Zobrazeno 1 - 10 of 128 pro vyhledávání: '"Serge Bouquet"'
1
Acoustic stability of nonadiabatic high-energy-density shocks
Autor: Ernazar Abdikamalov, César Huete, Francisco Cobos-Campos, Serge Bouquet
Publikováno v: Physical Review Fluids
Physical Review Fluids, American Physical Society, 2020, 5 (11), ⟨10.1103/PhysRevFluids.5.113403⟩
e-Archivo. Repositorio Institucional de la Universidad Carlos III de Madrid
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As predicted by D'yakov [Shock wave stability, Zh. Eksp. Teor. Fiz. 27, 288 (1954)] and Kontorovich [On the shock waves stability, Zh. Eksp. Teor. Fiz. 33, 1525 (1957)], an initially disturbed shock front may exhibit different asymptotic behaviors, d
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f63fef8ed56e8a9e9bf8bf17b26a29b6
https://hal.archives-ouvertes.fr/hal-03209540
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2
HADES code for numerical simulations of high-mach number astrophysical radiative flows
Autor: H. C. Nguyen, L. Di Menza, M. Mancini, Claire Michaut, Serge Bouquet
Publikováno v: High Energy Density Physics
High Energy Density Physics, Elsevier, 2017, 22, pp.77-89. ⟨10.1016/j.hedp.2017.01.001⟩
The understanding of astrophysical phenomena requires to deal with robust numerical tools in order to handle realistic scales in terms of energy, characteristic lengths and Mach number that cannot be easily reproduced by means of laboratory experimen
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::80ce5358f10b261f718fe2fab6d874e9
https://hal.archives-ouvertes.fr/hal-02264303
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3
Numerical study of the adiabatic index effect for the Vishniac instability in supernova remnants
Autor: C. Cavet, Christophe Sauty, Claire Michaut, Serge Bouquet, Fabrice Roy, H. C. Nguyen
Publikováno v: Astrophysics and Space Science
Astrophysics and Space Science, 2011, 336, pp.183-187. ⟨10.1007/s10509-011-0688-8⟩
International audience; The Vishniac instability is supposed to explain the fragmentation of the thin shell of shocked matter in the radiative phase of supernova remnants. However its implication and its consequence on the morphological evolution of
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::42071a958affb47185685462840c030d
https://doi.org/10.1007/s10509-011-0688-8
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4
Theoretical and numerical studies of the Vishniac instability in supernova remnants
Autor: C. Cavet, Claire Michaut, H. C. Nguyen, Emeric Falize, Serge Bouquet, Laurent Di Menza
Publikováno v: Astrophysics and Space Science
Astrophysics and Space Science, 2009, 322, pp.91-95. ⟨10.1007/s10509-008-9926-0⟩
International audience; Vishniac instability has been theoretically studied in supernova remnants where it is supposed to explain the fragmentation of the interstellar medium. However its role is not fully demonstrated in these astrophysical objects.
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4889a09b473e0061f256775e4439a9b1
https://doi.org/10.1007/s10509-008-9926-0
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5
Analytical study of the buoyancy–drag equation
Autor: Pierre Gandeboeuf, Serge Bouquet, Pierre Pailhoriès
Publikováno v: Mathematical Methods in the Applied Sciences. 30:2027-2035
The buoyancy–drag equation (BDE) is used for describing the time evolution of the mixing zone, between two fluids, due to Rayleigh–Taylor instabilities in a highly non-linear regime. The BDE is similar to an equation of motion for each fluid and,
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::bad241933b96359ba737684b6222a70a
https://doi.org/10.1002/mma.944
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6
Theoretical and Experimental Studies of Radiative Shocks
Autor: G. Herpe, Stefano Atzeni, Serge Bouquet, L. Boireau, Alessandra Benuzzi-Mounaix, N. Osaki, Berenice Loupias, Tommaso Vinci, C. Michaut, Emeric Falize, M. Koenig
Publikováno v: Astrophysics and Space Science
Astrophysics and Space Science, 2007, 307, pp.159-164. ⟨10.1007/s10509-006-9203-z⟩
International audience; This paper deals with the radiative shock from both theoretical and numerical points of view. It is based on the whole experimental results obtained at Laboratoire d'Utilisation des Lasers Intenses (LULI, École Polytechnique)
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ade8336c30b8a231bea8e51e8c8dc19a
https://doi.org/10.1007/s10509-006-9203-z
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7
Laser-driven shock waves for the study of extreme matter states
Autor: Alessandra Ravasio, Angelo Schiavi, T. R. Boehly, T. A. Pikuz, Tommaso Vinci, Dimitri Batani, C. A. Cecchetti, Serge Bouquet, Stefano Atzeni, G. Huser, Marco Borghesi, S. Le Pape, P. K. Patel, M. M. Notley, Norimasa Ozaki, Yefim Aglitskiy, Damien Hicks, E. A. Henry, H. S. Park, R. Dezulian, A. J. Mackinnon, M. Rabec Le Gloahec, M. Koenig, C. Michaut, R. Clark, A. Y. Faenov, Alessandra Benuzzi-Mounaix, S Bandyopadhyay, K. A. Tanaka, Berenice Loupias
Publikováno v: Plasma Physics and Controlled Fusion
Plasma Physics and Controlled Fusion, 2006, 48, pp.347-B358. ⟨10.1088/0741-3335/48/12B/S32⟩
International audience; During the last ten years, the ability of high power lasers to generate high energy density shocks has made them a reliable tool to study extreme states of matter. These states of matter are relevant in many important physics
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3514f30f77cecda4b330388fb0696377
https://doi.org/10.1088/0741-3335/48/12b/s32
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