[PDF] Top 20 Towards an improved model of self-interacting dark matter haloes
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Towards an improved model of self-interacting dark matter haloes
... the self-interaction is strong enough for SIDM to be distinct from CDM on small scales (see ...of dark matter (DM) haloes distinctly from CDM and explain the sizes of DM density cores ...the ... See full document
34
How does gas cool in dark matter haloes?
... isolated haloes. Our controlled numerical experiments will be run for haloes having the density profile (for DM particles) of Navarro, Frenk & White (1997) (hereafter NFW), with a range of masses, ... See full document
14
An interacting dark sector and the first gravitational-wave standard siren detection
... cosmological model characterised by a non–standard interacting dark ...CDM model (Di Valentino & Melchiorri 2018), in which the in- clusion of the GW170817 Hubble constant measurement led ... See full document
10
Small-Scale Cosmology “Crisis” and Self-Interacting Right-Handed Neutrino Warm Dark Matter
... [14], self-interactions among WDM right-handed Neutrinos, in minimal exten- sions of the Standard Model, may provide solution to all three problems of the small-scale cosmology, and model more ... See full document
16
An interacting dark sector and the implications of the first gravitational-wave standard siren detection on current constraints
... cosmological model characterized by a non- standard interacting dark ...CDM model (Di Valentino & Melchiorri 2018), in which the inclusion of the GW170817 Hubble constant measurement led ... See full document
9
Search for Boosted Dark Matter Interacting with Electrons in Super-Kamiokande
... dark matter component accounting for most of the dark matter energy density of the ...boosted dark matter can remain consistent with ...boosted dark matter can be ... See full document
9
Dark Matter Halo Mergers and Quasars
... surrounding dark matter ...a model for the creation rate of dark matter haloes, informed by both coagulation theory and the modified excursion set approach with moving ...simple ... See full document
373
nIFTy cosmology: comparison of galaxy formation models
... associating dark matter haloes with galaxies: the HOD (Jing, Mo & Boerner 1998; Cooray & Sheth 2002), as well as the complementary models of the conditional luminosity function (CLF; Yang, Mo ... See full document
31
Observable tests of self-interacting dark matter in galaxy clusters: Cosmological simulations with SIDM and baryons
... Self-interacting dark matter (SIDM) has become an attractive alternative to collisionless cold dark matter (CDM) because it can alleviate tensions between the results of DM-only ... See full document
17
Studying dark matter haloes with weak lensing
... Standard Model of Particle Physics, such as electrons, protons and neutrons, compose only a minor part — about 5% — while the majority of the matter constituents appears to be something new: dark ... See full document
183
Interacting and Non-Interacting Holographic Gas Model of Dark energy in f(G) Gravity
... during late time epochs [25]. Nojiri et al. [26] have discussed some fundamental cosmic issues, like inflation, late-time acceleration, bouncing cosmology and claimed that some modified theories of gravity, like f (R ) , ... See full document
9
Numerical convergence of simulations of galaxy formation: the abundance and internal structure of cold dark matter haloes
... cold dark matter model (see, ...of dark matter haloes is therefore closely related to the observed lu- minosity function of galaxies, and is a central aspect of the- oretical ... See full document
22
The gas fractions of dark matter haloes hosting simulated L^ galaxies are governed by the feedback history of their black holes
... Halo gas, often termed the circumgalactic medium (CGM), is the interface between galaxies and the intergalactic medium (IGM), and acts as reservoir of both the fuel for ongoing star-formation, and of the heavy elements ... See full document
10
Bent by baryons: the low-mass galaxy-halo relation
... on dark matter only simulations for abundance matching is inappropriate and can lead to incorrect ...cold dark matter, but simply to a failure to account for baryonic ...used ... See full document
7
KSVZ axion model with quasidegenerate minima:A unified model for dark matter and dark energy
... first model of this type was the universe multiplication model proposed in ...a model based on nonlocal constraints ...observed dark energy density must be explained by the potential energy of ... See full document
10
Halkola, Aleksi (2007): Gravitational Lensing in Galaxy Cluster Abell 1689. Dissertation, LMU München: Fakultät für Physik
... the haloes of the cluster galaxies in Chapter ...galaxy haloes. Optical traces in the galaxy haloes indicate that the haloes of field galaxies stay roughly isothermal beyond several hundred ... See full document
175
A Model of Dark Matter and Dark Energy Based on Relativizing Newton’s Physics
... of dark matter and dark energy in the universe are among the outstanding open issues of modern ...is dark matter made of?” has not been answered ...particle dark matter ... See full document
26
The Novel Interaction Model of Dark Energy and Dark Matter
... namely Dark Matter and Dark Energy ...novel model gives the sum “attractive force” of all matters in the ...the matter suppresses firstly, sharp inflates sec- ondly, slowly expands ... See full document
6
The light photon, dark matter and the whirling of dark matter, the theory of the birth of universe
... particles Dark Energy mass particles have, original gravitational force in Universe, either existing or ...of Dark Energy forming Dark ...the dark energy particles/Dark matter, ... See full document
28
Jeans that fit : weighing the mass of the Milky Way analogues in the ΛCDM universe
... More recently there have been attempts to test the efficacy of dif- ferent methods in robustly measuring the mass distributions of the MW-like galaxies using spatial and kinematic data. For example, Candlish et al. ... See full document
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