Zobrazeno 1 - 10
of 204
pro vyhledávání: '"Jean‐Michel Alimi"'
Autor:
Majd Shalak, Jean-Michel Alimi
Publikováno v:
Physical Sciences Forum, Vol 7, Iss 1, p 53 (2023)
In this paper, we study the dynamical and statistical properties of the cosmic web and investigate their ability to infer the corresponding cosmological model. Our definition of the cosmic web is based on the local dimensionality of the gravitational
Externí odkaz:
https://doaj.org/article/c983724b00ac49489ea1cd02d56e5c39
Autor:
Rémy Koskas, Jean-Michel Alimi
Publikováno v:
Physical Sciences Forum, Vol 7, Iss 1, p 25 (2023)
Halo Dark Matter (DM) formation is a complex process, intertwining both gravitational and cosmological nonlinear phenomena. One of the manifestations of this complexity is the shape of the resulting present-day DM halos: simulations and observations
Externí odkaz:
https://doaj.org/article/7184c7b723814f1389721955a1adb012
Publikováno v:
Physical Review D
Physical Review D, American Physical Society, 2020, 101 (2), ⟨10.1103/PhysRevD.101.023512⟩
Physical Review D, American Physical Society, 2020, 101 (2), pp.023512. ⟨10.1103/PhysRevD.101.023512⟩
Phys.Rev.D
Phys.Rev.D, 2020, 101 (2), pp.023512. ⟨10.1103/PhysRevD.101.023512⟩
Physical Review D, American Physical Society, 2020, 101 (2), ⟨10.1103/PhysRevD.101.023512⟩
Physical Review D, American Physical Society, 2020, 101 (2), pp.023512. ⟨10.1103/PhysRevD.101.023512⟩
Phys.Rev.D
Phys.Rev.D, 2020, 101 (2), pp.023512. ⟨10.1103/PhysRevD.101.023512⟩
The late integrated Sachs-Wolfe (ISW) effect correlates the Cosmic Microwave Background (CMB) temperature anisotropies with foreground cosmic large-scale structures. As the correlation depends crucially on the growth history in the era of dark energy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c12b17cf7a5ae25fa1f61b0a57c3c1f8
https://hal.archives-ouvertes.fr/hal-02453823
https://hal.archives-ouvertes.fr/hal-02453823
Autor:
Paul de Fromont, Jean-Michel Alimi
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2018, 475 (2), pp.1912-1924. ⟨10.1093/mnras/stx2948⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 475 (2), pp.1912-1924. ⟨10.1093/mnras/stx2948⟩
Mon.Not.Roy.Astron.Soc., 2018, 475 (2), pp.1912-1924. 〈10.1093/mnras/stx2948〉
Mon.Not.Roy.Astron.Soc., 2018, 475 (2), pp.1912-1924. ⟨10.1093/mnras/stx2948⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 475 (2), pp.1912-1924. ⟨10.1093/mnras/stx2948⟩
Mon.Not.Roy.Astron.Soc., 2018, 475 (2), pp.1912-1924. 〈10.1093/mnras/stx2948〉
The statistical properties of cosmic structures are well known to be strong probes for cosmology. In particular, several studies tried to use the cosmic void counting number to obtain tight constrains on Dark Energy. In this paper we address this que
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5ef53eb932bff437a6bcf89440b372c
https://hal.archives-ouvertes.fr/hal-01807619
https://hal.archives-ouvertes.fr/hal-01807619
Autor:
Paul de Fromont, Jean-Michel Alimi
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, 2018, 473 (4), pp.5177-5194. ⟨10.1093/mnras/stx2677⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2018, 473 (4), pp.5177-5194. ⟨10.1093/mnras/stx2677⟩
Mon.Not.Roy.Astron.Soc., 2018, 473 (4), pp.5177-5194. 〈10.1093/mnras/stx2677〉
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 473 (4), pp.5177-5194. ⟨10.1093/mnras/stx2677⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2018, 473 (4), pp.5177-5194. ⟨10.1093/mnras/stx2677⟩
Mon.Not.Roy.Astron.Soc., 2018, 473 (4), pp.5177-5194. 〈10.1093/mnras/stx2677〉
The absence of a physically motivated model for large scale profiles of cosmic voids limits our ability to extract valuable cosmological information from their study. In this paper, we address this problem by introducing the spherically compensated c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::463eda414be51ba40fd449aecc225d5c
https://hal.archives-ouvertes.fr/hal-01758670
https://hal.archives-ouvertes.fr/hal-01758670
Autor:
Pier Stefano Corasaniti, Vincent Reverdy, Xavier Delaruelle, Jean-Michel Alimi, Irène Balmès, Yann Rasera, Vincent Bouillot, phane Requena, Jean-Noel Richet
Publikováno v:
The International Journal of High Performance Computing Applications. 29:249-260
We report the realization of the first cosmological simulations on the scale of the whole observable universe. These simulations have been carried out on 4752 nodes of the Curie supercomputer as a part of the Dark Energy Universe Simulation: Full Uni
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, 2015, 450 (1), pp.145-159. ⟨10.1093/mnras/stv558⟩
Monthly Notices of the Royal Astronomical Society, 2015, 450 (1), pp.145-159. ⟨10.1093/mnras/stv558⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 450 (1), pp.145-159. ⟨10.1093/mnras/stv558⟩
Monthly Notices of the Royal Astronomical Society, 2015, 450 (1), pp.145-159. ⟨10.1093/mnras/stv558⟩
Observations of colliding galaxy clusters with high relative velocity probe the tail of the halo pairwise velocity distribution with the potential of providing a powerful test of cosmology. As an example it has been argued that the discovery of the B
Publikováno v:
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.2302-2307, ⟨10.1142/9789813226609_0266⟩
14th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories, Jul 2015, Rome, Italy. pp.2302-2307, ⟨10.1142/9789813226609_0266⟩
International audience; We discuss numerical investigations of the effects of cosmological inhomogeneities on light propagation. A new algorithm directly integrating the geodesics equations has been developed and has been run on very large scale cosm
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, 2014, 437 (3), pp.2328-2339. ⟨10.1093/mnras/stt2050⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2014, 437 (3), pp.2328-2339. ⟨10.1093/mnras/stt2050⟩
We study the imprint of Dark Energy on the density profile of Dark Matter halos using a set of high-resolution large volume cosmological N-body simulations from the Dark Energy Universe Simulation Series (DEUSS). We first focus on the analysis of the
Autor:
Jean-Michel Alimi, André Füzfa
Publikováno v:
Fuzfa, A &-M. Alimi, J 2006, ' Is Dark Energy Abnormally Weighting? ', Int.J.Mod.Phys.D, vol. 16, pp. 2587-2592 . https://doi.org/10.1142/S0218271807011206, https://doi.org/10.1142/S0218271807011206
We present a new interpretation of dark energy in terms of an \textit{Abnormally Weighting Energy} (AWE). This means that dark energy does not couple to gravitation in the same way as ordinary matter, yielding a violation of the weak and strong equiv