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pro vyhledávání: '"dark matter: velocity"'
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Publikováno v:
European Physical Journal C: Particles and Fields, Vol 81, Iss 3, Pp 1-18 (2021)
Eur.Phys.J.C
Eur.Phys.J.C, 2021, 81 (3), pp.239. ⟨10.1140/epjc/s10052-021-09012-z⟩
European Physical Journal
Eur.Phys.J.C
Eur.Phys.J.C, 2021, 81 (3), pp.239. ⟨10.1140/epjc/s10052-021-09012-z⟩
European Physical Journal
Direct detection experiments obtain 90% upper limits on the elastic scattering cross sections of dark matter with nucleons assuming point-like interactions and standard astrophysical and cosmological parameters. In this paper we provide a recasting o
Publikováno v:
JCAP
JCAP, 2021, 10, pp.069. ⟨10.1088/1475-7516/2021/10/069⟩
JCAP, 2021, 10, pp.069. ⟨10.1088/1475-7516/2021/10/069⟩
We investigate the role played by symmetries in the perturbative expansion of the large-scale structure. In particular, we establish which of the coefficients of the perturbation theory kernels are dictated by symmetries and which not. Up to third or
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0138480c0294957e5a3b5e5e98d4a63e
https://hal.archives-ouvertes.fr/hal-03364371
https://hal.archives-ouvertes.fr/hal-03364371
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 652, pp.A91. ⟨10.1051/0004-6361/202140575⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 652, pp.A91. ⟨10.1051/0004-6361/202140575⟩
Astronomy and Astrophysics-A&A, 2021, 652, pp.A91. ⟨10.1051/0004-6361/202140575⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 652, pp.A91. ⟨10.1051/0004-6361/202140575⟩
Aims.Observational data show that the observed luminous matter is not sufficient to explain several features of the present universe, from gravitational structure formation to the rotational velocities in galaxies and clusters. The mainstream explana
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8357625ab82ca784f86b176e37a7e5e
Autor:
Mihael Petač
Publikováno v:
Physical Review D
Physical Review D, American Physical Society, 2020, 102 (12), pp.123028. ⟨10.1103/PhysRevD.102.123028⟩
Physical Review D, American Physical Society, 2020, 102 (12), pp.123028. ⟨10.1103/PhysRevD.102.123028⟩
We for the first time provide self-consistent axisymmetric phase-space distribution models for the Milky Way's dark matter (DM) halo which are carefully matched against the latest kinematic measurements through Bayesian analysis. By using broad prior
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16c869fe14415eade81b7fd8ec525e67
https://hal.archives-ouvertes.fr/hal-02940000/document
https://hal.archives-ouvertes.fr/hal-02940000/document
Publikováno v:
JCAP
JCAP, 2020, 10, pp.031. ⟨10.1088/1475-7516/2020/10/031⟩
JCAP, 2020, 10, pp.031. ⟨10.1088/1475-7516/2020/10/031⟩
Reducing theoretical uncertainties in Galactic dark matter (DM) searches is an important challenge as several experiments are now delving into the parameter space relevant to popular (particle or not) candidates. Since many DM signal predictions rely
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64b0c9b7799df8b7ff0fb5740853f6da
https://hal.archives-ouvertes.fr/hal-02628073
https://hal.archives-ouvertes.fr/hal-02628073
Publikováno v:
JCAP
JCAP, 2019, 12 (12), pp.043. ⟨10.1088/1475-7516/2019/12/043⟩
JCAP, 2019, 12, pp.043. ⟨10.1088/1475-7516/2019/12/043⟩
JCAP, 2019, 12 (12), pp.043. ⟨10.1088/1475-7516/2019/12/043⟩
JCAP, 2019, 12, pp.043. ⟨10.1088/1475-7516/2019/12/043⟩
Among the different strategies aiming to detect WIMP dark matter (DM), a neutrino signal coming from the Sun would be a smoking gun. This possibility relies on the DM capture by the Sun driven by the local DM distribution assumptions: the local mass
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a29cd63c2dca4609e7404792f6accd0c
https://hal.archives-ouvertes.fr/hal-02188366
https://hal.archives-ouvertes.fr/hal-02188366
Publikováno v:
Phys.Rev.Lett.
Phys.Rev.Lett., 2018, 120 (4), pp.041102. ⟨10.1103/PhysRevLett.120.041102⟩
Physical Review Letters
Physical Review Letters, American Physical Society, 2018, 120 (4), pp.041102. ⟨10.1103/PhysRevLett.120.041102⟩
Phys.Rev.Lett., 2018, 120 (4), pp.041102. 〈10.1103/PhysRevLett.120.041102〉
Phys.Rev.Lett., 2018, 120 (4), pp.041102. ⟨10.1103/PhysRevLett.120.041102⟩
Physical Review Letters
Physical Review Letters, American Physical Society, 2018, 120 (4), pp.041102. ⟨10.1103/PhysRevLett.120.041102⟩
Phys.Rev.Lett., 2018, 120 (4), pp.041102. 〈10.1103/PhysRevLett.120.041102〉
The Milky Way dark matter halo is formed from the accretion of smaller subhalos. These sub-units also harbor stars---typically old and metal-poor---that are deposited in the Galactic inner regions by disruption events. In this Letter, we show that th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d5cea652f584ae8d87ce518dce27aa5
https://hal.archives-ouvertes.fr/hal-01703801
https://hal.archives-ouvertes.fr/hal-01703801
Autor:
Bozorgnia, N., Calore, F., Schaller, M., Lovell, M., Bertone, G., Frenk, C.S., Crain, R.A., Navarro, J.F., Schaye, J., Theuns, T., Kim, Y., Lindner, A., Semertzidis, Y.K.
Publikováno v:
12th Patras Workshop on Axions, WIMPs and WISPs
12th Patras Workshop on Axions, WIMPs and WISPs, Jun 2016, Jeju Island, South Korea. pp.14-17, ⟨10.3204/DESY-PROC-2009-03/Bozorgnia_Nassim⟩
Proceedings of the 12th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2016: June 20-24, 2016 : Jeju Island, South Korea, 14-17
STARTPAGE=14;ENDPAGE=17;TITLE=Proceedings of the 12th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2016
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 14-17 (2017). doi:10.3204/DESY-PROC-2009-03/Bozorgnia_Nassim
Bozorgnia, Nassim "The Local Dark Matter Distribution from Hydrodynamic Simulations" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20-2016-06-24, Jeju Island
Bozorgnia, Nassim "The Local Dark Matter Distribution from Hydrodynamic Simulations" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20-2016-06-24, Jeju Island12th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2016, Jeju Island, South Korea, 2016-06-20-2016-06-24
12th Patras Workshop on Axions, WIMPs and WISPs, Jun 2016, Jeju Island, South Korea. pp.14-17, ⟨10.3204/DESY-PROC-2009-03/Bozorgnia_Nassim⟩
Proceedings of the 12th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2016: June 20-24, 2016 : Jeju Island, South Korea, 14-17
STARTPAGE=14;ENDPAGE=17;TITLE=Proceedings of the 12th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2016
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 14-17 (2017). doi:10.3204/DESY-PROC-2009-03/Bozorgnia_Nassim
Bozorgnia, Nassim "The Local Dark Matter Distribution from Hydrodynamic Simulations" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20-2016-06-24, Jeju Island
Bozorgnia, Nassim "The Local Dark Matter Distribution from Hydrodynamic Simulations" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotron : 2017 ; PATRAS 2016 : 12th "Patras" Workshop on Axions, WIMPs and WISPs, 2016-06-20-2016-06-24, Jeju Island12th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2016, Jeju Island, South Korea, 2016-06-20-2016-06-24
Bozorgnia, Nassim "The Local Dark Matter Distribution from Hydrodynamic Simulations" in 12th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2016 / Kim, Younglm, Lindner, Axel, Semertzidis, Yannis K. (eds.), Verlag Deutsches Elektronen-Synchrotr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b210fc3f5c4feaafadfc1fb70134c750
https://hal.archives-ouvertes.fr/hal-01669689
https://hal.archives-ouvertes.fr/hal-01669689
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2016, 94 (12), pp.123009. ⟨10.1103/PhysRevD.94.123009⟩
Physical Review D
Physical Review D, American Physical Society, 2016, 94 (12), pp.123009. ⟨10.1103/PhysRevD.94.123009⟩
Phys.Rev.D, 2016, 94 (12), pp.123009. ⟨10.1103/PhysRevD.94.123009⟩
Physical Review D
Physical Review D, American Physical Society, 2016, 94 (12), pp.123009. ⟨10.1103/PhysRevD.94.123009⟩
Directionally sensitive dark matter (DM) direct detection experiments present the only way to observe the full three-dimensional velocity distribution of the Milky Way halo local to Earth. In this work we compare methods for extracting information ab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ec2079af2f1d2fd83a2376735a1f12a
https://hal.archives-ouvertes.fr/hal-01554705
https://hal.archives-ouvertes.fr/hal-01554705