نتائج البحث - "dark matter: velocity"

1

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2

Recasting direct detection limits within micrOMEGAs and implication for non-standard dark matter scenarios

المؤلفون: Geneviève Bélanger, Alexander Pukhov, Ali Mjallal

المساهمون: Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)

المصدر: 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

مصطلحات موضوعية: Particle physics, Physics and Astronomy (miscellaneous), nucleus: form factor, Dark matter, FOS: Physical sciences, lcsh:Astrophysics, dark matter: direct detection, 01 natural sciences, High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, lcsh:QB460-466, mediation, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, 010306 general physics, numerical calculations, cross section: elastic scattering, Engineering (miscellaneous), Physics, Detection limit, Elastic scattering, 010308 nuclear & particles physics, nucleon, MicroMegas detector, High Energy Physics - Phenomenology, Distribution (mathematics), [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], lcsh:QC770-798, dark matter: velocity, Nucleon

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a10bc19f533b16ca019667efe3698d03
https://doaj.org/article/f55294a0f9ab4ad5bcc2ab26ed052770

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Find this article in full text from ProQuest

3

The large scale structure bootstrap: perturbation theory and bias expansion from symmetries

المؤلفون: Filippo Vernizzi, Massimo Pietroni, Guido D'Amico, Marco Marinucci

المساهمون: Istituto Nazionale di Fisica Nucleare [Parma] (INFN), Istituto Nazionale di Fisica Nucleare, Institut de Physique Théorique - UMR CNRS 3681 (IPHT), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)

المصدر: JCAP
JCAP, 2021, 10, pp.069. ⟨10.1088/1475-7516/2021/10/069⟩

مصطلحات موضوعية: High Energy Physics - Theory, momentum: external, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Galilean invariance, symmetry: space-time, perturbation, gravitation: model, Dark matter, FOS: Physical sciences, Context (language use), hierarchy, dark matter: density, 01 natural sciences, Gravitation, Momentum, nonrelativistic, Theoretical physics, momentum: conservation law, cosmological model: parameter space, 0103 physical sciences, structure, dark energy, bootstrap, 010303 astronomy & astrophysics, perturbation theory, Physics, Conservation law, higher-order: 3, diffeomorphism: invariance, 010308 nuclear & particles physics, Astronomy and Astrophysics, invariance: Galilei, High Energy Physics - Theory (hep-th), Dark energy, Perturbation theory (quantum mechanics), dark matter: velocity, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0138480c0294957e5a3b5e5e98d4a63e
https://hal.archives-ouvertes.fr/hal-03364371

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MOND-like behavior in the Dirac-Milne universe -- Flat rotation curves and mass/velocity relations in galaxies and clusters

المؤلفون: Clément Stahl, Bruce N. Miller, Yohan Dubois, Gabriel Chardin, Giovanni Manfredi

المساهمون: AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), University of Oxford, Memory and Aging Center [San Francisco, CA, États-Unis], University of California [San Francisco] (UC San Francisco), University of California (UC)-University of California (UC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), University of Oxford [Oxford], University of California [San Francisco] (UCSF), University of California-University of California, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique et Chimie des Matériaux de Strasbourg (IPCMS), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS)-Matériaux et nanosciences d'Alsace, Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Strasbourg (UNISTRA)-Réseau nanophotonique et optique, Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Strasbourg (UNISTRA)

المصدر: 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⟩

مصطلحات موضوعية: cosmological model, Cosmology and Nongalactic Astrophysics (astro-ph.CO), media_common.quotation_subject, Dark matter, FOS: Physical sciences, Lambda-CDM model, Astrophysics, dark matter: velocity: dispersion, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, rotation, Cosmology, dark matter, Gravitation, General Relativity and Quantum Cosmology, velocity: dispersion, 0103 physical sciences, MOND, antimatter, cloud, structure, cluster, dark energy, 010303 astronomy & astrophysics, Galaxy rotation curve, media_common, gravitation: surface, Physics, polarization, 010308 nuclear & particles physics, Computer Science::Information Retrieval, formation, nucleosynthesis, Astronomy and Astrophysics, acceleration, redshift, Astrophysics - Astrophysics of Galaxies, Universe, Modified Newtonian dynamics, Space and Planetary Science, gravitation, Astrophysics of Galaxies (astro-ph.GA), Dark energy, cosmology: miscellaneous, galaxy: velocity: dispersion, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], fundamental constant, Astrophysics - Cosmology and Nongalactic Astrophysics

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8357625ab82ca784f86b176e37a7e5e

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Equilibrium axisymmetric halo model for the Milky Way and its implications for direct and indirect dark matter searches

المؤلفون: Mihael Petač

المساهمون: Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)

المصدر: Physical Review D
Physical Review D, American Physical Society, 2020, 102 (12), pp.123028. ⟨10.1103/PhysRevD.102.123028⟩

مصطلحات موضوعية: Milky Way, Dark matter, FOS: Physical sciences, Astrophysics, dark matter: density, 01 natural sciences, Bayesian, flux: time dependence, symmetry: axial, anisotropy: velocity, High Energy Physics - Experiment, dark matter: coupling, High Energy Physics - Experiment (hep-ex), phase space, High Energy Physics - Phenomenology (hep-ph), near detector, 0103 physical sciences, conservation law, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Sensitivity (control systems), 010306 general physics, halo: rotation, Physics, 010308 nuclear & particles physics, dark matter: mass, Galactic Center, scattering: operator, Relative velocity, Coupling (probability), sensitivity, Astrophysics - Astrophysics of Galaxies, Baryon, High Energy Physics - Phenomenology, modulation, halo: model, annihilation, dark matter: heavy, kinematics, Astrophysics of Galaxies (astro-ph.GA), [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], direct detection, Halo, dark matter: velocity, galaxy, velocity dependence, numerical calculations: Monte Carlo, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics and astroparticle physics

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16c869fe14415eade81b7fd8ec525e67
https://hal.archives-ouvertes.fr/hal-02940000/document

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Predicting the dark matter velocity distribution in galactic structures: tests against hydrodynamic cosmological simulations

المؤلفون: Martin Stref, Julien Lavalle, Thomas Lacroix, Emmanuel Nezri, A. Nuñez-Castiñeyra

المساهمون: Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), ANR-18-CE31-0006,GaDaMa,Matière Noire Galactique(2018)

المصدر: JCAP
JCAP, 2020, 10, pp.031. ⟨10.1088/1475-7516/2020/10/031⟩

مصطلحات موضوعية: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Structure formation, Dark matter, galaxy: dark matter, FOS: Physical sciences, Primordial black hole, dark matter: phase space, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, anisotropy, Parameter space, Gravitational microlensing, 01 natural sciences, Galactic dynamics, High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, structure formation, galaxy: mass, numerical calculations, Astrophysics::Galaxy Astrophysics, Physics, 010308 nuclear & particles physics, Astronomy and Astrophysics, Observable, dark matter searches, Astrophysics - Astrophysics of Galaxies, Galaxy, formation: structure, Stars, High Energy Physics - Phenomenology, annihilation, Astrophysics of Galaxies (astro-ph.GA), [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], hydrodynamics, dark matter: velocity, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], black hole: primordial, Astrophysics - Cosmology and Nongalactic Astrophysics

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64b0c9b7799df8b7ff0fb5740853f6da
https://hal.archives-ouvertes.fr/hal-02628073

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Dark matter capture by the Sun: revisiting velocity distribution uncertainties

المؤلفون: Emmanuel Nezri, V. Bertin, A. Nuñez-Castiñeyra

المساهمون: Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)

المصدر: 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⟩

مصطلحات موضوعية: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Dark matter, Inverse transform sampling, FOS: Physical sciences, WIMP: mass, Context (language use), Astrophysics, 01 natural sciences, WIMP: dark matter, High Energy Physics - Phenomenology (hep-ph), benchmark, WIMP, 0103 physical sciences, distribution function, Physics, mass: density, 010308 nuclear & particles physics, Astronomy and Astrophysics, Escape velocity, Astrophysics - Astrophysics of Galaxies, Galaxy, solar, dark matter: capture, High Energy Physics - Phenomenology, Distribution function, Astrophysics of Galaxies (astro-ph.GA), [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], direct detection, history, galaxy, dark matter: velocity, Neutrino, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a29cd63c2dca4609e7404792f6accd0c
https://hal.archives-ouvertes.fr/hal-02188366

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Empirical Determination of Dark Matter Velocities using Metal-Poor Stars

المؤلفون: Jonah Herzog-Arbeitman, Piero Madau, Mariangela Lisanti, Lina Necib

المساهمون: Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris ( IAP ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS )

المصدر: 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〉

مصطلحات موضوعية: Cosmology and Nongalactic Astrophysics (astro-ph.CO), [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Dark matter, Scalar field dark matter, sloan digital sky survey, General Physics and Astronomy, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, High Energy Physics - Phenomenology (hep-ph), accretion, dark matter: halo, star, 0103 physical sciences, structure, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Physics, cross section, 010308 nuclear & particles physics, scattering, Astronomy, Astrophysics - Astrophysics of Galaxies, Accretion (astrophysics), Galaxy, solar, Dark matter halo, Baryon, baryon, High Energy Physics - Phenomenology, Stars, halo: model, kinematics, Astrophysics of Galaxies (astro-ph.GA), [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph], dispersion, direct detection, Halo, Astrophysics::Earth and Planetary Astrophysics, dark matter: velocity, galaxy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d5cea652f584ae8d87ce518dce27aa5
https://hal.archives-ouvertes.fr/hal-01703801

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The Local Dark Matter Distribution from Hydrodynamic Simulations

المؤلفون: 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.

المساهمون: Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), GRAPPA (ITFA, IoP, FNWI)

المصدر: 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

مصطلحات موضوعية: hydrodynamics, Astrophysics::Cosmology and Extragalactic Astrophysics, dark matter: velocity, dark matter: density, galaxy, dark matter: direct detection, numerical calculations, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 7. Clean energy, solar

وصف الملف: application/pdf

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b210fc3f5c4feaafadfc1fb70134c750
https://hal.archives-ouvertes.fr/hal-01669689

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Reconstructing the three-dimensional local dark matter velocity distribution

المؤلفون: Bradley J. Kavanagh, Ciaran A. J. O'Hare

المساهمون: Institut de Physique Théorique - UMR CNRS 3681 (IPHT), Centre National de la Recherche Scientifique (CNRS)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire de Physique Théorique et Hautes Energies (LPTHE), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)

المصدر: 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⟩

مصطلحات موضوعية: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Discretization, dimension: 3, Dark matter, FOS: Physical sciences, dark matter: direct detection, 01 natural sciences, dark matter, Galactic halo, phase space, High Energy Physics - Phenomenology (hep-ph), galaxy: halo, 0103 physical sciences, recoil, Range (statistics), Statistical physics, structure, 010306 general physics, capture, Physics, 010308 nuclear & particles physics, dark matter: mass, parametrization, Dark matter halo, High Energy Physics - Phenomenology, Classical mechanics, halo: model, Phase space, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], Halo, dark matter: velocity, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Parametrization, Astrophysics - Cosmology and Nongalactic Astrophysics

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ec2079af2f1d2fd83a2376735a1f12a
https://hal.archives-ouvertes.fr/hal-01554705

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