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pro vyhledávání: '"Novak, J��r��me"'
We make extensive numerical studies of masses and radii of proto-neutron stars during the first second after their birth in core-collapse supernova events. We use a quasi-static approach for the computation of proto-neutron star structure, built on p
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https://explore.openaire.eu/search/publication?articleId=doi_________::65294c6d36bdb4687f0cb03160e4e61b
We present a numerical model for uniformly rotating superfluid neutron stars, for the first time with realistic microphysics including entrainment, in a fully general relativistic framework. We compute stationary and axisymmetric configurations of ne
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https://explore.openaire.eu/search/publication?articleId=doi_________::42b46f7efe9692fdf94909a7d3bb6345
Autor:
Tiec, Alexandre Le, Novak, J��r��me
The existence of gravitational radiation is a natural prediction of any relativistic description of the gravitational interaction. In this chapter, we focus on gravitational waves, as predicted by Einstein's general theory of relativity. First, we in
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https://explore.openaire.eu/search/publication?articleId=doi_________::a1df2abd28104c4c5a4bc012707136f3
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
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https://explore.openaire.eu/search/publication?articleId=doi_________::acb68a32328aa24a82066ed4d4c8eff3
Equations arising in General Relativity are usually too complicated to be solved analytically and one has to rely on numerical methods to solve sets of coupled partial differential equations. Among the possible choices, this paper focuses on a class
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https://explore.openaire.eu/search/publication?articleId=doi_________::acdf51367f9145eb141b2659689fbfc4