Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Aurore Blelly"'
Publikováno v:
Physical review. E. 106(4-2)
Perfectly matched layers (PMLs) are widely used in particle-in-cell simulations, in order to absorb electromagnetic waves that propagate out of the simulation domain. However, when charged particles cross the interface between the simulation domain a
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 509 (4), pp.5902-5917. ⟨10.1093/mnras/stab3314⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 509 (4), pp.5902-5917. ⟨10.1093/mnras/stab3314⟩
Mon.Not.Roy.Astron.Soc., 2021, 509 (4), pp.5902-5917. ⟨10.1093/mnras/stab3314⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 509 (4), pp.5902-5917. ⟨10.1093/mnras/stab3314⟩
The forthcoming space-based gravitational wave observatory LISA will open a new window for the measurement of Galactic binaries, which will deliver unprecedented information about these systems. However, the detection of Galactic binary gravitational
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54458a7cbe4b3ba894ba6777db9f2796
http://arxiv.org/abs/2104.05250
http://arxiv.org/abs/2104.05250
Publikováno v:
GECCO '18 Companion
GECCO '18 Companion, Jul 2018, Kyoto, Japan. ⟨10.1145/3205651.3208303⟩
GECCO '18 Companion, Jul 2018, Kyoto, Japan. 2018, 〈10.1145/3205651.3208303〉
GECCO (Companion)
GECCO '18 Companion, Jul 2018, Kyoto, Japan. ⟨10.1145/3205651.3208303⟩
GECCO '18 Companion, Jul 2018, Kyoto, Japan. 2018, 〈10.1145/3205651.3208303〉
GECCO (Companion)
International audience; Benchmarking algorithms is a crucial task to understand them and to make recommendations for which algorithms to use in practice. However, one has to keep in mind that we typically compare only algorithm implementations and th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cbce894bc83c28605228a896db609af4
https://hal.inria.fr/hal-01811588/document
https://hal.inria.fr/hal-01811588/document
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2020, 102 (10), pp.104053. ⟨10.1103/PhysRevD.102.104053⟩
Physical Review D
Phys.Rev.D, 2020, 102 (10), pp.104053. ⟨10.1103/PhysRevD.102.104053⟩
Physical Review D
The detection of galactic binaries as sources of gravitational waves promises an unprecedented wealth of information about these systems, but also raises several challenges in signal processing. In particular the large number of expected sources and