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A fraction of the dark matter in the solar neighborhood might be composed of non-galactic particles with speeds larger than the escape velocity of the Milky Way. The non-galactic dark matter flux would enhance the sensitivity of direct…

高能物理 - 唯象学 · 物理学 2021-10-22 Gonzalo Herrera , Alejandro Ibarra

We calculate the contribution of extragalactic dark matter to the local dark matter density and flux in the Milky Way. By analyzing the Galactic escape velocity as a function of direction, we establish the criterion for separating dark…

高能物理 - 唯象学 · 物理学 2025-10-20 Shokhruz Kakharov , Abraham Loeb

In some scenarios, the dark matter particle predominantly scatters inelastically with the target, producing a heavier neutral particle in the final state. In this class of scenarios, the reach in parameter space of direct detection…

高能物理 - 唯象学 · 物理学 2023-04-19 Gonzalo Herrera , Alejandro Ibarra , Satoshi Shirai

We use the APOSTLE suite of cosmological hydrodynamical simulations of the Local Group to examine the high speed tail of the local dark matter velocity distribution in simulated Milky Way analogues. The velocity distribution in the Solar…

星系天体物理 · 物理学 2024-03-26 Isabel Santos-Santos , Nassim Bozorgnia , Azadeh Fattahi , Julio F. Navarro

The velocity distribution of the dark matter particles on the outskirts of the Solar System remains unclear. We suggest to determine it using experimentally found properties of the oldest halo objects. Indeed, the oldest halo stars and…

高能天体物理现象 · 物理学 2015-05-27 Anton N. Baushev

Exotic dark matter together with the vacuum energy (associated with the cosmological constant) seem to dominate the Universe. Thus its direct detection is central to particle physics and cosmology. Supersymmetry provides a natural dark…

天体物理学 · 物理学 2008-11-26 J. D. Vergados , D. Owen

If dark matter (DM) is composed by particles which are non-gravitationally coupled to ordinary matter, their annihilations or decays in cosmic structures can result in detectable radiation. We show that the most powerful technique to detect…

宇宙学与河外天体物理 · 物理学 2015-06-24 Marco Regis , Jun-Qing Xia , Alessandro Cuoco , Enzo Branchini , Nicolao Fornengo , Matteo Viel

Dark matter comprises the bulk of the matter in the universe but its particle nature and cosmological origin remain mysterious. Knowledge of the dark matter density distribution in the Milky Way Galaxy is crucial to both our understanding…

High-velocity particles ( $v>v_\mathrm{esc}$) in the Milky Way are rare but nonetheless important to characterize due to their impact on dark matter (DM) direct detection experiments. We select halos similar in mass to the Milky Way in a…

星系天体物理 · 物理学 2025-02-26 Aidan DeBrae , Peter Behroozi , Nicolas Garavito-Camargo

Exotic dark matter together with the vacuum energy (associated with the cosmological constant) seem to dominate the Universe. Thus its direct detection is central to particle physics and cosmology. Supersymmetry provides a natural dark…

天体物理学 · 物理学 2010-11-19 J. D. Vergados , D. Owen

We show that subhalos falling into the Milky Way create a flow of tidally-stripped debris particles near the galactic center with characteristic velocity behavior. In the Via Lactea-II N-body simulation, this unvirialized component…

宇宙学与河外天体物理 · 物理学 2013-01-03 Mariangela Lisanti , David N. Spergel

A small admixture of dark matter gravitationally bound to the proto-Solar gas cloud could be adiabatically contracted into Earth-crossing orbits with a local density comparable to (or even exceeding) the Galactic halo density. We show that…

高能物理 - 唯象学 · 物理学 2020-07-23 Noah B. Anderson , Angelina Partenheimer , Timothy D. Wiser

The dark matter of our galactic halo may be constituted by elementary particles that interact weakly with ordinary matter (WIMPs). In spite of the very low counting rates expected for these dark matter particles to scatter off nuclei in a…

高能物理 - 唯象学 · 物理学 2007-05-23 Paolo Gondolo

A sample of 11 thousand galaxies with radial velocities V_ LG < 3500 km/s is used to study the features of the local distribution of luminous (stellar) and dark matter within a sphere of radius of around 50 Mpc around us. The average…

宇宙学与河外天体物理 · 物理学 2015-06-04 I. D. Karachentsev

The local density of dark matter is an important quantity. On the one hand, its value is needed for dark matter direct detection searches. On the other hand, a precise and robust determination of the local dark matter density would help us…

星系天体物理 · 物理学 2020-05-20 Pablo F. de Salas

The Milky Way Galaxy contains a large, spherical component which is believed to harbor a substantial amount of unseen matter. Recent observations indirectly suggest that as much as half of this ``dark matter'' may be in the form of old,…

天体物理学 · 物理学 2009-10-12 B. R. Oppenheimer , N. C. Hambly , A. P. Digby , S. T. Hodgkin , D. Saumon

We consider the direct detection of WIMPs reaching the Earth from outside the Milky Way. If these WIMPs form a distinct population they will, although of much lower flux than typical galactic halo WIMPs, have a number of features which…

天体物理学 · 物理学 2009-11-06 Katherine Freese , Paolo Gondolo , Leo Stodolsky

Dark matter in the halos surrounding galaxy groups and clusters can annihilate to high-energy photons. Recent advancements in the construction of galaxy group catalogs provide many thousands of potential extragalactic targets for dark…

宇宙学与河外天体物理 · 物理学 2018-05-07 Mariangela Lisanti , Siddharth Mishra-Sharma , Nicholas L. Rodd , Benjamin R. Safdi , Risa H. Wechsler

Exotic dark matter together with dark energy or cosmological constant seem to dominate in the Universe. An even higher density of such matter seems to be gravitationally trapped in our Galaxy. The nature of dark matter can be unveiled only,…

核理论 · 物理学 2009-09-29 J. D. Vergados

We use FIRE-2 zoom simulations of Milky Way size disk galaxies to derive easy-to-use relationships between the observed circular speed of the Galaxy at the Solar location, $v_\mathrm{c}$, and dark matter properties of relevance for direct…

星系天体物理 · 物理学 2024-08-15 Patrick G. Staudt , James S. Bullock , Michael Boylan-Kolchin , David Kirkby , Andrew Wetzel , Xiaowei Ou
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