Zobrazeno 1 - 10
of 71
pro vyhledávání: '"Miguel A Sánchez-Conde"'
Publikováno v:
Physical Review D. 107
Clusters of galaxies are the largest gravitationally-bound systems in the Universe. Their dynamics are dominated by dark matter (DM), which makes them among the best targets for indirect DM searches. We analyze 12 years of data collected by the Fermi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::298628e7d933ff9040c861b8676d4473
https://doi.org/10.1103/physrevd.107.083030
https://doi.org/10.1103/physrevd.107.083030
Autor:
Oliver Newton, Noam I Libeskind, Alexander Knebe, Miguel A Sánchez-Conde, Jenny G Sorce, Sergey Pilipenko, Matthias Steinmetz, Rüdiger Pakmor, Elmo Tempel, Yehuda Hoffman, Mark Vogelsberger
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, 514 (3), pp.3612-3625. ⟨10.1093/mnras/stac1316⟩
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2022, 514, pp.3612-3625. ⟨10.1093/mnras/stac1316⟩
Monthly Notices of the Royal Astronomical Society, 2022, 514 (3), pp.3612-3625. ⟨10.1093/mnras/stac1316⟩
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2022, 514, pp.3612-3625. ⟨10.1093/mnras/stac1316⟩
The Local Group is a unique environment in which to study the astrophysics of galaxy formation. The proximity of the Milky Way and M31 enhances the frequency of interactions of the low-mass halo population with more massive dark matter haloes, which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1cc60dc80883acb558d65c7f170e75aa
https://doi.org/10.1093/mnras/stac1316
https://doi.org/10.1093/mnras/stac1316
Publikováno v:
Galaxies, Vol 8, Iss 1, p 5 (2019)
The Λ CDM cosmological framework predicts the existence of thousands of subhalos in our own Galaxy not massive enough to retain baryons and become visible. Yet, some of them may outshine in gamma rays provided that the dark matter is made of weakly
Externí odkaz:
https://doaj.org/article/efb8ae50ce2b446a95dd36054556ab89
In this work, we carry out a suite of specially-designed numerical simulations to shed further light on dark matter (DM) subhalo survival at mass scales relevant for gamma-ray DM searches, a topic subject to intense debate nowadays. Specifically, we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c2efc282c72b576c1e07e52deba279c
https://doi.org/10.1093/mnras/stac2921
https://doi.org/10.1093/mnras/stac2921
Autor:
Ángeles Moliné, Jascha A. Schewtschenko, Miguel A. Sánchez-Conde, Alejandra Aguirre-Santaella, Sofía A. Cora, Mario G. Abadi
Publikováno v:
Galaxies, Vol 7, Iss 4, p 80 (2019)
One possible and natural derivation from the collisionless cold dark matter (CDM) standard cosmological framework is the assumption of the existence of interactions between dark matter (DM) and photons or neutrinos. Such a possible interacting dark m
Externí odkaz:
https://doaj.org/article/e37e1d4f98f84952a05f25767e493994
Autor:
Thomas Lacroix, Gaétan Facchinetti, Judit Pérez-Romero, Martin Stref, Julien Lavalle, David Maurin, Miguel A. Sánchez-Conde
Gamma-ray observations have long been used to constrain the properties of dark matter (DM), with a strong focus on weakly interacting massive particles annihilating through velocity-independent processes. However, in the absence of clear-cut observat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af1b68392fb380cffbb76cbe24871199
http://arxiv.org/abs/2203.16440
http://arxiv.org/abs/2203.16440
We present a model for the remnants of haloes that have gone through an adiabatic tidal stripping process. We show that this model exactly reproduces the remnant of an NFW halo that is exposed to a slowly increasing isotropic tidal field and approxim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd45fdeec5ff70de5c8076c7685bead2
Autor:
Ángeles Moliné, Miguel A Sánchez-Conde, Alejandra Aguirre-Santaella, Tomoaki Ishiyama, Francisco Prada, Sofía A Cora, Darren Croton, Eric Jullo, R Benton Metcalf, Taira Oogi, José Ruedas
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2023, 518 (1), pp.157-173. ⟨10.1093/mnras/stac2930⟩
Monthly Notices of the Royal Astronomical Society, 2023, 518 (1), pp.157-173. ⟨10.1093/mnras/stac2930⟩
In this work, we investigate the structural properties, distribution and abundance of ΛCDM dark matter subhaloes using the Phi-4096 and Uchuu suite of N-body cosmological simulations. Thanks to the combination of their large volume, high mass resolu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::650c2c7723f7d0739b140cf764fed1ff
http://arxiv.org/abs/2110.02097
http://arxiv.org/abs/2110.02097
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Around one third of the point-like sources in the Fermi-LAT catalogs remain as unidentified sources (UniDs) today. Indeed, these unIDs lack a clear, univocal association with a known astrophysical source identified at other wavelengths, or to a well-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::59f991f9a7bdf517892d21ba288bcf07
https://doi.org/10.22323/1.395.0493
https://doi.org/10.22323/1.395.0493
Autor:
Julien Lavalle, Gaétan Facchinetti, Martin Stref, Thomas Lacroix, David Maurin, Miguel A. Sánchez-Conde, J. Pérez-Romero
Publikováno v:
PoS
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.571, ⟨10.22323/1.395.0571⟩
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.571, ⟨10.22323/1.395.0571⟩
International audience; Indirect searches with gamma rays set strong constraints on the properties of self-annihilating dark matter particle candidates. Observations of dwarf galaxies and galaxy clusters are especially interesting. Here we revisit th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8db99edf768505509d2e0744a1325974
https://hal.archives-ouvertes.fr/hal-03373327
https://hal.archives-ouvertes.fr/hal-03373327