Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Aurélien Sourie"'
Autor:
Nicolas Chamel, Aurélien Sourie
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 493 (1), pp.L98-L102. ⟨10.1093/mnrasl/slaa015⟩
Royal Astronomical Society. Monthly Notices. Letters
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 493 (1), pp.L98-L102. ⟨10.1093/mnrasl/slaa015⟩
Royal Astronomical Society. Monthly Notices. Letters
Timing of the Crab and Vela pulsars have recently revealed very peculiar evolutions of their spin frequency during the early stage of a glitch. We show that these differences can be interpreted from the interactions between neutron superfluid vortice
Autor:
Aurélien Sourie, Nicolas Chamel
Publikováno v:
International journal of modern physics b, 34 (10
The hydrodynamic forces acting on a quantized vortex in a superfluid have long been a highly controversial issue. A new approach, originally developed in the astrophysical context of compact stars, is presented to determine these forces by considerin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::442d64a526e60aa4b1d9e731b2ad197b
http://arxiv.org/abs/2202.06011
http://arxiv.org/abs/2202.06011
Autor:
Aurélien Sourie, Nicolas Chamel
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 503 (1), pp.1407-1417. ⟨10.1093/mnras/stab606⟩
Monthly notices of the Royal Astronomical Society, 503 (1
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 503 (1), pp.1407-1417. ⟨10.1093/mnras/stab606⟩
Monthly notices of the Royal Astronomical Society, 503 (1
Our recent Newtonian treatment of the smooth-averaged mutual-friction force acting on the neutron superfluid and locally induced by the pinning of quantized neutron vortices to proton fluxoids in the outer core of superfluid neutron stars is here ada
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::efe61834132f80f4c1280cd58c844f00
https://hal.archives-ouvertes.fr/hal-03164443
https://hal.archives-ouvertes.fr/hal-03164443
Autor:
Aurélien Sourie, Nicolas Chamel
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 493 (1), pp.382-389. ⟨10.1093/mnras/staa253⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 493 (1), pp.382-389. ⟨10.1093/mnras/staa253⟩
Monthly notices of the Royal Astronomical Society, 493 (1
Monthly notices of the Royal Astronomical Society
Mon.Not.Roy.Astron.Soc., 2020, 493 (1), pp.382-389. ⟨10.1093/mnras/staa253⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 493 (1), pp.382-389. ⟨10.1093/mnras/staa253⟩
Monthly notices of the Royal Astronomical Society, 493 (1
Monthly notices of the Royal Astronomical Society
The superfluid and superconducting core of a cold rotating neutron star (NS) is expected to be threaded by a tremendous number of neutron quantized vortices and proton fluxoids. Their interactions are unavoidable and may have important astrophysical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::67b71fe4f0cdd02ea1fae3e11439c8bb
http://arxiv.org/abs/2001.08964
http://arxiv.org/abs/2001.08964
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
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
Publikováno v:
The Fourteenth Marcel Grossmann Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories. World Scientific Publishing Co. Pte. Ltd.
14th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories
14th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories, Jul 2015, Rome, Italy. pp.4125-4130, ⟨10.1142/9789813226609_0551⟩
14th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories
14th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories, Jul 2015, Rome, Italy. pp.4125-4130, ⟨10.1142/9789813226609_0551⟩
International audience; We describe recent progress in the modelling of realistic equilibrium configurations of rotating superfluid neutron stars, in a fully general relativistic framework. We compute stationary and axisymmetric configurations of neu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02cd15f116aa402ddf8ed182cd9f2f1d
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/301581
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/301581
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2017, 464 (4), pp.4641-4657. ⟨10.1093/mnras/stw2613⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 464 (4), pp.4641-4657. ⟨10.1093/mnras/stw2613⟩
Mon.Not.Roy.Astron.Soc., 2017, 464 (4), pp.4641-4657. 〈10.1093/mnras/stw2613〉
Mon.Not.Roy.Astron.Soc., 2017, 464 (4), pp.4641-4657. ⟨10.1093/mnras/stw2613⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 464 (4), pp.4641-4657. ⟨10.1093/mnras/stw2613⟩
Mon.Not.Roy.Astron.Soc., 2017, 464 (4), pp.4641-4657. 〈10.1093/mnras/stw2613〉
In this paper, we study in detail the role of general relativity on the global dynamics of giant pulsar glitches as exemplified by Vela. For this purpose, we carry out numerical simulations of the spin up triggered by the sudden unpinning of superflu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c213eec8090239176435ca49849d125f
https://hal.archives-ouvertes.fr/hal-01554210
https://hal.archives-ouvertes.fr/hal-01554210
Publikováno v:
Proceedings of The Modern Physics of Compact Stars 2015 (MPCS2015)
Realistic global neutron star models require numerical approach. Here, we briefly motivate and recall the general-relativistic framework for the description of rotating compact stars and show how global observable quantities can be computed unambiguo