys.Rev.C, 2020, 101 (1), pp.015806. ⟨10.1103/PhysRevC.101.015806⟩
Physical Review C
Physical Review C, American Physical Society, 2020, 101 (1), pp.015806. ⟨10.1103/PhysRevC.101.015806⟩
Physical Review C, 101
The role of the crust on the tidal deformability of a cold nonaccreted neutron star is studied using the recent unified equation of state BSk24. This equation of state, which is based on the nuclear-energy density functional theory, provides a thermo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92417b7fb5ca63440acb5ea9753f2414
https://hal.archives-ouvertes.fr/hal-02483984
https://hal.archives-ouvertes.fr/hal-02483984
Autor:
Loïc Perot, Nicolas Chamel, A. K. Dutta, Stéphane Goriely, Alexander Y. Potekhin, Anthea Fantina, J. M. Pearson, Camille Ducoin
Publikováno v:
AIP Conf.Proc.
Xiamen-CUSTIPEN Workshop on the EOS of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy
Xiamen-CUSTIPEN Workshop on the EOS of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy, Jan 2019, Xiamen, China. pp.020021, ⟨10.1063/1.5117811⟩
AIP Conference Proceedings, 2127
Xiamen-CUSTIPEN Workshop on the EOS of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy
Xiamen-CUSTIPEN Workshop on the EOS of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy, Jan 2019, Xiamen, China. pp.020021, ⟨10.1063/1.5117811⟩
AIP Conference Proceedings, 2127
The role of the symmetry energy on the internal constitution and the global structure of a cold nonaccreted neutron star is studied using a set of unified equations of state. Based on the nuclear energy-density functional theory, these equations of s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::478108e2a1d2c197929149c4cad9cae0
https://hal.archives-ouvertes.fr/hal-02123345
https://hal.archives-ouvertes.fr/hal-02123345
Publikováno v:
Phys.Rev.C
Phys.Rev.C, 2019, 100 (3), pp.035801. ⟨10.1103/PhysRevC.100.035801⟩
Physical Review C
Physical Review C, American Physical Society, 2019, 100 (3), pp.035801. ⟨10.1103/PhysRevC.100.035801⟩
Physical review. C. Nuclear physics, 100
Phys.Rev.C, 2019, 100 (3), pp.035801. ⟨10.1103/PhysRevC.100.035801⟩
Physical Review C
Physical Review C, American Physical Society, 2019, 100 (3), pp.035801. ⟨10.1103/PhysRevC.100.035801⟩
Physical review. C. Nuclear physics, 100
The role of the symmetry energy and the neutron-matter stiffness on the tidal deformability of a cold nonaccreted neutron star is studied using a set of unified equations of state. Based on the nuclear energy-density functional theory, these equation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c0fbc7081b5b60c52b2da375bf5a1b9
https://hal.archives-ouvertes.fr/hal-02317297
https://hal.archives-ouvertes.fr/hal-02317297