Results 71 to 80 of about 28,520 (293)

The impact of baryons on the direct detection of dark matter

open access: yes, 2016
The spatial and velocity distributions of dark matter particles in the Milky Way Halo affect the signals expected to be observed in searches for dark matter.
Bailin, Jeremy   +5 more
core   +1 more source

The connection between the host halo and the satellite galaxies of the Milky Way [PDF]

open access: yes, 2016
Many properties of the Milky Way's dark matter halo, including its mass assembly history, concentration, and subhalo population, remain poorly constrained.
Benson, Andrew   +7 more
core   +3 more sources

An In Situ Embedded B‐MOF Sponge With Shape‐Memory for All‐in‐One Diabetic Wound Therapy

open access: yesAdvanced Healthcare Materials, EarlyView.
A smart shape‐memory sponge dressing (P1A3@B‐MOF) is developed for accelerated diabetic wound healing. It achieves pH‐responsive corelease of Zn2+ and salvianolic acid B, synergistically providing antibacterial action, repolarizing macrophages to the M2 phenotype, and promoting angiogenesis.
Hai Zhou   +11 more
wiley   +1 more source

Minimum-entropy Constraints on Galactic Potentials

open access: yesThe Astrophysical Journal
A tracer sample in a gravitational potential, starting from a generic initial condition, phase-mixes toward a stationary state. This evolution is accompanied by an entropy increase, and the final state is characterized by a distribution function (DF ...
Leandro Beraldo e Silva   +5 more
doaj   +1 more source

Grand Rotation Curve and Dark-Matter Halo in the Milky Way Galaxy [PDF]

open access: yesPublications of the Astronomical Society of Japan, 2012
A grand rotation curve of the Milky Way Galaxy was constructed, which covers a wide range of radius from the Galactic Center to $ \sim$ 1 Mpc, and was deconvolved into bulge, disk, and halo components by least-squares fittings. We determined the masses and scale radii of the bulge and disk to be $ {M_{\rm b}}$$ =$ (1.652 $ \pm$ 0.083) $ \times$ 10 ...
openaire   +2 more sources

Subhaloes in Self-Interacting Galactic Dark Matter Haloes

open access: yes, 2012
We present N-body simulations of a new class of self-interacting dark matter models, which do not violate any astrophysical constraints due to a non-power-law velocity dependence of the transfer cross section which is motivated by a Yukawa-like new gauge
Abraham Loeb   +63 more
core   +1 more source

Are there MACHOs in the Milky Way halo? [PDF]

open access: yes, 2002
Microlensing searches aim to detect compact halo dark matter via its gravitational lensing effect on stars within the Large Magellanic Cloud. The most recent results have led to the claim that roughly one fifth of the galactic halo dark matter may be in ...
A. M. Green   +26 more
core   +2 more sources

3D Soft Hydrogels Induce Human Mesenchymal Stem Cells “Deep” Quiescence

open access: yesAdvanced Healthcare Materials, EarlyView.
Three‐dimensional soft hydrogels mimicking the bone marrow niche induce deep quiescence in human mesenchymal stem cells. Unlike 2D culture, 3D matrices halt proliferation, regulate cell‐cycle and quiescence markers, and downregulate mTORC1 signaling, preserving stem cell phenotype and therapeutic potential ex vivo.
David Boaventura Gomes   +11 more
wiley   +1 more source

Semianalytic Modeling of Dark Matter Subhalo Encounters with Thin Stellar Streams: Statistical Predictions for GD-1-like Streams in Cold Dark Matter

open access: yesThe Astrophysical Journal
Stellar streams from disrupted globular clusters are dynamically cold structures that are sensitive to perturbations from dark matter subhalos, allowing them in principle to trace the dark matter substructure in the Milky Way.
Duncan K. Adams   +5 more
doaj   +1 more source

Erratum: Estimating the dark matter halo mass of our Milky Way using dynamical tracers [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
Our paper ‘Estimating the dark matter halo mass of our Milky Way using dynamical tracers’ published in MNRAS, 2015, 453, 377 contained typographic errors in equations (12) and (6) as detailed below. Our code used the correct expressions in both cases; hence, none of our figures or conclusions are affected by these errors.
Wang, W.   +5 more
openaire   +3 more sources

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