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Dark matter

WISPy cold dark matter

WISPy cold dark matter

... In this paper, we shall revisit the misalignment mechanism for both cases: we treat first axion-like particles (ALPs — which may arise as pseudo-Nambu-Goldstone bosons in field theory and appear generically in all string ...

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Dark matter baryons separation at the lowest mass scale: The bullet group

Dark matter baryons separation at the lowest mass scale: The bullet group

... Merging galaxy clusters are unique astrophysical probes of the properties of dark matter (DM), which accounts for the majority of the mass in the Universe. During a cluster merger, the cluster galaxies are ...

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SEARCHING FOR DARK MATTER ANNIHILATION IN THE SMITH HIGH VELOCITY CLOUD

SEARCHING FOR DARK MATTER ANNIHILATION IN THE SMITH HIGH VELOCITY CLOUD

... with dark matter annihilation in the Smith Cloud, we model the Smith Cloud itself according to the spatially extended dark matter profiles described in Section ...Cloud dark ...

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Gravitino dark matter in split supersymmetry with bilinear R parity violation

Gravitino dark matter in split supersymmetry with bilinear R parity violation

... the dark matter density ...stable dark matter ...indirect dark matter detection via gamma rays, electron–positron pairs, neutrinos, ...

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Evidence of Lensing of the Cosmic Microwave Background by Dark Matter Halos

Evidence of Lensing of the Cosmic Microwave Background by Dark Matter Halos

... With this Letter, we demonstrate that CMB observations are now achieving the sensitivity and resolution to provide mass estimates of dark matter halos belonging to galaxy groups and clusters. With the ...

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Gravitino dark matter and neutrino masses in partial split supersymmetry

Gravitino dark matter and neutrino masses in partial split supersymmetry

... Because R-parity is not conserved, the lightest super- symmetric particle (LSP) will be unstable and decay into standard-model particles. This will occur very fast if the LSP is the traditional neutralino, losing it as a ...

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Black hole spin and radio loudness in a Lambda cold dark matter universe

Black hole spin and radio loudness in a Lambda cold dark matter universe

... cold dark matter paradigm and a semi-analytic model of galaxy formation to investigate the spin development of central supermassive black holes (BHs) and its relation to the BH host galaxy ...

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Chaotic motion and the evolution of morphological components in a time dependent model of a barred galaxy within a dark matter halo

Chaotic motion and the evolution of morphological components in a time dependent model of a barred galaxy within a dark matter halo

... the dark matter ...the dark matter halo, and found that tidal debris in cosmological hydrodynamical simulations experience more chaotic evolution than in collisionless ...

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Strong optimized conservative Fermi LAT constraints on dark matter models from the inclusive photon spectrum

Strong optimized conservative Fermi LAT constraints on dark matter models from the inclusive photon spectrum

... various dark matter annihilation and decay final states, Warit Mitthumsiri for his work on the MC simulations, and Eric Charles, Ilias Cholis, Tongyan Lin, Michele Papucci, and Gabrijela Zaharijas for ...

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Modeling of the HerMES submillimeter source lensed by a dark matter dominated foreground group of galaxies

Modeling of the HerMES submillimeter source lensed by a dark matter dominated foreground group of galaxies

... the dark mat- ter content of intermediate redshift halos with high accu- ...projected dark matter fraction of about ...small-scale dark matter ...

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Analytic derivation of non-linear dark matter clustering from the filtering of the primordial density field

Analytic derivation of non-linear dark matter clustering from the filtering of the primordial density field

... the matter content of the ...Hot Dark Matter transfer function, which eliminates power on small and intermedi- ate scales, has to be ...the matter content of the universe is dominated by ...

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Eddington Born Infeld action for dark matter and dark energy

Eddington Born Infeld action for dark matter and dark energy

... Supersymmetric and exotic particles in the standard model are the best candidates for dark matter (for a review see [3]). Several experiments are now being devised for a direct detection of these particles. ...

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Note on bigravity and dark matter

Note on bigravity and dark matter

... for dark matter and dark ...the dark matter/dark energy interpretation still ...as matter or as dark energy, and there exist solutions interpolating between ...

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Updated search for spectral lines from Galactic dark matter interactions with pass 8 data from the Fermi Large Area Telescope

Updated search for spectral lines from Galactic dark matter interactions with pass 8 data from the Fermi Large Area Telescope

... Dark matter in the Milky Way may annihilate directly into γ rays, producing a monoenergetic spectral ...for dark matter annihilation or ...motivated dark matter scenarios and ...

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WIMP dark matter as radiative neutrino mass messenger

WIMP dark matter as radiative neutrino mass messenger

... for dark matter ...fermionic dark matter ...the dark matter candidate and the charged component of ...the dark matter mass is forced to be ...observed dark ...

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Dark Matter in Ultra diffuse Galaxies in the Virgo Cluster from Their Globular Cluster Populations

Dark Matter in Ultra diffuse Galaxies in the Virgo Cluster from Their Globular Cluster Populations

... with that of the massive galaxy M84 and the center of the Virgo cluster itself. These findings, in addition to having a dynamically and spatially (∼ 1 kpc) off-centered nucleus and being extremely elongated, suggest that ...

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"For terror of the deadness beyond": arctic environments and inhuman ecologies in Michelle Paver’s "Dark matter"

"For terror of the deadness beyond": arctic environments and inhuman ecologies in Michelle Paver’s "Dark matter"

... vibrant matter: “the capacity of things—edibles, commodities, storms, metals—not only to impede or block the will of humans but also to act as quasi agents or forces with trajectories, propensities, or tendencies ...

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How robust are predictions of galaxy clustering?

How robust are predictions of galaxy clustering?

... For this comparison we use publicly available galaxy cata- logues produced by two groups who have independently developed semi-analytical models of galaxy formation. Semi-analytical mod- els attempt to calculate the fate ...

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Ly alpha emitting galaxies at z=3 1: L* progenitors experiencing rapid star formation

Ly alpha emitting galaxies at z=3 1: L* progenitors experiencing rapid star formation

... The observed properties of LAEs at z = 3.1 make them the most promising candidates to be high-redshift progenitors of present-day L ∗ galaxies like the Milky Way. Our results suggest that LAEs are observed during the ...

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Delta gravity and dark energy

Delta gravity and dark energy

... of matter is in the form of unknown matter (dark matter, DM) and that the dynamics of the expansion of the Universe is governed by a myste- rious component that accelerates the expansion ...

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