Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Simon Rozier"'
Autor:
Simon Rozier, Raphaël Errani
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 1, p 91 (2024)
Placed slightly out of dynamical equilibrium, an isolated stellar system quickly returns toward a steady virialized state. We study this process of collisionless relaxation using the matrix method of linear response theory. We show that the full phas
Externí odkaz:
https://doaj.org/article/465b3506309945a39fd35d7622b94ee4
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, ⟨10.1093/mnras/stab2596⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, ⟨10.1093/mnras/stab2596⟩
Globular clusters contain a finite number of stars. As a result, they inevitably undergo secular evolution (`relaxation') causing their mean distribution function (DF) to evolve on long timescales. On one hand, this long-term evolution may be interpr
Autor:
Jean-Baptiste Fouvry, Douglas C. Heggie, Christophe Pichon, Simon Rozier, Anna Lisa Varri, Philip G. Breen
Publikováno v:
Proceedings of the International Astronomical Union. 14:494-497
Recent observations of globular clusters imposed major revisions to the previous paradigm, in which they were considered to be isotropic in velocity space and non-rotating. However, the theory of collisionless spheroids with some kinematic richness h
Publikováno v:
Physical Review D
Physical Review D, American Physical Society, 2018, 97 (8), pp.083502. ⟨10.1103/PhysRevD.97.083502⟩
Phys.Rev.D
Phys.Rev.D, 2018, 97 (8), pp.083502. ⟨10.1103/PhysRevD.97.083502⟩
Phys.Rev.D, 2018, 97 (8), pp.083502. 〈10.1103/PhysRevD.97.083502〉
Physical Review D, American Physical Society, 2018, 97 (8), pp.083502. ⟨10.1103/PhysRevD.97.083502⟩
Phys.Rev.D
Phys.Rev.D, 2018, 97 (8), pp.083502. ⟨10.1103/PhysRevD.97.083502⟩
Phys.Rev.D, 2018, 97 (8), pp.083502. 〈10.1103/PhysRevD.97.083502〉
If the symmetry breaking responsible for axion dark matter production occurs during the radiation-dominated epoch in the early Universe, then this produces large amplitude perturbations that collapse into dense objects known as axion miniclusters. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d5513629ebf3c7a6d1c6587a0621408
https://hal.archives-ouvertes.fr/hal-01768113
https://hal.archives-ouvertes.fr/hal-01768113