[HTML][HTML] Baryon cycles in the biggest galaxies
The universe's biggest galaxies have both vast atmospheres and supermassive central
black holes. This article reviews how those two components of a large galaxy couple and …
black holes. This article reviews how those two components of a large galaxy couple and …
Dark matter self-interactions and small scale structure
We review theories of dark matter (DM) beyond the collisionless paradigm, known as self-
interacting dark matter (SIDM), and their observable implications for astrophysical structure …
interacting dark matter (SIDM), and their observable implications for astrophysical structure …
The dawn of FIMP dark matter: a review of models and constraints
N Bernal, M Heikinheimo, T Tenkanen… - … Journal of Modern …, 2017 - World Scientific
We present an overview of scenarios where the observed Dark Matter (DM) abundance
consists of Feebly Interacting Massive Particles (FIMPs), produced nonthermally by the so …
consists of Feebly Interacting Massive Particles (FIMPs), produced nonthermally by the so …
A face emotion recognition method using convolutional neural network and image edge computing
H Zhang, A Jolfaei, M Alazab - IEEE Access, 2019 - ieeexplore.ieee.org
To avoid the complex process of explicit feature extraction in traditional facial expression
recognition, a face expression recognition method based on a convolutional neural network …
recognition, a face expression recognition method based on a convolutional neural network …
ETHOS–an effective theory of structure formation: dark matter physics as a possible explanation of the small-scale CDM problems
M Vogelsberger, J Zavala… - Monthly Notices of …, 2016 - academic.oup.com
We present the first simulations within an effective theory of structure formation (ETHOS),
which includes the effect of interactions between dark matter and dark radiation on the linear …
which includes the effect of interactions between dark matter and dark radiation on the linear …
Simulations of solitonic core mergers in ultralight axion dark matter cosmologies
B Schwabe, JC Niemeyer, JF Engels - Physical Review D, 2016 - APS
Using three-dimensional simulations, we study the dynamics and final structure of merging
solitonic cores predicted to form in ultralight axion dark matter halos. The classical …
solitonic cores predicted to form in ultralight axion dark matter halos. The classical …
What does the Bullet Cluster tell us about self-interacting dark matter?
A Robertson, R Massey, V Eke - Monthly Notices of the Royal …, 2016 - academic.oup.com
We perform numerical simulations of the merging galaxy cluster 1E 0657-56 (the Bullet
Cluster), including the effects of elastic dark matter scattering. In a similar manner to the …
Cluster), including the effects of elastic dark matter scattering. In a similar manner to the …
Gravitational probes of dark matter physics
MR Buckley, AHG Peter - Physics reports, 2018 - Elsevier
The nature of dark matter is one of the most pressing questions in physics. Yet all our
present knowledge of the dark sector to date comes from its gravitational interactions with …
present knowledge of the dark sector to date comes from its gravitational interactions with …
The Frontier Fields lens modelling comparison project
M Meneghetti, P Natarajan, D Coe… - Monthly Notices of …, 2017 - academic.oup.com
Gravitational lensing by clusters of galaxies offers a powerful probe of their structure and
mass distribution. Several research groups have developed techniques independently to …
mass distribution. Several research groups have developed techniques independently to …
Indirect and direct search for dark matter
M Klasen, M Pohl, G Sigl - Progress in Particle and Nuclear Physics, 2015 - Elsevier
The majority of the matter in the universe is still unidentified and under investigation by both
direct and indirect means. Many experiments searching for the recoil of dark-matter particles …
direct and indirect means. Many experiments searching for the recoil of dark-matter particles …