Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Rafael Yunis"'
Publikováno v:
Astronomy Reports. 65:1068-1073
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, 502 (3), pp.4227-4246. ⟨10.1093/mnras/staa3986⟩
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 502 (3), pp.4227-4246. ⟨10.1093/mnras/staa3986⟩
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
The formation and stability of collisionless self-gravitating systems are long standing problems, which date back to the work of D. Lynden-Bell on violent relaxation and extends to the issue of virialization of dark matter (DM) halos. An important pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9210f147c24c6babbd521e614c241491
https://hal.archives-ouvertes.fr/hal-03143591
https://hal.archives-ouvertes.fr/hal-03143591
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We provide a general framework for self-interacting warm dark matter (WDM) in cosmological perturbations, by deriving from first principles a Boltzmann hierarchy which retains certain independence from a particular interaction Lagrangian. We consider
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb5095fd28629f4f7a1d9da437682eaf
https://iopscience.iop.org/article/10.1088/1475-7516/2020/09/041
https://iopscience.iop.org/article/10.1088/1475-7516/2020/09/041
Autor:
Nick E. Mavromatos, Rafael Yunis, A. Krut, Jorge A. Rueda, M. Carinci, Ángeles Moliné, Carlos R. Argüelles, Remo Ruffini
Publikováno v:
Physics of the Dark Universe. 30:100699
The neutrino minimal standard model ($\nu$MSM) has been tightly constrained in the recent years, either from dark matter (DM) production or from X-ray and small-scale observations. However, current bounds on sterile neutrino DM can be significantly m